Welcome to the CAP2023 Indico site. This site is being used for abstract submission and congress scheduling. Post-deadline poster abstracts will be accepted until May 22, 2023. The Congress program can be seen by selecting "Timetable" in the left menu. Congress registration is now open using the link in the left menu.
Bienvenue au site web Indico pour ACP2023. Ce site servira à la soumission de résumés et à la préparation de l'horaire. Les résumés d'affiches après la date limite seront acceptés jusqu'au 22 mai 2023. Le programme du congrès peut être consulté en sélectionnant "Timetable" dans le menu de gauche. L'inscription au congrès est maintenant ouverte en utilisant le lien dans le menu de gauche.
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Panel with Dr. Ania Harlick, Dr. Henry Shum, Dr. Nomaan X, Dr. Sabrina Leslie, and Dr. Sanjeev Seahra
Life as a physicist can take you many directions; just in academia, there are many different fields and positions one might end up in. On this panel, we hear about physicists of many walks of life and different stages of their careers for some insight of what the future might hold for you as a physicist, and the obstacles that may come. The panelists range from postdoc to head of department; a broad scope that should cover everyone's interest! The panelists will introduce themselves along with their careers, and then participants will have the chance to ask questions to the panelist(s) of their choice.
This is a COVID-safe event; all participants must wear a face mask.
A presentation/workshop by Dr. Stephen Heard
As an author of a scientific paper, you face a bewildering array of options for publication. There are thousands of journals: some very general, and some narrow in scope; some well-known, and some obscure. The situation is complicated even further by the recent proliferation of “predatory” journals and by an escalation in publishing costs. Dr. Heard will discuss some of the factors one might consider in choosing a journal. Participants will then work in small groups to evaluate journals and consider strategy for publishing a paper.
This is a COVID-safe event; all participants must wear a face mask.
Dr. Stephen Heard is a Professor of Biology at the University of New Brunswick, and the author of The Scientist’s Guide to Writing: How to Write More Easily and Effectively Throughout Your Scientific Career (Princeton University Press; 2nd ed. 2022). He has published over 90 scientific papers and served as a journal Associate Editor for more than 20 years.
While it is considered to be one of the most promising hints of new physics beyond the Standard Model, dark matter is as yet known only through its gravitational influence on astronomical and cosmological observables. I will discuss our current best evidence for dark matter’s existence as well as the constraints that astrophysical probes can place on its properties while highlighting some tantalizing anomalies that could indicate non-gravitational dark matter interactions. Future observations, along with synergies between astrophysical and experimental searches, have the potential to illuminate dark matter’s fundamental nature and its influence on the evolution of matter in the cosmos from the first stars and galaxies to today.
Hyperbolic lattices are a new form of synthetic quantum matter in which particles effectively hop on a discrete tiling of two-dimensional hyperbolic space, a non-Euclidean space of negative curvature. Hyperbolic tilings were studied by the British-Canadian geometer H.S.M. Coxeter and popularized through art by M.C. Escher. Recent experiments in circuit quantum electrodynamics and electric circuit networks have demonstrated the coherent propagation of wave-like excitations on hyperbolic lattices. In this talk, I will survey a few of the many exciting directions opened up by this new field, including generalizations of Bloch band theory for hyperbolic lattices, hyperbolic topological materials, and tabletop simulations of the AdS/CFT correspondence.
The Standard Model (SM) of particle physics has been very successful in describing the elementary particles and their interactions. The search for neutrinoless double-beta decay ($0\nu\beta\beta$) offers a way to probe for physics beyond the SM. Observation of $0\nu\beta\beta$ would unambiguously demonstrate violation of lepton number. Additionally, it could also help explain the observed baryon asymmetry in the universe, validate the Majorana nature of neutrinos, and probe new mass generation mechanisms up to the GUT scale. The proposed nEXO experiment will search for $0\nu\beta\beta$ decay in $^{136}$Xe with a projected half-life sensitivity exceeding $10^{28}$ years at the $90\%$ confidence level. nEXO will employ a liquid xenon (LXe) Time Project Chamber (TPC) filled with 5 tonnes of Xe enriched to $\sim90\%\;^{136}$Xe. In parallel, new avenues are being investigated for future upgrades to nEXO with the aim to suppress backgrounds obscuring the $0\nu\beta\beta$ signal. One approach is the extraction and identification of the $\beta\beta$-decay daughter Ba ion, also known as Ba tagging, which will ensure classification of an event as a $\beta\beta$ event irrefutably. Groups at McGill University and TRIUMF are developing an accelerator driven ion source to implant radioactive ions inside a volume of LXe, for subsequent ion extraction using methods under development by other groups within the nEXO collaboration. In the first phase of this development, ions will be extracted using an electrostatic probe for subsequent identification using $\gamma$ spectroscopy. The motivation for the project, the experimental apparatus, and recent updates will be presented along with planned measurements.
Radioactivity in particulates contributes significantly to the background in ultra-low background experiments. The alpha generated from dust provides a degraded energy signal on the detector that mimics low-energy nuclear recoil events, which is background to rare event particle detectors, especially dark matter search experiments. A particulate cleaning station, which includes controlled gas flow on the material surface, a flowmeter, an optical microscope, and a profilometer to scan the surface, has been developed and used to study the cleaning efficiency of dust with various speeds of gas. In this talk, the hardware of the system, the analysis technique, and the cleaning efficiency of different materials and sizes of dust with various gas speeds will be presented.
LoLX is a small scale R&D experiment, hosted at McGill University, which aims to study the properties of liquid xenon (LXe) scintillation light and characterize Cherenkov light emission in LXe with cutting-edge photo-detection technology. It supports next-generation rare-decay experiments, such as nEXO, which will search for neutrinoless double-beta decay in LXe. Interactions in nEXO produce scintillation light in the vacuum ultraviolet (VUV), and the photo-detection technology of choice are silicon photomultipliers (SiPMs), which have a high efficiency in this region, as well as exceptional gain.
The previous detector design included 96 Hamamatsu VUV4 SiPMs in a cylindrical geometry. Optical filters are used to separate Cherenkov and scintillation light produced by a radioactive beta source. In this talk we will present LoLX², the new cubic version of LoLX, which addresses a few issues encountered in its first iteration.
LoLX² will assess the performance of two types of SiPMs, Hamamatsu VUV4 and FBK HD3. It will deploy 40 of each type as well as a VUV-sensitive photomultiplier tube (PMT), which serves as a benchmark for SiPM photo-detection efficiency in VUV. We will give an overview of the new LoLX inner detector designed at TRIUMF, its assembly and the testing of the FBK HD3 SiPMs.
I present studies on a deep convolutional autoencoder originally designed to remove electronic noise from a p-type point contact high-purity germanium (HPGe) detector. With their intrinsic purity and excellent energy resolutions, HPGe detectors are suitable for a variety of rare event searches such as neutrinoless double-beta decay, dark matter candidates, and other exotic physics. However, noise from the readout electronics can make identifying events of interest more challenging. At lower energies, where the signal-to-noise ratio is small, distinguishing signals from backgrounds can be particularly difficult.
I demonstrate that a deep convolutional autoencoder can denoise pulses while preserving the underlying pulse shape well. Results show that a deep learning-based approach is more effective than traditional denoising methods. I also present several studies on how the use of this autoencoder can lead to better physics outcomes through improvements in the energy resolution and better background rejection. Finally, I highlight extensions of this research that our group is working on and show how our methods are broadly applicable to the particle astrophysics community.
nEXO is a proposed tonne-scale experiment which aims to search for neutrinoless double beta ($0\nu\beta\beta$) decay in the isotope $^{136}$Xe. The observation of $0\nu\beta\beta$ decay would demonstrate lepton number violation in weak processes and the Majorana nature of neutrinos. This would be an explicit signature of physics beyond the Standard Model and also may provide insight into the observed matter-antimatter asymmetry in the Universe. nEXO is being designed to investigate this rare decay with a projected half-life sensitivity that is greater than $10^{28}$ years at the 90% confidence level.
In order to reduce the impact of cosmogenic backgrounds, the experiment is anticipated to be located at SNOLAB, an underground laboratory located two kilometres below the surface. The xenon-filled Inner Detector is designed to be located at the centre of a water tank to shield against radioactive backgrounds and to tag passing cosmogenic muons. This 12.3 m in diameter and 12.8 m in height tank, which is filled with 1.5 kilotonnes of ultra-pure deionized water and instrumented with an array of 8-inch photomultiplier tubes (PMTs), constitutes the Outer Detector. The PMTs will be used to veto potential background events in the Inner Detector that may be introduced by spallation neutrons from passing cosmic muons and other secondary particles.
A calibration system is being developed for nEXO's Outer Detector. The aim of this system is to calibrate the timing properties of the PMT's readout system and monitor the optical properties of the water. I will discuss the design implemented for calibrating the Outer Detector by analyzing the result of a GPU-accelerated ray-tracing software (Chroma) as well as considering the different strategies currently used by other similar experiments.
The interpretation of experimental results in particle physics is complicated by the fact that essentially all experimental probes of short distance physics are complex multi-scale processes, and so our ability to interpret experiments depends on our ability to factorize the physics at different distance scales. A simple example is the factorization of hadronic cross sections into short-distance scattering amplitudes and long-distance parton distribution functions, but for more complex situations with additional scales the issue of factorization can be significantly more involved.
Effective Field Theory (EFT) is a general approach in which only the degrees of freedom relevant at a particular length scale are included as degrees of freedom in the theory, and provides a systematically improvable approach to factorization. For collider physics, the appropriate EFT goes under the name of “Soft-Collinear Effective Theory” (SCET). In this talk I’ll discuss a recent, simple formalism for SCET and discuss its application to the study of power corrections to various processes.
The instability of the vacuum in the presence of a strong static electric field that creates charged pairs is Schwinger pair production. In this talk we describe the classical field theory of pair creation using non-hermitian quantum mechanics. The Klein-Gordon equation in 1+1 dimensions in the presence of a constant electric field with an ansatz $\phi(x,t) = e^{-\mathrm{i}\omega t}\phi_{\omega}(x)$, can be mapped to an effective time independent Schr\"{o}dinger equation with a shifted inverted harmonic oscillator (IHO) potential. In this talk we address the question of implementing appropriate long distance physics (boundary condition at infinity) for the IHO that describes pair production using the philosophy of point particle effective field theory (PPEFT). The point particle effective action describes the local interaction of the high energy source. To the leading order, it amounts to adding a complex Dirac delta function at large distances which then fixes appropriate boundary condition for the wavefunction of the IHO at large distances in a renormalization group (RG) invariant way, that describes particle production. We derive Schwinger's pair production rate using the imaginary part of the point particle effective action that renders the emission probability RG invariant.
The Eguchi-Hanson-AdS_5 family of spacetimes are a class of static, geodesically complete, asymptotically locally AdS_5 soliton solutions of the vacuum Einstein equations with a negative cosmological constant. They have negative mass and are parameterized by an integer p ≥ 3 with a conformal boundary with spatial topology L(p, 1). In this talk, I will introduce mode solutions of the scalar wave equation on this background and show that the geometry admits a normal mode spectrum. In addition, I will also discuss other geometric properties of these soliton spacetimes.
We study the quantum-classical Einstein equation from a Hamiltonian perspective where the classical gravitational phase space variables and matter state evolve self-consistently. Applied to cosmology, we show that the resulting equations with a quantized massive scalar field permit exact semiclassical static universes, where the curvature and cosmological constant $\Lambda$ arise as discrete values associated to the eigenstates of the scalar field. Linear stability analysis reveals stable and unstable modes that are functions of $\Lambda$, and independent of the size and curvature of the static universe. The unstable mode leads to an inflating "emergent" universe. We also show numerically that the classical and quantum-classical evolutions agree at late times.
In this talk, we present a novel approach to fully renormalize observables such as theoretical predictions for cross sections and decay rates in particle physics. While renormalization techniques have been utilized to absorb infinities, the theoretical expressions for observables are still not fully renormlazed as they contain dependence on arbitrary subtraction schemes and scales. We resolve this to achieve full renormalization based on a new principle termed as the Principle of Observable Effective Matching (POEM) to simultaneously gain both scale and scheme independence. We illustrate this with an example of the total cross section of the electron positron to hadrons whereby we utilize 3- and 4-loop MS scheme expressions via perturbative Quantum Chromodynamics (pQCD). With POEM and a process termed as Effective Dynamical Renormalization,we fully renormalize these expressions. We obtain prediction of 1.052431+0.0006−0.0006 at Q=31.6GeV, which is in excellent agreement with the experimental value of Rexpe+e−=1.0527+0.005−0.005.
We really understand a phenomenon in science when we can use it to make something new. This interplay between fundamental science and new materials is particularly vibrant in the highly interrelated fields of biological physics and soft materials, where a confluence of experimental techniques and theoretical approaches meet to address fundamental questions. What is a gel? How do macromolecules, such as proteins and DNA, function in the crowded and confined environment of a cell? What role do motor-driven "active" processes play in transporting material in a cell? And what role do hydrodynamic interactions (the fluid-mediated interaction between macromolecules) play? I will try to paint a picture that motivates these questions.
Magnetic resonance imaging (MRI) is a non-invasive diagnostic tool that uses magnetic fields and radio waves to create detailed images of the body's internal structures. This lecture introduces MRI and explains the physical principles behind the formation of images from signals derived from the magnetic moments of 1H nuclei.
The lecture will discuss the fundamental concepts of MRI, including nuclear magnetic resonance (NMR). NMR is the underlying physical phenomenon that allows MRI to work and involves the interaction of magnetic fields with the atomic nuclei in the body's tissues.
Next, the lecture explains how strong magnetic fields are used in MRI. A magnetic field aligns the magnetic moments of the atomic nuclei in the body's tissues, which can then be excited with radio frequency (RF) fields. The excited nuclei then emit RF signals that are picked up by the MRI's detectors, known as radio frequency coils. Linear gradients in the magnetic field are used to spatially encode the detected RF signals so that images can be formed using the Fourier Transform.
Different sources of contrast in images will be introduced, including T1, T2, and proton density. Examples of how each of these highlights different properties of the body's tissues will be presented.
Safety considerations for MRI will be briefly discussed. Finally, some applications of MRI in medicine will be presented, including its use in cancer, neurological disorders, and musculoskeletal injuries.
Overall, this lecture briefly introduces the physics involved in MRI image generation. It is intended for anyone interested in learning more about this important diagnostic tool.
Aside from the lightest elements, hydrogen, helium and some lithium, which were formed in the big bang, the vast majority of the elements around us were (and are) formed in stars, through chains of nuclear reactions and decays. While the general picture of how the various elements are formed is mostly complete, constructing a detailed understanding of element formation remains an active area of research. This includes building an understanding of the origin of elements heavier than iron, formed mainly in chains of neutron captures and beta decays such as the rapid and slow neutron capture processes. Other active areas of investigation include the formation of elements, both heavier and lighter in hydrogen, in stellar explosions such as novae, x-ray bursts, and supernovae. These scenarios typically involve rapid chains of proton or alpha capture reactions followed by beta decays.
Forming a complete understanding of stellar nucleosynthesis requires complex modelling of stellar processes, and a key ingredient in these models are the rates of the nuclear reactions involved. In turn, constraining these rates requires input from nuclear physics, including laboratory measurements of important reactions using stable and radioactive beam facilities. In this talk, I will discuss some of the forefront techniques used to understand stellar nuclear reactions through accelerator-based measurements, including both direct and indirect measurements. As illustrative examples, I will discuss the results of some recent experiments exploiting these techniques, as well as future efforts on the horizon. I will also present some of the latest developments in experiment design and detector technology, which will be applied to future measurements.
Bound-state $\beta$-decay ($\beta_b^-$-decay) is a radically transformative decay mode that can change the stability of a nucleus and generate temperature- and density-dependent decay rates. In this decay mode the $\beta$-electron is created directly in a bound atomic orbital of the daughter nucleus instead of being emitted into the continuum, so the decay channel is only significant in almost fully stripped ions during extreme astrophysical conditions. The $\beta_b^-$-decay of $^{205}\text{Tl}^{81+}$ could influence our understanding of the production of $^{205}\text{Pb}$, a short-lived radioactive (SLR, 17.3 Myr) nucleus that is fully produced by the s-process in stars. In the context of the early Solar system, SLRs are defined by half-lives of 0.1-100 My and their abundance in meteorites can be used to constrain the formation of the Solar System [1]. Historically, it has been noted that thermal population of the 2.3 keV state of $^{205}\text{Pb}$ in stellar conditions could dramatically reduce the abundance of s-process $^{205}\text{Pb}$ by speeding up the EC-decay to $^{205}\text{Tl}$. This destruction of $^{205}\text{Pb}$ is potentially balanced by the $\beta_b^-$-decay of $^{205}\text{Tl}^{81+}$ [2]. Currently, a theoretical prediction for the half-life of fully stripped $^{205}\text{Tl}$ is used in stellar models, but given the importance of the $^{205}\text{Pb}$/$^{204}\text{Pb}$ chronometer, a measurement of the $\beta_b^-$-decay for $^{205}\text{Tl}^{81+}$ was conducted at the GSI Heavy Ion Facility in March 2020. A $^{205}\text{Tl}^{81+}$ beam was stored in the Experimental Storage Ring, and the growth of $^{205}\text{Pb}^{81+}$ daughters with storage time was directly attributable to the $\beta^-_b$-decay channel. The authors will report a preliminary measured half-life and detail how this half-life can be used to more accurately predict the $^{205}\text{Pb}$ abundance in the early Solar System.
[1] M. Lugaro, et al. Progress in Particle and Nuclear Physics, 102:1–47, 2018.
[2] K. Yokoi, et al. Astronomy and Astrophysics, 145:339–346, 1985.
Nuclear pairing, i.e., the tendency of nucleons to form pairs, has important consequences to the physics of neutron star crusts and heavy nuclei. While the pairing found in nuclei typically happens between identical nucleons and in singlet states, recent investigations have shown that certain heavy nuclei can exhibit triplet and mixed-spin pairing correlations in their ground states. In this talk, I will present new investigations on the effect of nuclear deformation on these novel superfluids. Signatures of these pairing effects can be directly seen in nuclear experiments on spectroscopic quantities and two-particle transfer direct reaction cross sections. Indirectly, pairing correlations of nuclear superfluidity can be probed in cold-atomic experiments utilizing Feshbach resonances. On that note, preliminary results on phenomenological investigations of $s$- and $p$-wave pairing in cold-atomic gases will also be discussed.
The slow (s) and rapid (r) neutron capture processes have long been considered to produce nearly the entirety of elements above Fe. Under further scrutiny, when comparing expected s-process and r-process yields with spectroscopic data, inconsistencies in abundance arise in the Z=40 region. These differences are expected to be attributable to the intermediate (i) neutron capture process. Sensitivity studies have shown that the intermediate neutron-capture process follows reaction pathways through experimentally accessible neutron-rich nuclei, providing opportunities to constrain the neutron capture rates that define them. Of these exotic nuclei, $^{90}$Sr provides a strong case in providing new information on i-process abundances.
I will discuss the $\beta$-Oslo analysis of $^{91}$Sr to reduce uncertainties in the $^{90}$Sr(n,$\gamma$)$^{91}$Sr reaction, measured via the $\beta$-decay of $^{91}$Rb into $^{91}$Sr with the SuN total absorption spectrometer at the NSCL in 2018. By simultaneously measuring both $\gamma$-ray and excitation energies, a coincidence matrix was produced to perform the Oslo analysis, providing experimental information on the Nuclear Level Density (NLD) and $\gamma$-ray Strength Functions ($\gamma$SF), two critical components in limiting the uncertainty of the neutron capture cross section when it cannot be directly measured. This constrained uncertainty will allow us to better characterize the contribution of $^{90}$Sr to the i process and make progress in explaining observed abundances in suspected i-process stellar environments.
The impact of the coronavirus disease of 2019 (COVID-19) on secondary education continues to disrupt and profoundly affect student learning and success at post-secondary institutions. Many university instructors have noted and reported that there has emerged a significant gap between course instructor expectations and students’ abilities for pandemic cohorts of students. Urgent consideration must be given as to how best to support these and similarly affected incoming cohorts of undergraduate students. This talk examines and proposes resources to support instructors on how to teach students post covid and invites discussion and suggestions on the way forward.
Review sessions, designed to provide students additional practice and support for summative assessments, help with prioritizing course material. With multitude of resources available online, the importance shifts to ensuring that students are engaged, inspired, aware of the level at which they will be tested, and able to assess their own knowledge. In courses that have problem solving skills as one of the course outcomes, the ability to so apply the knowledge is especially important.
We have explored an inclusion of various competitive setups that all emphasized learning and growth as the main goal, focused on the process and quality of work, gave everyone equal chance of winning and had no profound effect on students’ grade in the course. While the context was always light-hearted and fun, the content of the questions was tightly related to the course material, allowing for self-evaluation and self-reflection, and had full intention of preparing students for the summative assessment.
All discussed activities were designed for electromagnetism courses intended for different audiences – from algebra-based service courses, through those intended for students in engineering, to senior physics majors, showing that the technique, supported by the appropriate content, can be employed at all learning levels.
Over the past decade, there has been a growing recognition in the physics community of the need for students in undergraduate physics programs to develop computational skills. Not only are computational skills utilized in a wide variety of careers, but they also teach students transferrable skills such as problem solving, analysis and critical thinking. While the value of these skills is generally acknowledged, the integration of coding activities into physics courses begs the question: How does the engagement with computational activities enhance students’ learning of physics? This research project seeks to investigate the benefits and challenges of using computational exercises to learn the content delivered in undergraduate physics courses. In a second-year electricity and magnetism course, students wrote python code to numerically compute vector derivatives for a variety of fields that were presented either visually or symbolically. Learning gains were investigated using pre- and post-quizzes. Additionally, interviews were conducted with students as they developed their code. This provided insights into their thought process, confidence in their code, and reconciliation of the computed results with their pre-conceptions of the divergence and curl of the vector fields explored.
Multiple choice questions are a common teaching and evaluation tool supporting Peer Instruction (PI) pedagogy in large-enrolment introductory physics classes across Canadian universities. Unfortunately, the multiple-choice format limits the opportunities for the students to formulate their own ideas. In addition, such questions often over-simplify the phenomena presented. Case studies based on open-ended and more realistic scenarios can provide a viable additional option for student collaborations in the classroom and beyond. This talk will present an example of such activity – a case study exploring the air resistance and the concept of the terminal velocity. Air resistance is the topic that is often ignored in the introductory physics curriculum, despite being virtually unavoidable in real life. The case study explores the topic through the analysis of a real event: a historic 2012 fall from the stratosphere in which the skydiver broke the world records for the highest “freefall” and the highest manned balloon flight, as well as becoming the first person to break the sound barrier in “freefall”. The students were provided the set of data of the skydiver's speed versus time and were asked a series of questions about the flight requiring them to analyze the data provided. While the full effect of such case studies on conceptual learning still needs to be formally evaluated, it is already clear that they have a potential to increase the students' engagement with the material.
The Bomem DA3 series of Fourier transform (FT) spectrometers were the first commercially available research-grade instruments of their type. They were available for purchase from 1980-2000. This FT could achieve an ultimate resolution of 0.0025 cm-1, with a resolvance of 106 at any wavelength, impressive specifications even for a similar modern instrument. The scanning Michelson interferometer and on-board electronics were simple and robust, but the computer systems that controlled the instrument, collected the interferograms and processed the spectra have long been obsolete.
We inherited a DA3 FT from Dr. Anthony Merer at UBC and, with the help of colleagues in Lyon, France who run a similar instrument, our group has revived it with new methods for control of the mechanical components, and for new data collection and processing procedures. The instrument is now routinely used to record dispersed fluorescence spectra of metal-bearing molecules generated in our lab at UNB. The talk will focus on the revival of the DA3, ways in which we have obtained improved performance from it, and extensions to its capabilities not available in the 1980s.
A kW laser beam focused on metal creates a highly dynamic environment of considerable importance to automotive production and 3D additive manufacturing. For example, laser welding allows the use of non-traditional materials to reduce vehicle weight (for improved fuel efficiency) but provides no direct on-the-fly quality indicator. The dramatic increase in demand for electric vehicles has required the development of completely new manufacturing techniques (e.g., welding 100s of battery tabs) necessitating the development of new monitoring techniques to ensure compliance with stringent part quality requirements. Metal 3D printing promises custom part creation at the push of a button, but slow print speeds coupled with inconsistent part quality and expensive ex situ quality assurance (e.g., x-ray CT) have slowed widescale adoption. We developed inline coherent imaging, an interferometric imaging approach easily deployable in the field that can monitor laser processing operando at high speeds (>300 kHz) and high resolutions (< 10 micron) [1]. Recent work combines this approach with other in situ diagnostics (e.g., integrating sphere radiometry) to capture simultaneous depth and absorptance to reveal the microscopic origin of the highly efficient energy coupling from light to metal integral to laser welding [2]. Simultaneous capture of morphology through both inline coherent imaging and high-speed x-ray imaging (possible only with synchrotron-based light sources) definitively explains the supposed “noise” in optical depth imaging [in preparation]. In metal 3D printing, we track morphology layer by layer, providing an immediate check on surface roughness, recoater blade damage, and powder packing density [3]. Defects are corrected through closed-loop control before subsequent layer deposition.
[1] Webster et al., Optics Letters 39, 6217-6220 (2014).
[2] Allen et al., Procedia CIRP 111, 5-9 (2022).
[3] Fleming et al., Additive Manufacturing 32, 100978 (2020).
Performing in-situ ion beam analysis to determine metal oxide growth mechanisms poses challenges due to the incompatibility of a electrolyte solution with ultra-high vacuum (UHV). To circumvent this problem, a specialized in-situ cell was developed which isolates the liquid electrolyte from the UHV using a silicon wafer, preventing any contact between vacuum and liquid. This wafer is equipped with a 50-200nm thin Si3N4 window, then coated in the metal under investigation and inserted with the metal in contact with the electrolyte, isolating the electrolyte from the vacuum. As a result, the ion beam can pass through the Si3N4 window, interacting with the material on the opposite side. This technique allows electrochemical methods such as anodization and impedance measurements to be taken under UHV and in-situ with Rutherford backscattering spectroscopy (RBS).
Upon preliminary testing of magnetron sputter deposited thin film Ti, higher oxide growth during anodization was reported compared to literature and ex-situ anodization studies. Exposure of Ti/Si3N4 sample to a 1 MeV He+ ion beam for 30 minutes with no applied potential showed a spontaneous formation of a continuous oxide layer. Next, the study focused on radiolysis product generation after ruling out considerations such as charging from the ion beam on the Si3N4 surface facing vacuum. Radiolysis was done using two separate alpha sources; 241Am at 0.525 Bq, 5.7 MeV, and 241Am/247Cm/244Pu at 0.525 Bq, 5.7 MeV. Ti samples with known oxide thickness were submerged in 0.27 M NaCl solution for various times, with a maximum of 193 hours, with the nuclide source facing the solution. Additional covered and uncovered samples were created with similar setups for control. Channeling RBS experiments were performed on the samples, and the resultant spectra were analyzed using SIMNRA to determine oxide growth as a function of incident alpha particles. Using linear regression analysis, the growth of titanium oxide as a result of alpha radiolysis in a conductive analyte was quantified. From these experiments, it was found that the formation of radiolysis products in an electrolyte solution contributed to the spontaneous oxide growth of Ti.
Appropriate characterization is vital for improvement of the electronic properties of semiconductors in photovoltaic devices, which will enable solar energy to compete with non-renewable energy sources. A critical electro-optical characterization tool for determining the carrier mobility in thin-film solar cells is offered by photo-carrier extraction by linearly increasing voltage (photo-CELIV) [1], in which a nano-second laser pulse is applied to a device followed by a linear extraction voltage ramp. The maximum intensity and extraction time of the transient offer information on the photocarrier mobility. In this presentation, we describe how a photo-CELIV apparatus has been integrated with a confocal optical microscope to extend the ability of photo-CELIV to obtain cross-sectional mobility profiles along the z-axis of a solar cell. High laser power density at the microscope’s focal plane leads to a drastic increase in non-geminate recombination, such that the concentration of charge carriers extracted from the microscope focal plane saturates. A model has been developed to analyze the photo-CELIV transients at each confocal plane and calculate the cross-sectional mobility profile based on discretization of the active layer into N slices of unknown mobility. To test this method, we apply it to a hydrogenated amorphous silicon (a-Si:H) solar cell, which is a well understood material, and thus well suited for testing this novel characterization technique. Comparison of our results with measurements of the hydrogen content profile shows very good correlation, allowing for direct confirmation of our obtained mobility profile.
[1] Juška et al, Phys. Rev. Lett., 2000, 84, 4946
The nonlinear relationship between the form and function of physical structures in our built environment raises challenges for design. Modern design methods, such as topology optimization, provide structural solutions but obscure the relationship between the form of the solution and the formulation of the underlying design problem. Here, we show that embedding computational structure design in statistical physics provides unprecedented insight into the origin and organization of design features. We show how our "hyperoptimization" approach, a generalized, superset of molecular dynamics and standard simulated annealing optimization, surmounts known design problems including grayscale ambiguity, manufacturing inaccuracy, and artificially over-specified criteria in computational morphogenesis.
Skyrmions are a topologically non-trivial magnetic state that has been observed in several different magnetic materials, such as the chiral cubic magnets Cu2OSeO3, FeGe, and MnSi. In these non-centrosymmetric systems, competition between the symmetric exchange interaction and Dzyaloshinskii-Moriya interaction results in the formation of incommensurate spin textures, such as the vortex-like skyrmions. In metallic systems, such as FeGe, these skyrmions can be manipulated by small electrical currents, with motion occurring at very small current densities. This raises the possibility for them to be used in ultra-low energy electronic applications, such as memory devices or stochastic computing. In this talk, I will introduce general features of the skyrmion state, and present recent work on skyrmions in thin lamella of FeGe and Cu2OSeO3, investigated using soft X-ray scattering. In particular, I will discuss aspects of skyrmion metastability in these systems, as well as investigations of the current-induced motion of skyrmions in sample with variable thickness, and the prospects of this leading towards potential applications.
The properties of heavy 5d transition metal oxides, such as iridates and osmates, are often remarkably different from those of their lighter 3d counterparts. In particular, the presence of strong spin-orbit coupling (SOC) in these compounds can give rise to a variety of exotic quantum states, including spin-orbital Mott insulators, topological insulators, Weyl semimetals, and quantum spin liquids. In materials based on edge-sharing octahedral crystal structures, large SOC can also lead to unconventional magnetism, and a form of highly anisotropic, bond-directional Ising interaction known as the Kitaev interaction. The first, and best known, experimental realizations of Kitaev magnetism are honeycomb lattice materials: the 5d iridates A$_2$IrO$_3$ (A = Na, Li) and the 4d halide α-RuCl$_3$. These compounds have attracted considerable attention due to predictions of a Kitaev quantum spin liquid with exotic anyonic excitations. However, there has recently been growing interest in the search for Kitaev magnetism in other families of materials with different lattice geometries. In this talk, I will describe several candidates for Kitaev magnetism beyond the honeycomb lattice. This will include (1) potential face-centered-cubic (fcc) Kitaev systems, such as the double perovskite iridates (A$_2$BIrO$_6$) and iridium halides (A$_2$IrX$_6$), and (2) potential Kitaev chain systems in quasi-1D iridates.
We present the results of a finite-temperature study of a Heisenberg-Dzyaloshinskii-Moriya Hamiltonian on AB-stacked kagome bilayers. We develop an exact analytical coarse-graining procedure to map the microscopic Hamiltonian onto a generalized XY model on a triangular lattice. To leading order, the effective XY model includes both bilinear and biquadratic interactions. In a large portion of the parameter space, the biquadratic couplings dominate in the system, leading to two phase transitions: a high-temperature nematic, and a low-temperature Ising transition. In bilayer systems, these transitions are accompanied respectively by the binding/unbinding of half-integer or integer topological vortex defects. Furthermore, we show that when the ground state is incommensurate, thermal fluctuations change the nature of the low-temperature transition from continuous to first-order. These predictions are confirmed by the numerical Monte-Carlo finite-size analysis.
The Heisenberg-compass model on a square lattice offers a simple example of a frustrated magnet that exhibits the phenomenon of order by disorder (ObD). In this system the ordering direction is selected by quantum zero-point fluctuations for much of the phase diagram, providing a minimal context to explore manifestations of ObD, such as the presence of a pseudo-Goldstone gap. We explore the Heisenberg-compass model by exact diagonalization on small clusters. By employing translation symmetries of the model, ground state properties, including energies and correlation functions, are studied for clusters of up to 25 spins. We find a phase diagram qualitatively consistent with the classical result, identifying the magnetic ordering pattern via the spin-spin correlation functions. The low-lying spectrum, specifically the evolution of the spin-wave gap, will be presented as a function of the Heisenberg and compass exchanges. We find good agreement between the exact diagonalization results and semi-classical expectations from non-linear spin-wave theory.
Canadian Science Publishing welcomes all CAP attendees for a discussion about the future of science publishing and how publishing serves the research community. CSP will present a brief outlook on the changes within publishing companies (including our own not-for-profit structure) as well as the future of scientific publishing with particular focus on Open Access and Open Science. We will present for discussion models of agreements that make it possible for OA to be financially feasible for today’s researchers, and welcome feedback on how the Canadian Journal of Physics can better serve the physics research community. The second half of the session will be open for community discussion with representatives from CSP as well as the Editors in Chief of the Canadian Journal of Physics, Profs. Robert Mann and Marco Merkli.
As teachers we want our students to learn. As students we want high marks. What classroom practices build a bridge between these wants? We will explore the role of questions and student cognition, white boards, and low-cost hands-on experiences to promote learning about the abstract concepts of electric fields and magnetic fields.
The Large Hadron Collider restarted collisions at $\sqrt{s}$ = 13.6 TeV in 2022, beginning the start of a planned 4-year Run 3. The ATLAS experiment is now commissioning several upgraded detector systems to best take advantage of the new dataset, including the New Small Wheels and phase-1 liquid argon electronics upgrade to which Canadian physicists made substantial contributions. This talk will highlight the ongoing status of data-taking and commissioning of these systems, and highlight the first physics results from ATLAS utilizing the run 3 dataset.
Top quark being the heaviest elementary particle, and the only quark which decays in its bare form, has the potential to reveal crucial information on particle dynamics. For example, precise measurement of top quark mass is needed to understand the vacuum structure, including its stability. Having the strongest coupling with Higgs boson, it can reveal information related to the electroweak symmetry breaking in a unique way. BSM effects can affect the couplings of the top quark with the Higgs boson, as well as other quarks and gauge bosons. Some of these lead to rare decays of top quark with small branching fractions, but significantly larger than the corresponding SM predictions. With very large cross section at TeV energies of pp collisions, the LHC at the end of its Run3 is expected to produce close to half-a-million top quark-antiquark pairs. Such statistics is capable of probing some of the BSM scenarios of rare decays. Proper understanding of the role of CP-symmetry in particle dynamics is another important issue. For example, presence of non-zero electric dipole moment of an elementary particle would indicate violation of CP-symmetry beyond what the CKM quark mixing structure prescribes. Top quark is an ideal system to probe this. In addition to the top quark-antiquark pair production, sizeable production of single top events and four-top events are expected at the LHC in its high luminosity version beyond Run3.
In the talk, we shall review the top quark study in the light of LHC within and beyond the SM, summarising the experimental and theoretical results so far. Some emphasise will be given to the Flavour-Changing-Neutral-Current (FCNC) interactions of the top quark, as this is one of our current interests.
As the heaviest known fundamental particle, the top quark plays a special role in many theories of new physics beyond the Standard Model. Reconstruction of top anti-top pair production to the best possible resolution is therefore crucial to enhancing our sensitivity to Beyond Standard Model effects in precision measurements and searches at the Large Hadron Collider (LHC), from improved mass resolutions for bump hunting to more diagonal unfolding matrices for differential cross-section measurements. As such, we’ve designed a deep neural network (TRecNet) that infers the four-vectors of the top and anti-top quarks from detector-level decay products in the semi-leptonic decay channel at ATLAS. The performance of TRecNet and several slight variations of the network are compared to traditional top reconstruction algorithms based on likelihood fits and are shown to improve upon both reconstruction efficiency and resolution.
We use the newly proposed Energy Mover’s Distance as a measure of jet isotropy to define new jet substructure observables for quark/gluon discrimination and identifying hadronically-decaying top quarks with large transverse momentum. We assess their effectiveness by comparing them with other classifiers. The quark/gluon study is conducted at hadron level while the top quark study is conducted at detector-level in events reconstructed with a simulated version of the ATLAS detector implemented in GEANT4.
The $t$-channel single-top quark production is observed for the first time at a centre-of-mass energy of 5.02 TeV using proton-proton collision data collected by the ATLAS detector at the Large Hadron Collider. The observation is made using an event selection optimized for the $l$+jets decay topology of the single-top process, which requires candidate events to have exactly one charged lepton (electron or muon), exactly two jets, only one of which must arise from a $b$-hadron decay, and a large transverse momentum imbalance; and after which using a multivariate discriminant to separate the $t$-channel signal events from background events that satisfy the $l$+jets topology. Using a profile likelihood fit, we measured the production cross-section of single-top quarks and antiquarks individually, the inclusive cross-section for the combined production, the ratio of single-top quark to antiquark production, and $V_{tb}$ in the CKM matrix.
During the past few decades, many astronomical and cosmological studies provided strong evidence for the existence of dark matter.
Though, to this day, we do not have any hint about what dark matter is, which motivates taking any opportunity to probe this question.
One possible solution is to extend the Standard Model with a new U(1) gauge group.
This introduces a new mediator: a light boson, usually associated with a dark photon A', that couples to the Standard Model kinetically.
On top of that, the ATOMKI collaboration has recently observed an anomaly [Phys. Rev. Lett. 116, 052501 (2016)] that might be explained by a 17 MeV dark photon.
For these reasons, we search for a low mass dark photon decaying to an electron and positron using the $387$ fb$^{-1}$ of 10.58 GeV centre-of-mass data collected with the Belle II detector at the SuperKEKB $e^+e^-$ collider. We probe $e^+e^- \rightarrow \gamma_{ISR} [A' \rightarrow e^+e^- ]$ visible decays in a mass range from 10 MeV up to 200 MeV.
We present new preliminary results that set a $90\%$ CL upper limit on the kinetic coupling of the dark photon, and give the first results of a search in $e^+e^-$ collisions in the region below 20 MeV, a region also sensitive to the ATOMKI anomaly.
PICO-40L is a bubble chamber detector with a target material of superheated C3F8, located at the SNOLAB underground research facility outside Sudbury, Ontario. With its abundance of non-zero-spin fluorine nucleons in the detector target and its effective blindness to electron recoil interactions, it is projected to set world-leading exclusion limits in the spin-dependent dark matter interaction parameter space. Unlike previous generations of the PICO experiment, PICO-40L employs a "Right Side Up" design, with the target fluid above the chamber compression and expansion system, which is expected to eliminate a class of backgrounds from previous versions of the detector. PICO-40L is currently in the commissioning stage and is expected to start its year-long blinded data-taking run in the mid-to-late summer of this year. The analysis strategy, as well as the results from the early commissioning runs, will be presented in this talk.
The DEAP-3600 experiment at SNOLAB primarily searches for Weakly Interacting Massive Particle (WIMP) dark matter candidates through interactions with argon nuclei. The detector consists of 3.3 tonnes of liquid argon housed in a spherical acrylic vessel which is viewed by 255 photomultiplier tubes. Data have been taken stably from November 2016 to March 2020 and the detector is currently undergoing hardware upgrades. DEAP-3600 achieved world-leading constraints on Planck-scale mass dark matter, and the most sensitive limit on the spin-independent WIMP-nucleon cross-section among the argon-based experiments. This talk presents the latest DEAP-3600 results demonstrating the background models, updates on the dark matter search, as well as other physics analyses and measurements.
Entropy production is a necessary ingredient for addressing the over-population of thermal relics. It is widely employed in particle physics models for explaining the origin of dark matter. A longlived particle that decays to the known particles, while dominating the universe, plays the role of the dilutor. We point out the impact of its partial decay to dark matter on the primordial matter power spectrum. For the first time, we derive a stringent limit on the branching ratio of the dilutor to dark matter from large scale structure observation using the SDSS data. This offers a novel tool for testing models with a dark matter dilution mechanism. We apply it to the left-right symmetric model and show that it firmly excludes a large portion of parameter space for right-handed neutrino warm dark matter.
The SNO+ Experiment is a versatile multipurpose neutrino detector situated at SNOLAB, with the primary goal of searching for neutrinoless double beta decay. After a successful operating phase as a water Cherenkov detector, the SNO+ target medium was switched to a liquid scintillator to increase the light yield of the detector, thereby enabling a much richer physics programme. In addition to ongoing measurements of reactor antineutrinos, solar neutrinos, geoneutrinos, supernova neutrinos, and other exotic phenomena, the SNO+ experiment is now preparing for a future phase capable of neutrinoless double beta decay. After presenting an overview of the detector and recent preliminary results, the upcoming physics capabilities of the experiment will be discussed.
Quantum black holes are one of the main playgrounds of any theory of quantum gravity. Describing such objects is a principal goal of these theories. I will review the fundamentals of analyzing black holes in non-perturbative canonical quantum gravity and briefly present some of the models arising from this approach. I will also present a short overview of some of the phenomenological aspects of these black holes in the effective regime that are predicted by such models.
Following the techniques of canonical loop quantum gravity, a full Thiemann regularization is performed on the scalar constraint of classical general relativity. The regularized Hamiltonian is then considered for a general spherically-symmetric spacetime, without recourse to additional gauge-fixing conditions commonly imposed to aid in computing the radial holonomies. By investigating the form of the modified scalar constraint in various contexts, including cosmological and black hole spacetimes, we develop an effective framework for the dynamics of spherically-symmetric spacetimes endowed with an underlying discrete structure.
Caustics are regions of high intensity created generically by the natural focusing of waves, and are universally described by catastrophe theory. Each distinct class of catastrophe is uniquely described by its own diffraction pattern, the simplest two being the Airy and Pearcey functions. A more exotic form of logarithmic wave singularity occurs near event horizons, which have acoustic analogues in quantum fluids such as Bose-Einstein condensates where Hawking radiation can be simulated. In such systems logarithmic singularities are regulated by taking into account non-linear dispersive effects, and are properly described by an Airy-type wave function supplemented by a logarithmic phase term. We find the presence of additional sub-dominant waves not yet predicted near the horizon. Furthermore, the horizon and the caustic do not in general coincide; the finite spatial region between them delineates a broadened horizon. Our catastrophe theory motivated approach allows us to comment on the stability/universality of inter-atomic length scale corrections to the Hawking spectrum (analogous to Planck scale corrections for gravitational Hawking radiation).
We use a novel approach to numerically calculate Fast-Oscillating Integrals (FOI) using the Picard-Lefschetz theory. In this theory, analytic oscillatory integrals are converted into sums of convex integrals by deforming the integration domain in the complex plane. Feldbrugge, Pen, and Turok 2019 introduced a new numerical integrator to evaluate the interference effects near caustics in lenses in one dimension. Recent studies have also used this numerical integrator to study lensing of gravitational waves as well, however one shortcoming of the integrator is that it is not optimal. In this work, we optimize the convergence to desired contours in the complex plane and further generalize the algorithm to work for random functions that appear in various physical applications like scintillation of radio signals in astrophysical sources.
Magnetic resonance imaging (MRI) is well known as a non-invasive diagnostic imaging technique available to clinical medicine. MRI provides high spatial resolution images with flexible soft tissue contrast as the signal encoding is more complicated than other imaging modalities.
Machine learning, especially deep learning, has become a popular research topic to solve nonlinear problems. It has played an important role in many areas, from self-driving car to chatGDP. The MRI research community has embraced the opportunity and exploited the powerful tool in image classification/feature detection, and signal processing/image reconstruction. However, diagnostic imaging presents different challenges compared to other digital image processing tasks such as computer vision. In this talk, I will present the capabilities and potential pitfalls of deep learning, focusing on the applications in MRI.
Introduction: Hyperpolarized 129Xe lung MRI is an efficient technique used to investigate and assess pulmonary diseases. However, the longitudinal observation of the emphysema progression using hyperpolarized gas MRI-based Apparent Diffusion Coefficient (ADC) can be problematic, as the disease-progression can lead to increasing unventilated-lung areas, which likely excludes the largest ADC estimates. One solution to this problem is to combine static-ventilation and ADC measurements following the idea of 3He MRI ventilatory ADC (vADC). We have demonstrated this method adapted for 129Xe MRI to help overcome the above-mentioned shortcomings and provide an accurate assessment of the emphysema progression.
Methods: Ten study-subjects with written informed consent provided to an ethics-board-approved study protocol, underwent spirometry and 3He/129Xe MRI scanning. 129Xe imaging was performed at 3.0T (MR750, GEHC, WI) using whole-body gradients (5G/cm maximum) and a commercial 129Xe quadrature-flex RF coil (MR Solutions, USA).1 Hyperpolarized 129Xe gas (polarization=35%) was obtained from a turn-key, spin-exchange polarizer system (Polarean-9820 129Xe polarizer). VDP was generated using the DL. We used 2-D U-Net architecture for segmentation and ResNet-152 as the backbone network that was trained on the ImageNet and a low-resolution MRI dataset. The segmentation masks were compared to ground truths using dice similarity coefficient.
Results: Fig.1 shows the acquired static-ventilation images (top-panel), matched voxel-size unweighted (b=0,) images (middle-panel) and correspondent ADC maps (bottom-panel) in coronal view for a representative study-subject demonstrating a good- match between static-ventilation and matched resolution unweighted-slices. Table 1 shows the demographic, PFTs, mean VDP, ADC, and vADC estimations for all study-subjects.
Discussion and Conclusion: In this proof-of-concept-study, we showed that the emphysema-progression can be potentially quantified with using the pulmonary static-ventilation and diffusion-weighted images of hyperpolarized 129Xe utilizing the ventilatory ADC approach powered by the DL-segmentation.
INTRODUCTION: A non-invasive imaging technique inhaled hyperpolarized (HP) 129Xe magnetic resonance imaging (MRI) is presently employed to assess lung structure and function1. It is possible to quantify the ventilation/perfusion (V/P) of the lungs simultaneously using this MRI technique because the solubility of xenon in lung tissues is higher compared to other imaging gases. This measurement is possible owing to the distinct and broad range of chemical shift frequencies (~200 ppm) of 129Xe when residing in lung tissue, brain tissue, and red blood cells as opposed to the gas phase.
[15O]-water positron emission tomography (PET) is the gold standard imaging method for determining cerebral perfusion2,3. In this study, simultaneous in-vivo 129Xe-based MRI and [15O]-water PET images were collected and compared.
METHODS: [15O]-water solution (30mL) contained in a 60mL plastic syringe was used to dissolve 30mL of the hyperpolarized 129Xe gas. Anesthesia was induced in rats with 5% isoflurane and oxygen and maintained at 2%. A 24g tail vein catheter was inserted for delivery of the [15O]-water / 129Xe mixture. Hyperpolarized 129Xe gas was obtained from a turn-key, spin-exchange polarizer system (Polarean 9800 129Xe polarizer). In-vivo PET imaging was obtained using a small animal MRI compatible PET insert (Cubresa Inc.) [15O]-water PET data was acquired simultaneously with 129Xe MRI using the integrated PET system in the 3T PET/MRI.
RESULTS: 2D axial 129Xe MRI images and [15O]-water PET images were acquired simultaneously indicating that the diameter of the phantom from both PET and MRI images were similar. The 129Xe image demonstrates a sufficient SNR level (80). The anatomical-proton and [15O]-water-PET-perfusion images of rat-brain were also produced.
CONCLUSIONS: The results of this study clearly indicate the feasibility of simultaneous hyperpolarized 129Xe MRI and [15O]-water PET measurements. This demonstration proves that 129Xe could be used as a potential non-radioactive and high-resolution imaging tool.
References:
1. Kaushik, S. S. et al. MRM (2016); 2. Fan, A., et. al. JCBFM (2016); 3. Ssali. T., et. al. JNM (2018).
Introduction: It has recently been shown1,2 that combining Compressed-Sensing with the Stretched-Exponential Model (SEM) can significantly increase SNR of accelerated/undersampled MR images. The reconstruction uses an exponentially decaying signal trend across a group of images assumed to represent the decaying density of resonant isotope in lungs after each wash-out breath. This decaying signal trend can be induced artificially to ensure the reconstruction : previous work was done using a specific averaging pattern1,2, but this signal decay can be a result of decaying hyperpolarized (HP) xenon polarization in a set of back-to-back acquisitions.
Method: In-vitro MRI was performed at 74mT on a phantom with 45mL of HP 129Xe (35% polarization): 3 sets of 10 undersampled images each were acquired (acceleration factor of 7), only refilling the phantom with fresh hyperpolarized xenon gas between sets. To ensure adequate sampling of the centre of k-space, the Fast-Gradient-Recalled-Echo (FGRE) sequence was modified for centric-out trajectory in both phase-encode and readout directions.
Seven coronal slices (30mm) of 9 undersampled (AF=7) 2D human lung images were acquired at 3T with 1L of inhaled HP 129Xe (33% polarization, 30/70 129Xe/4He), all acquired in one breath-hold (1s/slice, 7s total scan time). The previously used averaging pattern was applied before the reconstruction, and the SNR was fitted to the SEM using the Abascal method.3
Results: The signal of the phantom images followed the expected exponential decay trend. The reconstructed human lung images saw around 5x higher SNR compared to the original non-averaged images.
Conclusion: Although the signal decay of the phantom images followed the expected trend, the reconstruction was not able to be performed: this was caused by unexpected low frequency RF interference presenting as a consistent spike in k-space, confusing the reconstruction algorithm. The source of this interference and possible solutions are under investigation. The prospectively undersampled lung images show improved SNR within a single breath-hold: to remove the artefacts, a lung dataset will be assembled to train the artefact removal neural network2 developed previously on undersampled lung reconstructions.
References:
1 Perron et al. ISMRM (2021); 2 Perron et al. ISMRM (2022); 3 Abascal et al. IEEE Trans Med Imaging (2018).
A key question of modern physics concerns how the bulk of the universe's visible mass emerges from the Standard Model (SM). Some of this mass is generated by Higgs boson couplings to matter fields in the SM, but of the constituents of atomic matter, this suffices to explain only the mass of electrons in its entirety. The overwhelming majority of atomic mass resides in the nucleus, which is composed of neutrons and protons (nucleons), bound together by the exchange of pions and other mesons at shorter ranges. As far as these nucleons and pions are concerned, the Higgs-generated mass component is only a small fraction. The overhelming majority of the mass comes from the dynamical quark-gluon interactions of QCD, through a mechanism termed ``Emergent Hadronic Mass'' (EHM). Paradoxically, the study of the lightest pseudoscalar mesons, the pion and kaon, appear to hold the key to a further understanding of EHM and structure mechanisms. I will discuss the contributions the PionLT and KaonLT experiments at Jefferson Lab are expected to make towards the resolution of this puzzle, as well as the role of proposed future extensions of these measurements using the Jefferson Lab 22 GeV upgrade and the Electron-Ion Collider.
There are many open questions in the field of hadronic structure, as the properties of constituent quarks and gluons (e.g. spin and mass) do not explicitly add up to the properties of hadrons. The pion is a simple hadron, consisting of only two valence quarks (up and down), which makes it an ideal candidate for studies of hadronic structure. The exclusive pion electroproduction reaction, with a ground state nucleon p(e, e’ π+)n has been studied in detail at low momentum transfer (Q^2). The longitudinally polarized virtual photons dominate the cross-section of this reaction at low -t. A number of physical observables such as form factors and Generalized Parton Distributions (GPDs) can be extracted from this cross-section using models. Experimental Hall C at Jefferson Lab is the only active facility in the world that can host high precision studies of exclusive pion electroproduction reactions. With the 12 GeV upgrade, it allows the extraction of pion form factor at moderate Q^2, as well as giving a unique opportunity to study higher resonance of pion electroproduction reaction p(e, e’ π+)Δ. This research aims to measure the separated cross-section of the ground state reaction, as well as first measurement of the higher resonance reaction. The comparison of separated cross-section of two reactions will be invaluable for our understanding of hadronic structure.
Photoproduction mechanisms studied in the GlueX experiment allows the mapping of light mesons in unprecedented detail with particular interest in exotic meson candidates. This is achieved by impinging an 8.2-8.8 GeV linearly polarized photon beam on a liquid hydrogen target. The measurement of beam asymmetry $\Sigma$ will help constrain quasi-particle t-channel exchange processes using Regge theory. Understanding the photoproduction exchange mechanisms is a crucial ingredient in establishing hybrid and exotic photoproduced light meson states. $\Sigma$ is extracted from the azimuthal angular distribution between the meson production plane and the polarized photon beam. In particular, we will report results on the beam asymmetry measurements for $\eta$ in the reaction $\gamma$ p $\rightarrow$ $\eta$ $\Delta^+$. This reaction with a recoiling $\Delta^+$ will allow for comparison and validation of theoretical calculations and provide additional validation of the $\eta$ asymmetry with a recoiling proton. The different isospin of the $\Delta^+$ imposes additional restrictions that further constrain allowed Regge exchanges.
The KaonLT/PionLT Collaboration probes hadron structure by measuring deep exclusive meson production reactions at Jefferson Lab. A set of high momentum, high resolution spectrometers in Hall C allow for precision measurements from which form factors and other observables can be extracted. One possible measurement is the beam spin asymmetry, which describes the fractional difference in cross-section between events caused by an electron of positive or negative helicity. This asymmetry is caused by interference between longitudinally and transversely polarized virtual photons, which makes it possible to extract a polarized interference cross-section $\sigma_{LT’}/\sigma_0$. In this work, the asymmetry is calculated in the transition regime where the strong force is still poorly understood (Q$^2$ between 2 and 5.5 GeV$^2$), for the p + e → e’+ π + n reaction data from the recent KaonLT experiment. The dependence of $\sigma_{LT’}/\sigma_0$ on the four-momentum transfer to the target -t is then determined, and the results are compared to two different classes of theoretical models. By comparing with predictions made using both Regge trajectories and Generalized Parton Distributions, the asymmetry helps determine how to best describe hadronic reactions in the transition regime, thus providing insight into the strong force.
Hadrons are typically described using "quenched" constituent quark models, which posit a Hamiltonian acting on the state space of the valence quarks, neglecting mixing of higher Fock states. In recent years, experimentalists have observed states which are not well characterized by these models, motivating quark modellers to examine the effects of unquenching. The resultant mass shifts throw the entire predicted spectrum into disagreement with observation, which may indicate that the leading-order effects of unquenching have been absorbed into the phenomenologically-measured parameters of the quenched Hamiltonian. We have calculated corrections to the spectrum using a formalism which estimates and compensates for the effects of this parameter renormalization, leaving small residual mass shifts which better reflect the observable effects of unquenching.
There has been noted concern regarding the retention, academic success, and motivation of students in STEM courses, especially physics. Many factors can impact students’ persistence in STEM courses, however students who do persist often find themselves underprepared for problem-solving within authentic settings. Problem solving is a highly valued 21st Century workforce skill in Canada (Hutchison, 2022) that recent graduates seem to lack (Cavanagh, Kay, Klein, & Meisinger, 2006; Deloitte & The Manufacturing Institute, 2011; Binkley et al., 2012; Finegold & Notabartolo, 2010). To positively impact undergraduate physics education, conversations are needed on ways to transform curricula that support diverse populations of students. There are increasing calls for using evidence-based teaching strategies to improve STEM instruction (Cooper et al., 2015). Prior studies have revealed that both contrasting cases and argumentation tasks can support deeper learning and problem-solving skills. Yet, students are seldom encouraged to justify or to explain their solutions. They rarely reflect on the appropriateness of their responses and consider alternative solutions. Studies suggest that appropriate scaffolds are needed for these instructional strategies to be successful. In this talk I describe how we have integrated contrasting cases and argumentation and alternative forms of writing prompts (similarities and differences, invent a unifying statement, and argumentation) used in introductory physics for non-science majors as well as in calculus-based physics. Results suggest that prompts for identifying similarities and differences within cases tended to promote identification of surface features irrelevant to solving the problems. However, argumentation prompts to evaluate competing theories tended to support deeper understanding of underlying physics principles and appropriate application of principles.
What is most important for non-physics specialists to learn from an introductory physics course? How can course design and assessment support learning transferable skills, especially in large “lecture” classes? We will discuss preliminary results from a collaborative research-practice self-study partnership focusing on Sealfon’s implementation of learner-centered approaches in a 200-student first-semester algebra-based physics course with labs. The course design followed the two intentionalities of the Investigative Science Learning Environment (ISLE) approach (Brookes, Etkina, and Planinsic 2020): (1) We want students to learn physics by thinking like physicists; by engaging in knowledge-generating activities that mimic the actual practices of physics and using the reasoning tools that physicists use when constructing and applying knowledge. (2) The way in which students learn physics should enhance their well-being (via empowering versus authoritative teaching practices). In the lecture hall, students worked in pairs or small groups on knowledge-generating activities on their white boards (laminated sheets of paper). Sealfon regularly pulled a group’s whiteboard, displayed it to the class using a document camera, and discussed the activity with the class. In labs, students worked in small groups to design and conduct experiments to observe phenomena, propose explanations for patterns, and test ideas (hypotheses). Students completed reading and homework using the interactive Perusall platform with brief feedback provided by their teaching assistants. Nontraditional assessment elements included two-stage tests with an optional collaborative portion and an option to revise and resubmit problem-solving solutions on tests with oral quizzes given by teaching assistants.
Since the pandemic forced everything online, there have been rapid and significant changes to the way many of us have been teaching and learning. As more options for in-person activities become available again, we need to consider which elements of learning in the online environment benefit students and are worth keeping. Beginning in Fall 2020, we distributed anonymous online surveys (Fall and Winter) related to students’ interests, motivations and preparedness to all students taking introductory level physics courses at McMaster University. These students are taking physics courses which are aimed at either physical science students, life sciences students, or engineering students. While there is significant overlap in the content of these courses, the student cohorts differ by stream. Comparing results across years and between cohorts, can provide us with insight into our students’ experiences under different learning conditions.
With the shift to online learning, lab kits containing simple, affordable equipment were made to replace the previous in-person labs for our Physics for Life Sciences course. In these home labs, students can perform the experiments and collect their own data independently, and are able to learn about data analysis, graphing and different physics concepts. With most labs now back in person, this year, we took the opportunity to compare the two lab modalities. All students completed two different labs on the same theme (kinematics), one at-home and one in our on-campus labs. Students were then asked (anonymously) about their experiences in the two different labs: what they liked, how they felt they learned, and any challenges they encountered.
I will share some of our results from these surveys as well as some of our plans going forward based on what we have learned so far.
Students who excel in mathematics and physics in high school often consider engineering or physics for university-level studies. But how do they make their choice? How can the education system better advise them to choose the career that is best for each one of them individually? We present results from a survey on how first-year university students choose between the physical sciences and engineering, and examine aspects of how recent high-school students understand the differences and similarities between science and engineering, and how their understanding factors into their choice of university study. Results from our survey may inform outreach and pedagogy for science and engineering, and thus foster greater attraction and retention of undergraduate students in STEM fields, and greater career sustainability and life satisfaction for our graduates.
The accurate measurement of time is of critical importance to society as it provides the means to synchronize events in our lives. The world has ever-increasing demands for precise time in fields such as automation, energy grids, smart cities, financial markets, fundamental research, and global positioning and navigation. Since the world moved to an atomic definition of time in the 1960s, caesium fountain clocks have provided the most accurate realization of the SI second. At the National Research Council, the NRC-FCs2 fountain clock has been operating as a primary frequency standard for Canada since 2020. It is used to contribute to the steering of International Atomic Time, as well as Canada’s official timescale. I will outline the design and performance of the clock, describe the current efforts to re-evaluate the systematic shifts that limit the uncertainty, and discuss the upcoming redefinition of the SI second.
This project focuses on the investigation of trap energy levels introduced by radiation damage in epitaxial p-type silicon. Using 6-inch wafers of various boron doping concentrations (1e13, 1e14, 1e15, 1e16, and 1e17 cm$^{−3}$) with a 50 µm epitaxial layer, multiple iterations of test structures consisting of Schottky and pn-junction diodes of different sizes and flavours are being fabricated at RAL and Carleton University.
In this talk, details on the diode fabrication and electrical measurements of the structures will be given. IV and CV scans of fabricated test structures have been performed and cross-checked between institutes, the results of which will be presented. Furthermore, another focus of this talk will be in the characterisation of trap parameters obtained from Deep-Level Transient Spectroscopy (DLTS) and supplemented by Thermal Admittance Spectroscopy (TAS). Spectra for unirradiated and irradiated diode samples will be shown and their details collected from Arrhenius analyses will be listed. Lastly, DLTS and Charge Collection Efficiency (CCE) measurements conducted on samples before and after neutron irradiation will be evaluated and their results compared.
HELIX, the High Energy Light Isotope eXperiment, is a balloon-borne payload designed to measure the isotopic abundances of light cosmic ray nuclei. Precise measurements of the 10Be nuclear isotope from 0.2 GeV/n to 10 GeV/n will help study propagation processes of cosmic rays. These measurements will allow the refining of propagation models, critical for interpreting excesses and unexpected fluxes reported by several space-borne instruments in recent years. Rare light isotopes will be observed by HELIX with the first in a series of long duration balloon flights in the upcoming year. The instrument will undergo several tests and phases during its commissioning period during which it may be deconstructed and rebuilt. Knowing the position of components following each assembly is important to the measurements of various detectors. The metrology of HELIX was thus studied to provide knowledge of the distances between specified points and planes of the experiment payload.
A Total Station, a device that provides precise optical measurements in surveying and construction, was used to create a position-tracking system for HELIX. This study tested the measurement protocol with various student-designed rigs using retroreflective dots as targets. The retroreflectors have been placed on the experimental payload and are now ready for use in virtual geometry reconstruction. The metrology procedure and code produced through this project will serve as a local positioning system for HELIX components and the output points will be used to update the geometry of the detectors in simulations.
The ocean Sound Speed Profile directly affects how acoustic waves propagate in the ocean. As a result, knowledge of the sound speed profile is important in many underwater acoustic applications including acoustic imaging, source localization, and underwater communication. Measurement of ocean sound speed can also provide an indirect measure of ocean temperature using the close dependence of sound speed on water temperature. Our presentation focuses on remote estimation of the ocean sound speed profile by using an underwater acoustic pulse-echo method. We propose the use of a directional transmitter and a number of receivers offset at a comparatively small distance from the transmitter location. Sound is scattered by naturally occurring targets and these signals are detected by the receiving array. The arrival time and phase in the detected signals contains information on the location of these targets and importantly, the sound speed through the water column. Sound speed estimates can be generated directly by the arrival time data but we propose the use of an inverse approach working with the phase in the signals that allows for greater accuracy in the sound speed estimates. The viability of our approach is demonstrated through use of an acoustic model that generates simulated received signals for our system geometry. We are using the model analysis to guide in the design of a prototype system for future field trials.
Phytoglycogen (PG) nanoparticles are hyperbranched, dendritic polymers of glucose that are produced as compact nanoparticles in the kernels of sweet corn. Our measurements of their structure, morphology, hydration and mechanical properties illustrate the unique properties of native PG nanoparticles: they are soft, porous, hairy and hydrated. These physical properties, combined with their digestibility and lack of toxicity, make PG ideal for a broad range of applications in personal care, nutrition and biomedicine. The properties of PG can also be tuned through chemical modification, such as controlled digestion using dilute acids or enzymes, or through covalent attachment of a variety of different chemical groups that can impart charge and hydrophobicity. In this talk, I will describe the properties of native PG particles and how these properties are modified by acid hydrolysis and covalent attachment of cationic groups, anionic groups, and groups that are both anionic and hydrophobic. These simple modifications have produced significant and sometimes dramatic changes to the physical properties of these soft colloidal nanoparticles, opening up new possibilities for applications of this sustainable nanotechnology.
This talk reviews recent studies of the dynamical and mechanical behaviour of nanocolloidal soft glassy materials using Rheo-XPCS, x-ray photon correlation spectroscopy with in situ rheology [1]. Rheo-XPCS allows for simultaneous studies of the mechanics and nanoscale dynamics of materials over a wide range of timescales from milliseconds to hours. As such, it is an outstanding tool to characterize the behaviour of glassy and other metastable soft systems under the influence of applied stress and strain. I will present several case studies of soft glasses composed of concentrated suspensions of charged silica nanoparticles, demonstrating (i) their stress relaxation and micro-structural dynamics in response to applied step strains below and above the macroscopic yielding transition, (ii) their macro- and micro-structural creep dynamics in response to applied shear stresses, and (iii) their ability to acquire micro-structural and mechanical memory in response to applied oscillatory strain histories. These studies provide insights into the nanoscale origins of non-equilibrium phenomena in driven soft glassy systems.
[1] R.L. Leheny, M.C. Rogers, K. Chen, S. Narayanan, and J.L. Harden, “Rheo-XPCS,” Curr. Opin. Colloid Interface Sci. 20, 261 (2015).
Classical experiments, typically performed using bulk continuous matter can be applied for granular systems to better understand their properties, and explore the analogies between granular and bulk continuous systems. While the classic pendant drop experiment can be
used to measure the interfacial tension between fluids, here we perform the granular version of the pendant drop experiment. The system consists of aggregates of adhesive, monodisperse, frictionless oil droplets in an aqueous solution. Depending on the system parameters, the properties of aggregates resemble both liquid-like and solid-like systems.
Electrohydrodynamics of droplets immersed in an immiscible carrier fluid was first explored in a pioneering paper by G. I. Taylor who formulated the weakly conducting or leaky dielectric model and predicted the steady drop shape in the small-deformation limit. Contemporary literature in electrohydrodynamic studies focuses primarily on the deformations of single droplets. On the other hand, the collective behavior of many droplets shows a wide range of surprising phenomena. In the presence of a DC electric field, a multitude of unstable, chaotic, and turbulent behaviors are observed.
In this work, we use new substances for the continuous leaky dielectric phase and discrete dielectric phase. This opens new doors of possibilities to the experiments in electrohydrodynamics, with lower threshold voltages. The lower voltage thresholds enable new electrorheology experiments to be conducted, the results of which will be reported.
Single photon sources play a critical role in many emerging applications in quantum information science. Single photon quantum computing [1], and single photon quantum cryptography [2] both rely heavily on high-brightness, and high-indistinguishability single photon sources where subsequent single photons are identical in all degrees of freedom. In order to maximize indistinguishability, the quantum emitter must be driven resonantly so that incoherent relaxation pathways are eliminated. This, however, necessitates an efficient method for separating the single photons from the scattered excitation light. We present a novel driving scheme called Notched Adiabatic Rapid Passage (NARP) [3] where a frequency swept optical pulse containing a spectral hole resonant with the quantum emitter is used. The frequency-swept nature of the pulse allows the scheme to retain the benefits of Adiabatic Rapid Passage (ARP), including robustness to variations of the properties of pump laser and quantum emitter. It also enables the suppression of decoherence tied to electron-phonon coupling [4]. The spectral hole allows for the single photons to be spectrally filtered from the scattered laser light. Together, this excitation scheme would enable <10-8 scattered photons per single photon emission with a detection loss of 4%. We have demonstrated this scheme in a single semiconductor quantum dot.
[1] Madsen, L. S., et. al. Quantum computational advantage with a programmable photonic processor. Nature, 606(7912), 75-81 (2022).
[2] Bozzio, M., Vyvlecka, M., Cosacchi, M. et al. Enhancing quantum cryptography with quantum dot single-photon sources. npj Quantum Inf 8, 104 (2022).
[3] Wilbur, G. R., Binai-Motlagh, A., Clarke, A., Ramachandran, A., Milson, N., Healey, J. P., O’Neal, S., Deppe, D. G., Hall, K. C. Notch-filtered Adiabatic Rapid Passage for Optically-Driven Quantum Light Sources. APL Photonics (in press) (2022).
[4] A. Ramachandran, G. R. Wilbur, S. O’Neal, D. G. Deppe, and K. C. Hall, "Suppression of decoherence tied to electron–phonon coupling in telecom-compatible quantum dots: low-threshold reappearance regime for quantum state inversion," Opt. Lett. 45, 6498-6501 (2020)
High quality, uniform thin films of quantum materials are of extreme importance across many classes of device research. Minimizing energy consumption, while keeping flexibility in the deposition process, along with high structural stability, electrical and thermal conductivity, and optical transparency is critical in designing a reactor for quantum material thin film growth. Ultra-thin films based on tungsten semi-carbide (W2C) are excellent candidates as quantum materials with startling properties such as theoretically predicted negative Poisson’s ratio.[1] However, chemical-vapour thin-film deposition (CVD) techniques have not been reported to yield bona fide W2C films, arguably because they operate under thermodynamic equilibrium conditions, where the stable phases are segregated tungsten and carbon, or the carbon-rich WC. Here, we report of the synthesis of highly crystalline few-layer W2C, achieved using an ad-hoc designed remote plasma vapour deposition (RPVD) ultra-high vacuum reactor. The reactor built by us for this study generates tungsten ions from a 13.56 MHz radio frequency biased 2” target inductively coupled with hydrocarbon species from the ionisation of methane at ~10-6 mbar (~10-9 mbar base vacuum). The so achieved plasma is injected in a high-temperature furnace (900oC) where substrates are placed, by a 10-kV DC accelerating voltage. X-ray diffractometry, scanning tunneling microscopy, and elemental analysis have confirmed few-layer W2C crystals in the deposits, with decreasing thickness in backstream mode deposition, with the addition of varying amounts of Ar ions in the forward gas stream. Dramatic advantages of our high-vacuum RPVD deposition system rests in the high crystallinity of our deposits, where tungsten carbides without W2C structure (i.e. WC, or amorphous) were obtained by CVD or less advanced plasma deposition systems.[2]
[1] Wu et al, Phys. Chem. Chem. Phys., 2018, 20, 18924
[2] Baklanov et al, Mater. Res. Express, 2020, 9, 016403
Thermal transport in low-dimensional systems such as nanowires is interesting for applications involving system design at the nanoscale, but the effects of changes like the shape of a nanowire are not completely understood. In this work the behaviour of the thermal conductance of nanowires is investigated by introducing a single kink into an otherwise straight nanowire. The angle of this kink is varied to examine its effects on thermal transport. Kinked systems are constructed and simulated using Molecular Dynamics simulations, phonon Monte Carlo simulations and classical solutions of the heat equation. The effects of lattice orientation within the kink are found to be significant, but an examination of the heat flux field reveals additional complexities. Details of transport modeling, ratio of mean free path to characteristic system size, phonon reflections and system specularity yield differences in thermal behaviour throughout the systems. Comparing the heat flux between phonon Monte Carlo and classical solutions of the heat equation finds that the heat flux in systems where the mean free path of phonons is large compared to the system dimensions (such as those in the Monte Carlo simulation) may have heat flow concentrated in a channel smaller than the dimensions of the system.
The ATLAS experiment recorded 140 ifb in the LHC’s $\sqrt{s}$ = 13 TeV Run 2, and the analysis of this high-quality and well-understood dataset continues. Canadian physicists are involved in all aspects of data analysis, from the trigger systems to reconstruction to physics results. Recent results, including highlights from Higgs properties and precision measurements of the Standard Model, as well as searches for new physics, will be discussed.
Electron objects are used in a large fraction of ATLAS publications. Better identification implemented in the electron triggers would allow to lower their transverse momentum threshold and increase their acceptance. In particular, analysis with many electrons in the final state such as the ones studying the Higgs, the W boson or Beyond de Standard Model phenomena can suffer from large, sometimes dominant, fake or non-prompt electron background and would benefit from improved electron identification.
To address this problem, our group developed a convolutional neural network (CNN) to identify electrons in ATLAS. Our CNN shows significant improvement in performance when compared to the algorithms currently used in ATLAS for electron identification. Our first iteration of the CNN is trained using a Monte Carlo simulation (MC) sample, and we aim to improve even further the performance by designing a real data sample to train our CNN on.
With that goal in mind, we study a real data sample pure in background electrons and compare it to the MC we used for training the first CNN. We show that such sample can be obtained by applying various trigger, and transverse energy and pseudo-rapidty cuts. We show that the distributions of the various high level input variables differs between the two datasets, particularly at low transverse energy. We then find similar results when comparing the mean calorimeter images of each dataset.
We conclude that the low transverse energy region is imperfectly modelled by the MC and thus, training a CNN in real data should yield substantial improvements in performance.
The international CALICE collaboration is dedicated to detector R&D in calorimetry for new experiments. All project concepts now use high granularity to maximally profit from Particle Flow Algorithms and thus improve jet energy resolution, device versatility and response performance. A review of innovative analog or digital detector types, using technologies such as silicon, scintillators or resistive plate chambers, will be presented, as well as results from recent work realized in Canada.
The Belle II experiment, based at SuperKEKB, is collecting e+e- collision data at the Upsilon(4S) resonance energy. The Belle II physics program is enabled by the (all-time high) record luminosity of SuperKEKB; a metric that also incurs record high beam background in the detector. Accurate simulation of physics events in the detector during collisions is vital to obtaining quality physics results.
The effects of beam background are currently represented in simulations by overlaying background data measured randomly during data taking. The large size of these background data samples is a technical problem; they are challenging to use on distributed computing grids. As Belle II approaches higher luminosity, saving and using data samples will become unsustainable. An alternative scheme where data-like beam background samples are generated in lieu of data samples directly while simulating is necessary to continue producing the quality simulations essential for the Belle II physics program.
The novel generative adversarial network (GAN) implemented in the Belle II electromagnetic calorimeter (ECL) is capable of simulating data-like background waveforms in the 8736 CsI(Tl) ECL crystals, which will mitigate this problem. GANs can be used in High Energy Physics (HEP) experiments as a novel simulation method to generate random yet accurate background waveforms on the fly from lightweight neural networks that can be overlayed onto more complex physics simulations such as those coming from GEANT4. This talk will show GAN designs at Belle II, their training framework and the tests performed to determine their performance.
The analysis of collision events at the Large Hadron Collider (LHC) presents significant computational challenges, particularly due to the need for large amounts of Monte Carlo simulation to reduce statistical uncertainties in the simulated datasets. The most computationally intensive task in Monte Carlo detector simulation is the simulation of high-energy particles interacting with the calorimeter. In this work, we propose a novel approach that combines recent advancements in generative models and quantum annealing techniques to provide fast and efficient simulation of high-energy particle-calorimeter interactions. Our approach, the Quantum Variational Encoder (QVAE), utilizes a Variational Autoencoder (VAE) model with a Restricted Boltzmann Machine (RBM) prior implemented on an annealing Quantum Processing Unit (QPU). The quantum annealing QPU can generate a large number of samples from the latent space of a trained VAE model with high efficiency. We show the performance of the QVAE on simulated calorimetric cluster data. The promising evaluation results demonstrate the accuracy and reliability of our Quantum Variational Encoder. Furthermore, our proposed approach has the potential for significant improvement by extending it to use QPU samples during the training process, enhancing the computational efficiency even further.
In order to make new discoveries within the realm of particle physics it is imperative that we are able to compare data collected using the ATLAS detector with theoretical predictions as well as results from other experiments. The process of correcting ATLAS data such that the effects of the detector are eliminated is known as unfolding. At present, commonly used unfolding methods require data to be binned and are typically performed with low dimensionality. With recent advances in machine learning, however, it has become possible to perform unfolding with unbinned, high dimensional data. The method examined here, known as the OmniFold technique, utilizes iteratively trained neural networks to accomplish this task. In this presentation, the results for the first unbinned, 24 dimensional measurement with full uncertainties is shown. This measurement is performed using the full Run 2 proton-proton collision dataset recorded by the ATLAS detector and examines Z+jets events where the Z boson decays to two muons. Various observables related to the dimuon kinematics, track jet kinematics and track jet substructure are included in the unfolding. A select number of observables that may be derived after the unfolding are also examined.
Darkside-20k, planned to be constructed at the LNGS underground laboratory in Italy, is a forthcoming detector that aims at using a Liquid Argon (LAr) target to detect the scattering of dark matter particles from argon atoms. The detector will collect an exposure of 200 tonne-years while keeping the instrumental background level in the WIMP search region of interest to a minimum.
At the center of the detector, a two-phase Liquid Argon Time Projection Chamber (LArTPC) will be filled with low-radioactivity Underground Argon (UAr) with a 20-tonne active volume. The TPC barrel will be made up of eight gadolinium (Gd) loaded PMMA (acrylic) panels. The acrylic anode and cathode plates of the TPC barrel will be coated with Clevios to realize the electrical potentials in the TPC and with 1,1,4,4 tetraphenyl-1,3-butadiene (TPB) to wavelength shift the 128 nm argon scintillation light to ≈420 nm which is necessary for the Silicon Photomultiplier (SiPM)–based readout to detect light.
The thermal vacuum evaporation method is the most common way to deposit TPB on the acrylic time projection chamber. For Darkside-20k, a system with multiple point sources to coat the TPC barrel is proposed and, in this talk, I will present how using more than one point source can improve the uniformity of the TPB coatings. I will also talk about other important parameters that can affect the uniformity of the coatings.
The Cryogenic Underground TEst facility (CUTE) is located 2 km underground at SNOLAB in Sudbury, Ontario. The response of cryogenic germanium and silicon semiconductor detectors is characterised through testing at CUTE prior to use in the Super Cryogenic Dark Matter Search (SuperCDMS) experiment. SNOLAB and CUTE together provide a low background environment for testing, shielded from cosmic rays and other interfering radioactive backgrounds. CUTE currently has two sources available within the facility for gamma calibration, used to characterise the high voltage detector response. iZIP detectors being tested in the coming years will need a neutron calibration source available to characterise their response.
Transportation of radioactive sources within SNOLAB is a process requiring advance planning in order to notify other experiments about the possible presence of unaccounted for radioactive sources. Due to the ever-changing nature of any experimental work this process can cause further delays when testing cannot be done promptly as needed. The CUTE neutron calibration system is built to solve this issue. The system uses a californium 252 source which is pulled by a motor through a tube located within the shield water tank, allowing the location of the neutron source to be controlled remotely. Testing for the system has begun with implementation foreseen in September 2023. This talk will discuss the commissioning and applications of the neutron calibration system at CUTE.
The detection of dark matter (DM) is currently one of the leading challenges in particle physics. While many experiments attempt to detect dark matter in a variety of ways, the DEAP-3600 experiment uses roughly 3.3 tonnes of liquid argon in an attempt to detect the scintillation signal produced by a dark matter particle scattering on an argon nucleus. DEAP-3600 uses pulse shape discrimination to reject electromagnetic backgrounds by taking advantage of the difference in the time over which scintillation light is produced for various types of incident radiation and subsequently detected in the 255 photomultiplier tubes imaging the detector. The ability to understand and reject background interactions in the detector is key in ensuring a low-background dark matter search region.
In this talk, we discuss progress made on measurements benefiting current DM experiments like DEAP-3600 as well as future liquid argon detectors using Argon-1. Argon-1 is a modular single phase liquid argon detector located at Carleton University in Ottawa, Ontario, instrumented with two silicon photomultipliers (SiPMs) used to detect the scintillation light. We discuss pulse shape discrimination techniques employed using SiPMs, as well as studies on alpha particle quenching.
The Deep Underground Neutrino Experiment or DUNE is an ambitious accelerator based neutrino oscillation experiment that is not only able to resolve the mass hierarchy, but also has excellent potential to measure the charge-parity violating angle in the neutrino sector. DUNE will constrain systematic uncertainties by building a suite of detectors close to the neutrino source (near detector) and another at a distance of 1300km away (far detector). In DUNE, this Near Detector suite consists of three main components. Here the focus will lie on the Liquid Argon Near Detector or ND-LAr, which is built with a novel pixelated charge readout system. ND-LAr is a modular design of 35 identical LAr TPCs assembled in a 7 by 5 array. To prove the viability of this concept, a chain of prototypes has been constructed and tested with cosmic rays; From singular modules (60cm x 120cm x 60cm) to ultimately combining them in a 2x2 array in the NuMI neutrino beam at Fermilab. With a pixel pitch of 4.4mm in three of the four modules and a pitch of 3.8mm in the fourth, there are more than 300k readout channels across the 8 drift volumes. This talk will describe the characteristics of these modules and their responses to incoming charged particles by studying the pixel performance and the particle track widths. These studies will help us understand the differences between the modules in terms of the respective drift fields applied within them and the charge collection efficiencies.
The Hyper-Kamiokande (HK) is a next generation neutrino detector that will require new detector technologies and percent-level calibration to achieve its full physics potential. To achieve this goal, a 50-ton scale Water Cherenkov Test Experiment (WCTE) has been proposed and is scheduled to be installed at the T9 test beam experimental area in CERN, with the run starting in summer of 2024. To understand and characterize the T9 beam, several small detectors have been designed, including a Time-of-flight (TOF) detector, Aerogel Cherenkov Threshold (ACT) detectors, hole counters, and hodoscopes. These detectors will be placed between the beam-target stage and the WCTE water tank. However, the presence of these intermediary materials will modify the momentum and position distribution of the incoming T9 beam. To study these modifications, a dedicated Geant4 simulation has been performed, and the results will be discussed in this talk. Overall, this simulation aims to improve the accuracy and effectiveness of the WCTE detector by providing a better understanding of the T9 beam and its interactions with intermediary materials.
The Hyper-Kamiokande project plans to measure the phenomenon of neutrino oscillations with unprecedented precision, at the 1% systematic uncertainty level or less. To do so, multiple water cherenkov detectors will be deployed: near and far detectors, as well as a test experiment (WCTE) for the testing of new technologies and improvement of physics understanding. These detectors will use multi-photomultiplier tube (mPMT) modules, each of which consists of nineteen 3'' PMTs for the detection of cherenkov radiation produced by the resultant charged particle from a neutrino interaction. These mPMTs are under development at multiple locations. A number of measurements have been done on the modules, including optical tests to understand light-collection capabilities before and after the inclusion of additional reflective material on the PMT cups, pressure tests to measure the amount of deflection of the mPMT components at various water depths, and mechanical tests on the gel that optically couples the PMTs to the acrylic dome covering the module. This presentation will discuss these measurements, as well as provide an overview of the mechanical components and electronics that comprise the modules.
There exists a large body of indirect evidence for the existence of Dark Matter (DM) but, to date, no direct evidence has been found. Because of this, the wide range of possible parameter space that would then be used to explain dark matter’s observed effects has given rise to a large number of models. One possible form of DM is strongly self-interacting DM, which includes Strongly Interacting Massive Particles (SIMP), modeled after Quantum Chromodynamics (QCD). To narrow down possible models, direct detection of dark matter at accelerators is a high priority. Detecting or ruling out some possible DM models is a part of the experimental program for the MoEDAL experiment located at the LHC. The MAPP extension to the MoEDAL experiment, now approved for run 3, focuses on searching for Mili-Charged Particles (mCPs), and Long-Lived Particles (LLP). In this talk, we will discuss meson-like SIMP, and their potential detectability at the MoEDAL MAPP experiment. In order to model this DM, we construct a Lagrangian describing dark-pions using an approach inspired by Chiral Perturbation theory, an effective field theory of QCD. In addition to strong self interactions, our meson like DM also couples to dark gauge fields. To couple our model to the Standard Model, we include a vector portal term which kinetically mixes our dark gauge fields with standard model gauge fields. As part of our model, we also include a Wess-Zumino-Witten term, this term is important to control the overproduction of strongly self-interacting DM in the early universe. We focus on two processes: a Drell-Yan process involving a dark gauge field, which produces a pair of dark-pions, and photofusion of two dark photons to three dark-pions. Due to kinetic mixing, these dark-pions will have an effective electric charge that is a small fraction of that of the electron.
The far-infrared spectrum of CD$_{3}$SH has been recorded from 60 to 450 cm$^{-1}$ at the FIR beamline of the Canadian Light Source in Saskatoon in order to explore the evolution of the torsional structure in climbing up the ladder of torsional states. So far, the torsion-rotation levels have been extensively mapped up to the third excited torsional state, and we hope to push the assignments further up to the v$_{t}$ = 4 state and beyond to where the ground torsional ladder is passing through the lower vibrational levels with the possibility of interesting torsion-vibration interactions. Here the torsional levels are high above the potential barrier to internal rotation and are essentially free rotor states following the parabolic curves of our “Universal Spectral Predictor”. We wish to explore how well the free rotor pattern can be modeled in order to gain predictive power for extrapolation up to higher states and potentially address the long-standing torsional problem of simultaneous global fitting of ground and vibrational states.
Authors fabricated a unique plasmonic structure using gold nanorods (GNRs) along the length of a tapered fiber using a well-known phenomenon called “Optical tweezing”. The plasmonic structure, known as an optical fiber probe, was used to detect chemicals at lower concentrations. Surface-enhanced Raman spectroscopy (SERS) technique was used to obtain the data for chemicals adsorbed on the probe. The fiber probe was manufactured using a dynamic etching process. We will present the Raman spectra of Rhodamine 6G and Crystal Violet (CV), extensively used in the food and textile industry. Manufacturers use CV in aquaculture for its anti-parasitic and anti-microbial properties, which help prevent diseases and infections in fish and seafood farming. The usage of CV contains elevated toxicity levels, and the residue is strictly forbidden in food due to potential carcinogenic and mutagenic properties that pose a potential threat to both human and aquatic life. R6G is a synthetic dye commonly used in the food industry to provide color to various food products such as candies, energy drinks, sauces, dressings etc., as well as in the textile industry that uses massive amounts of dyes which is a major cause of water pollution. The manufactured probe is reliable, sensitive and compact. The “dip and dry” technique was used to adsorb analytes (R6G and CV) with different concentrations on the gold-nanorods coated fiber probe. The results based on GNRs (aspect ratio 3.8 and longitudinal surface plasmon resonance (LSPR) wavelength 785 nm, Nanopartz, USA) show that the minimum concentrations detected for R6G and CV were 10-12 M and 10-11 M, respectively.
Authors demonstrated a passively Q-Switched pulse laser by using an aqueous solution of colloidal gold nanorods (GNRs) and Poly vinyl Alcohol (PVA) as a Saturable Absorber (SA) in a fiber ring laser cavity. GNRs, due to its unique plasmonic and nonlinear properties, has the potential to generate ultrashort pulses. In addition, a tunable laser can be developed using a mixture of GNRs with different lengths (aspect ratios = length/diameter). However, the application of GNRs is limited in developing high-power lasers due to their low damage threshold. The aqueous solution used in the experiment increased the damage threshold of the GNRs, and their shape remained intact after prolonged exposure to high power. The heat accumulated in the GNRs can dissipate in the surrounding medium in less time than the time required to deform the shape of GNRs responsible for the plasmonic properties. PVA provided stability to the solution and restricted the accumulation of GNRs in the solution, resulting in uniform distribution of GNRs, which was examined in TEM images. The density of GNRs was increased in the aqueous solution to increase light absorption. Q-Switched pulses were generated having a width, repetition rate and average power of 9.2 µs, 21.5 kHz, and 3.25 mW, respectively, at 1560 nm central wavelength. The authors will present the design of the laser cavity, the process of preparing SA and Experimental results, which include TEM images showing the distribution of GNRs in PVA at different concentrations.
We will report on the development of efforts to create new spectroscopic reference data to help astronomers to find exoplanets. Astronomers routinely observe spectra of the molecule iron hydride (FeH) in the atmosphere of M-class stars. By measuring the Doppler shifts of transitions in FeH, they can determine a star’s radial velocity. If a star has an exoplanet, the star and the exoplanet will orbit their common center of mass inducing a periodic frequency wobble in the star’s FeH spectrum. However, M-class stars often have strong magnetic fields that modify its FeH spectrum through Zeeman splitting. While the infrared transition of interest (E$^4$Π- A$^4$Π, ~ 1600 nm) has been studied in detail, its response under magnetic field has not been studied in the lab, although it has been observed in sunspots (A. Asensio Ramos et al., 2004). Hence astronomers require an FeH spectrum to interpret their stellar observations when there is non-negligible magnetic field.
We are creating FeH in the lab to study the response of the E$^4$Π and A$^4$Π states to controlled magnetic fields. Transitions involving E$^4$Π and A$^4$Π are accessed through new higher-lying states that we have recently discovered. One of the new states is accessible from the ground state, X$^4$Δ, via laser excitation spectroscopy in the green region (~ 510 nm) and fluoresces to both the E$^4$Π and A$^4$Π states. Thus, we can obtain information about the infrared transition indirectly through Zeeman spectroscopy of the visible transitions. The second new higher-lying state is assigned as the (2)$^4$Φ state. This state is also accessed from the ground state (~ 515 nm) and fluoresces very strongly in the red (~ 625 nm) to the previously observed C$^4$Φ state.
Laser-cooled molecules exhibit several features that make them attractive virtual laboratories for probing new physics Beyond the Standard Model (BSM). Various proposed extensions to the Standard Model predict non-zero values for the electron's Electric Dipole Moment (eEDM). To date, no experiment has measured a non-zero eEDM; however measurements placing an upper bound on the value for the eEDM provide an experimental check on potential new physics theories. YbOH has recently been suggested as a molecule of interest in the search for BSM physics due to its large effective internal EM fields. Despite this interest, laboratory spectra of its isotopologue YbOD have remained elusive until now. We present our analysis of the first high-resolution LIF spectra of $^{174}$YbOD.
discussion & networking opportunities for session close out
Hyperpolarized (HP) gas MRI was previously developed to provide a way to study whole lung ventilation, alveolar morphometry and gas-exchange, with the first demonstration of 129Xe MRI lung imaging nearly 30 years ago. In the ensuing decades, HP gas MRI research has demonstrated that inhaled HP gas lung MRI provides unique measurements for a number of pulmonary diseases including chronic obstructive pulmonary disease (COPD), cystic fibrosis, asthma, lung cancer, and COVID. This MRI approach allows for visualization and quantification of lung units that participate in ventilation, and differentiating them from non-ventilating regions. This non-invasive, rapidly acquired and radiation-free lung imaging method, provides direct, spatial measurements of lung structure, function, and gas exchange down to the alveoli and acinar ducts.
HP gas 129Xe MRI has been recently FDA approved which means that this imaging technique is now a clinical-tool in USA. It is expected that Canada will also approve this method in near future. 129Xe lung MRI is extremely powerful and the only radiation-free tool for lung structure and function measurements. The proposed program and requested infrastructure will provide new tools for accurate lung damage assessment, therapy guidance, and evaluation of treatment outcomes. This is not only critical for the almost 6 million Canadians with asthma (3.8 million) and COPD (2.0 million), but also to the 3.5 million Canadians who were infected by COVID-19 in 2020 - 2022 and experienced lung damage (up to 10% infected) as a result. They will require longitudinal observation of the lung structure and function to best understand and manage the short and long-term health effects and to determine the impact of treatment strategies. The new tools being developed here will enable this.
There are a number of benefits associated with 129Xe brain MRI. First, 129Xe MRI brain perfusion images show a larger area of the brain affected by stroke compared to the traditional proton MRI, which can be an important and more accurate second stoke predictor, keeping in mind, that stroke is the 3rd leading cause of death in Canada and the 10th largest contributor to disability-adjusted life years (the number of years lost due to ill-health, disability or early death). As such, having these tools is so important in the management and prevention of stroke.
The brain is made of billions of cells called neurons, which are responsible for conducting electrical signals between the central nervous system and the rest of the body. The axon is the thread-like projection of the neuronal cell body and is usually insulated by the myelin sheath. The two hemispheres of the brain are connected by a white matter tract called the corpus callosum and the degeneration and dysfunction of axons within this brain region is indicative of many disorders, including Multiple Sclerosis. Such degeneration can be seen in the decreasing diameters of axons within the corpus callosum.
Current methods for measuring axon diameters require ex vivo tissue samples and electron microscopy analysis. Recently, Magnetic Resonance Imaging (MRI) is proving to be a useful tool for measuring axon diameters. Oscillating Gradient Spin Echo (OGSE) MRI pulse sequences can be used to probe micron-sized structures within the sample. This project investigated the use of OGSE sequences to measure axon diameters in the mouse corpus callosum. A CDI (Clostridioides difficile Infection) male mouse was anesthetized using isoflurane and perfused according to University of Winnipeg and Manitoba CACC protocol. Following sacrifice, the mouse brain in skull was isolated then soaked in paraformaldehyde for 48 hours, followed by phosphate-buffered saline for another 48 hours prior to imaging. The mouse brain was then transferred to a holding tube filled with Fomblin and the tube was placed inside the 21 cm horizontal bore 7 Tesla Bruker Magnet. Images were registered, ROIs were drawn in the corpus callosum, and axon diameters within the corpus callosum were inferred using custom-built Matlab code.
Axon diameters in various regions of the corpus collosum were inferred to be 5.4±0.8µm, 5.3±0.7µm and 6±1 µm. MRI using OGSE pulse sequences can probe micron-sized axons in fixed biological tissues. The next step is to reduce the uncertainty in the measurements.
The authors would like to acknowledge funding from NSERC and Mitacs, as well as assistance with animal care from Rhonda Kelly.
Approximately 1 in 6 people globally are affected by a Neurological disorder. Previous research has linked numerous Neurological disorders post-mortem to abnormalities in axon distribution and integrity within neural white matter tracts. Therefore, it is of high interest to investigate methods that will eventually be able to measure axon diameters in white matters tracts in live brains. This would allow for the development of new clinical applications such as earlier diagnosis and allow for the development of new treatments. Diffusion MRI is a method with the potential to infer microstructure in live brains using temporal diffusion spectroscopy (TDS). TDS, when used with certain pulse sequences, such as Oscillating Gradient Spin Echo (OGSE), can be used to infer micron-scale axon diameters. To calibrate TDS with OGSE, an ex vivo mouse brain was imaged and analyzed in this project and many substructures were studied to assess the differences within a mouse. The images were collected using a 7T Bruker AvanceIII NMR system with Paravision 5.0 and were processed and analyzed using MATLAB. The mean diameter inferred of axons in the corpus callosum ranged from 2.6 ± 3.4 μm to 5.6 ± 1.0 μm, with an average of 5.3 ± 0.2 μm. The next step is to increase the precision of the measurements with the goal of being able to measure axon diameters in in vivo mouse brains.
The authors wish to acknowledge Rhonda Kelley for her help with animal care and imaging. The authors acknowledge funding from NSERC and Mitacs.
Magnetic resonance imaging (MRI) is a powerful imaging technique for diagnosing disease. One major drawback of currently available MR systems is the cost of the high-field (>1T), general use magnets that are the current clinical standard. Thus, interest has grown in developing smaller, low-field, and diagnosis specific MR systems. These systems can reduce costs, and increase the accessibility of MRI by allowing MR systems to be used as part of bedside care. To aid in the design of new MR systems, we have developed the Numeric Integrator for the Bloch Equations (NIBLEs). NIBLEs is a Python 3 based simulation tool for simulating varied MR sequences and magnet configurations, with the aim of identifying the optimal system characteristics for a given use case to serve as a starting point for the development of specialized MR systems.
The NIBLEs toolset itself is divided into two main components; a toolset for defining sample properties to be used in later simulations, and a toolset for simulating MR hardware and experiments. The sample toolset allows a user to build a sample composed of spatially distributed magnetization vectors with varied properties used to simulate proton density, chemical shift, and NMR relaxation times. Meanwhile, the main simulator allows users to script an MR pulse sequence using functions that define the applied magnetic fields from the constituent components of an MR system (e.g. gradient coils and radiofrequency coils). This script provides the applied field and sample properties to the core solver, which uses a Runge- Kutta algorithm to numerically solve the Bloch equations to reproduce the signal space output of that experiment. Simulations will be presented to illustrate the capabilities of the NIBLEs solver to produce realistic results for NMR experiments, and MRI imaging protocols including Turbo Spin Echo and Gradient Echo imaging.
The weak mixing angle can be measured in parity-violating elastic electron-proton scattering. The aim of the P2 experiment is a very precise measurement of the weak mixing angle with an accuracy of 0.15% at a low four-momentum transfer of Q2 = 4.5x10^{-3} GeV^2. In combination with existing measurements at the Z pole with comparable accuracy, this comprises a test of the standard model with a sensitivity towards new physics up to a mass scale of 50 TeV. In addition to the measurement using a liquid hydrogen target, other targets, such as carbon and lead, are considered for measuring parity-violating elastic electron scattering. The experiment will be built at the future MESA accelerator in Mainz. In this talk, the motivation and challenges for these measurements will be discussed.
High Voltage Monolithic Active Pixel Sensors (HVMAPS) are a new type of electron detector. This hybrid pixel detector combines the semiconductor sensor elements that detect high energy particles with the readout electronics in one element. The demand for fast, high resolution and low noise detectors by experiments conducted at the LHC initiated the development of hybrid pixel detectors, first being developed at CERN in the 1980s [1]. Each pixel has its own integrated readout electronics. The manufacturing process provides high levels of customization like radiation thickness and radiation length, thereby allowing the control of material budget for detectors, where scattering could be an issue. HVMAPS have been used as detectors for the Mu3e experiment [2]. As thin as 50 microns, the latest version of the HVMAPS, (MuPix Version 11) are the ideal electron detector for applications in the MOLLER experiment at Jefferson Lab [3], The experiment proposes to measure the asymmetry of parity violating scattering, APV, in polarized electron-electron scattering, thereby measuring the Weinberg angle to a greater precision. This presentation outlines the use of HVMAPS in two aspects of the experiment: the Compton polarimeter, and the main detectors, for tracking the path and position of electrons respectively.
[1] Philip Garrou, C Bower, and P Ramm. Introduction to 3d integration. In Handbook of 3D Integration Vol 1-Technology and Applications of 3D Integrated Circuits. Wiley-VCH, 2008.
[2] Niklaus Berger, Mu3e Collaboration, et al. The mu3e experiment. Nuclear Physics B-Proceedings Supplements, 248:35–40, 2014.
[3] Mammei, Juliette. "The MOLLER experiment." arXiv preprint arXiv:1208.1260 (2012).
The TRIUMF Ultracold Advanced Neutron (TUCAN) source, when completed, will be a world-leading source of ultracold neutrons. The source is a unique combination of a spallation target coupled to a superfluid helium converter. A key component of the source is the liquid deuterium moderator, which surrounds the superfluid helium converter. The goal of the LD$_2$ moderator is to provide a high flux of cold neutrons into the superfluid, where they are then downscattered to become UCN. The liquid deuterium moderator has a 125 L volume, and experiences a heat load of 60 W for the design proton beam current of 40 $\mu$A. Cooling is provided by a distant cryocooler at higher elevation, in a thermosyphon loop with the moderator volume. The thermosyphon solution is unique in featuring no moving parts and single-phase (liquid) operation. This presentation will focus on the design of the liquid deuterium system, and the status and plans for this important component of the UCN source.
In order to search for the physics beyond the Standard Model at the precision frontier, it is sometimes essential to account for Next-to-Next-Leading Order (NNLO) corrections theoretical calculations. Using the covariant approach, we calculated the QED type leptonic tensor up to quadratic (one loop squared) NNLO (alpha cube) order, which can be used for the processes like (electron-proton) and (muon-proton) scattering relevant to MOLLER (background studies) and MUSE experiments, respectively. Recently we have used this approach for a hard photon bremsstrahlung process called "Bethe-Heitler". This is a 2->3 process where an electron scatters with a proton with the emission of a hard photon and is an important example in Quantum Electrodynamics (QED).
In this presentation, I will quickly review covariant approach and provide our latest results for quadratic QED electron-proton scattering along with the Bethe-Heitler process.
Performing measurements on anti-matter atoms is an alluring proposition for studying the symmetries between matter and anti-matter; however, it presents a number of technical challenges. The ALPHA group has met these challenges and successfully trapped large numbers of anti-hydrogen atoms, opening the door for many such measurements. The new ALPHA-g experiment has the ability to measure the gravitational force exerted by the Earth on these anti-hydrogen atoms, by counterbalancing this force with precisely controlled magnetic fields. By relaxing only the confinement along the gravitational axis, the anti-atoms are released into two “up” and “down” regions separated by tens of centimetres. Here they annihilate, and the ratio of counts in the two regions describes the overall – magnetic plus gravitational – bias.
Charged pions resulting from these annihilations are tracked in a time projection chamber; these tracks are fit and extrapolated back to a common annihilation vertex. Our ability to reconstruct the position of these annihilation vertices into the correct region was previously one of the limiting factors of the experiment. Here I present the steps taken to improve our position resolution beyond that necessary for the experiment.
Furthermore, due to the low number of anti-atoms produced and slow experiment timescale, cosmic rays produce a sizeable background in our time projection chamber. To mitigate this, a second plastic scintillator-based detector system was implemented, called the “barrel veto”. This was used to discriminate against the cosmic ray background based on event topology in the first data-taking run in 2022. It has the additional possibility of using time-of-flight to further identify background events. Here I present the usage of the barrel veto to reject the cosmic ray background, and demonstrate the overall effectiveness of the ALPHA-g detector system.
The ALPHA-g experiment at CERN aims to test the fundamental symmetry between matter and antimatter by precisely measuring the effect of Earth's gravity on antihydrogen atoms. To achieve this goal, the experiment uses a radial Time Projection Chamber (rTPC) as the primary detector for particle tracking. The rTPC provides a high spatial resolution of the antihydrogen annihilation vertices, which is crucial for a measurement of the interaction between antimatter and Earth's gravitational field. This presentation will discuss a simulation study of the rTPC's performance, which aims to quantify its spatial resolution, efficiency, and response to various experimental parameters. The study highlights the essential role of simulations in understanding systematics for future precision measurements. Specifically, the results demonstrate the importance of simulation studies in optimizing the performance of the rTPC and lays the groundwork for future investigations of the detector's tracking and vertex reconstruction algorithms.
The ways Physics and Astronomy are traditionally taught in Canadian Universities typically ignores millennia of knowledges of Indigenous Peoples. This is by design as textbooks and curriculum tend to build upon a European view of the growth of science, physics, and astronomy that centers one perspective. However, we can build a more diverse and improved curriculum by considering Indigenous methodologies, knowledges and stories in our research and teaching. In this talk I will reflect on experiences teaching an Indigenous centric astronomy course that considered Indigenous methods and the intersection of professional astronomy and colonization today. I will also offer insights into how physicists and astronomers can move to support inclusion and celebration of Indigenous knowledges in the classroom.
nEXO is a planned next-generation neutrinoless double beta decay experiment, designed to be at SNOLAB in Sudbury, Ontario, Canada. Within the international nuclear and astroparticle physics communities, we strive to be a leader and role model in the areas of Diversity, Equity, and Inclusion while drawing inspiration from the trailblazers who came before us. In 2018, nEXO wrote and adopted its Code of Conduct and created a standing Code of Conduct committee. In 2020, nEXO founded its Diversity, Equity, and Inclusion Committee. The nEXO-DEI committee has created a mentorship program, started an internal DEI lecture series, initiated an internal newsletter and information hub, and began surveying our own collaboration on ways that we can improve our culture. This talk outlines the works of these groups, the progress they have made, and where the future of DEI in the nEXO collaboration is headed.
Undergraduate research activities, strong mentorship and peer support have been demonstrated to improve the experiences of students studying science. This is especially important for Indigenous students for whom the transition from a high school setting, where students feel comfortable and may be embedded in robust Indigenous community, to university, which can be isolating and challenging. UWinnipeg has a large population of Indigenous students, and is uniquely situated to support and encourage Indigenous students in the sciences. This presentation will describe the suite of programs at UWinnipeg, namely the Pathway to Graduate Studies (P2GS) program for junior students and the Indigenous Summer Scholars program (ISSP) for students towards the end of their degree. In 2022 UWinnipeg helped develop a pilot program UWindsor. These programs offer a rich environment for research and scholarly success and a means to form a sense of community and belonging on campus. The P2GS program provides an opportunity for first and second year undergraduate students to upgrade their basic science skills, gain research experience in a university laboratory, and to form a network of peers, graduate students and faculty. The ISSP program matches senior undergraduate students with a research mentor to work on an independent research project. Both programs are deeply connected to and supported by the UWinnipeg chapter of the Canadian Indigenous Science and Engineering Society. I will also invite discussion about how these programs may be used as a model at other post-secondary institutions.
The authors thanks funding from NSERC PromoScience.
The Truth and Reconciliation Commission of Canada called on post-secondary institutions to integrate Indigenous knowledge and teaching methods into classrooms” (TRC, 2015). At the University of Windsor, there is a broad initiative to include Indigenous knowledge and ways of knowing in as many courses as programs as possible. I present the first attempt at indigenizing and decolonizing the physics curriculum at the University of Windsor. This involves the development of a brand-new second-year elective entitled 'History of Astronomy'. Throughout the development of the course, the goal of 'two-eyed seeing' was kept in mind. I will report on the challenges encountered and how we tried to meet these challenges.
TRIUMF, Canada’s Particle Accelerator Centre, delivers beams for fundamental science and a wide range of accelerator-based applications.
World-leading in radioisotope beam production, TRIUMF-ISAC is the only ISOL facility that is routinely operating targets under particle irradiation in the high-power regime in excess of 10 kW. TRIUMF’s current flagship project ARIEL, Advanced Rare IsotopE Laboratory, is adding two new target stations providing isotopes to the existing experimental stations in ISAC I and ISAC II at keV and MeV energies, respectively. In addition to the operating 500 MeV, 50 kW proton driver from TRIUMF’s cyclotron, ARIEL will make use of a 35 MeV, 100 kW electron beam from a new TRIUMF designed and built superconducting linear accelerator. Together with additional 200 m of RIB beamlines within the radioisotope distribution complex, this will put TRIUMF in the unprecedented capability of delivering three RIB beams to different experiments, while producing radioisotopes for medical applications simultaneously – enhancing the scientific output of the laboratory significantly.
To cope with the increased occupancy and radiation dose expected at the High-Luminosity LHC, the ATLAS experiment will replace its current Inner Detector with the Inner Tracker (ITk), containing all-silicon pixel and strip sub-detectors. The strip detectors will be built from modules each consisting of one or two n+-in-p sensors, one or two PCB hybrids containing the front-end electronics, and one powerboard. The sensors in the barrel region of the cylindrical ITk will use simple rectangular pixels, while those in the circular endcaps will use a radial pixel layout.
To validate the expected performance of the ITk strip detector, a series of testbeam campaigns has been performed over several years at the DESY-II electron accelerator. Beam particles are tracked by EUDET telescopes, consisting of six high-resolution pixel detectors, plus an additional fast detector to improve timing resolution. Tracks are reconstructed with a spatial resolution of several microns, and compared to hits in the module under test. To evaluate the end-of-life performance of the ITk, modules from different regions of the detector have been built using sensors and/or front-end electronics irradiated to the maximum dose expected in the HL-LHC, plus a 50% safety factor, and measured in the testbeam to assess charge collection, signal efficiency, and noise occupancy. The results of this analysis give confidence in the detector meeting specifications across its operational lifetime.
The ABCStar (ATLAS Binary Chip – Star Version) is a front-end readout chip for the silicon-strips portion of the ATLAS Inner Tracker (ITk) upgrade. These radiation-hard application specific integrated circuits (ASICs) are implemented in a commercial 130 nm CMOS process and are intended to handle the high rate of collision data at the High Luminosity LHC (HL-LHC), and last throughout the lifetime of the detector. Over 350,000 ABCStar ASICs need to be extensively tested to ensure that chips used for sensor module assembly follow all design specifications.
Conventionally, electronics for particle physics experiments have been tested using custom equipment in dedicated research facilities that allow for extensive research and experimentation. Rather than duplicating this approach, Carleton partnered with DA-Integrated, a specialist ASIC testing company in Canada, to implement an industrial-standard wafer testing program for the first time in a particle physics detector project. By leveraging their expertise and infrastructure we were able to obtain large improvements in throughput compared to existing approaches, without compromising test coverage or data collection. In addition, the enhanced wafer testing capabilities at DA-Integrated allowed for a detailed investigation of the digital performance of the ABCStar under different duty cycles and supplied voltages. These results were used to determine the operational window of the ABCStar to prevent data loss in the detector.
Production probing of the ABCStar is underway, with Carleton set to test half of the ABCStar ASICs required for ITk. Collaborating with DA-Integrated has bridged the methodological, technical and semantic gap between research facilities and the semiconductor testing industry. This will open new possibilities for ASIC testing in future particle physics projects.
New neutron sources are needed both for Canada and internationally as access to reactor based neutrons shrinks. Compact Accelerator-based Neutron Sources (CANS) offer the possibility of an intense source of pulsed neutrons with a capital cost significantly lower than spallation sources. In an effort to close the neutron gap in Canada a prototype, Canadian compact accelerator-based neutron source (PC-CANS) is proposed for installation at the University of Windsor. The PC-CANS is envisaged to serve two neutron science instruments, a boron neutron capture therapy (BNCT) station and a beamline for fluorine-18 radioisotope production for positron emission tomography (PET). To serve these diverse applications of neutron beams, a linear accelerator solution is selected, that will provide 10 MeV protons with a peak current of 20 mA within a 5% duty cycle. The accelerator is based on an RFQ and DTL with a post-DTL pulsed kicker system to simultaneously deliver macro-pulses to each end-station. This study compares the performance of various DTL solutions including Alvarez, CH, and APF structures.
The Off-Line Ion Sources (OLIS) facility is part of TRIUMF’s world-class Isotope Separator and Accelerator (ISAC) complex, specializing in nuclear and particle physics research. Delivery of stable beams from OLIS and rare isotope beams from ISAC and eventually ARIEL (the Advanced Rare Isotope Laboratory) to various experiments with desired intensity and quality requires a complex tune of many independent parameters, over a lengthy, manual procedure.
Here we present first results of tuning the OLIS beamline using Bayesian optimization, a state-of-the-art machine learning algorithm to maximize black-box functions. It takes advantage of probabilistic modeling using Gaussian processes with an iterative method (an acquisition function) of selecting sample points to search for the best solution. We have shown that the working model performs as well as human operators in minimizing beam loss over a section of beamline.
Our AI-driven method has far-reaching implications for automated tuning of the entire ISAC-I/II and ARIEL beamline complexes for rare and stable isotope beam transport.
Intricate periodic and aperiodic ordered phases have been discovered in various soft matter systems such as supramolecular assemblies, surfactant solutions and block copolymers, underscoring the universality of emergent order in condensed matter. Theoretical study of block copolymer systems has been successful, revealing that the formation of complex ordered phases could be regulated by several mechanisms including conformational asymmetry, copolymer architecture and variety of the polymeric components. However, extending this success to non-polymeric soft matter systems is not straightforward and the study of the emergence of complex ordered phases in soft matter still presents an unsolved problem. We tackled this challenging problem by developing molecularly-informed Landau theory and density functional theory for various soft matter systems. In particular, we have demonstrated that the proposed theoretical framework can describe the emergence of complex ordered phases such as the networked phases and the Frank-Kasper phases. Our study provides an initial step for the development of a generic theoretical framework for the understanding of the universality of the phase behavior involving complex ordered phases in various soft matter.
Recent experimental and theoretical studies have shown that many ordered structures, ranging in complexity from simple lamellae to complex Frank-Kasper (FK) phases, can be formed from diblock copolymers. In many of the experimental studies the polymeric samples used in are polydisperse, however most theoretical studies have examined monodisperse systems. Therefore, to conduct theoretical studies on the phase behaviour of polydisperse block copolymer systems is desirable. In our study, the molecular weight distribution of AB diblock copolymers is modelled as a four component blend. Self-consistent field theory is used to study the effects of the shape of the molecular weight distribution (MWD). It is found that the width and skewness of the MWD, and conformational asymmetry, all have significant effects on the formation of the FK phases. The theoretical results provide insight to regulating block copolymer phase behaviours via designed molecular weight distributions and shed light on the formation mechanisms of the FK phases.
Many soft matter theoretical problems can be reformulated into minimizing a cost function, in which the field-based physical properties (the target functions) are adjusted to achieve the minimum. The Neural-network approach approximates the target functions by forward-feeding neural networks and the machine-learning techniques adjust the network parameters to produce the approximation to the desirable solutions. The physical properties, such as the free energy, together with boundary conditions, etc, are modelled in the cost function. The decoupling between the function approximator and sampling space allows for further incorporation of the weighted Monte Carlo method. The algorithm is demonstrated here by solving a few classical theoretical problems in soft matter.
AI and machine learning – specifically neural network (NN) based approaches – have become an indispensable tool in many areas of physics research. Nevertheless, there is still much to learn about NNs at the fundamental level and for application specific methodologies. In this talk, I will discuss some of the work we have done both using physics applications to study how neural networks learn and using neural networks to study physics applications. Both areas of research center on using NNs to solve partial differential equations (PDEs). On the one hand, simple physical systems described by PDEs yield clean and well-posed problems that are useful for analyzing the training process. On the other hand, using NNs to solve PDE descriptions of systems such as biomolecules in nanoconfinement is a promising alternative to standard simulation approaches. I will also discuss some current and potential approaches that combine machine learning and simulation techniques to achieve significant efficiency gains.
Nanothermometry is a powerful tool that allows for controlling temperature at the nanoscale, and thus finds applications in research fields ranging from biomedicine to high-power microelectronics. Typical nanothermometry techniques employ secondary nanothermometers, where each individual nanosensor must be individually calibrated—ideally, both off- and in-situ. Here we utilize fluorescent nanodiamonds co-hosting germanium-vacancy and silicon-vacancy centers and a machine learning multi-feature linear regression (ML-MFR) algorithm to overcome this resource-expensive calibration requirement. By leveraging the temperature-dependent spectroscopy features of the diamond color centers (intensity, zero-phonon line wavelength, emission linewidth, etc.), we show that the MFR model yields more accurate temperature predictions than those produced, traditionally, by monitoring any one of these individual temperature-dependent observables. We observe nanoscale temperature readings with accuracy and resolution improved by factors of ~1.3-10.1x and ~1.2-8.3x, respectively. Importantly, the MFR algorithm does so without the need to calibrate every single nanothermometer prior to its use. The method is general, as it is suitable for any nanothermometry technique that uses nanosensors with at least two temperature-dependent observables, without requiring prior knowledge of the type of dependence. Furthermore, this approach is attractive for practical scenarios where calibration prior to employment is difficult or unfeasible, as the models can be pre-trained on similar nanosensors. This study demonstrates the practical benefits of a machine learning approach to nanothermometry which is applicable to a wide variety of research fields.
The high-entropy oxide (HEO) Mg$_{0.2}$Co$_{0.2}$Ni$_{0.2}$Cu$_{0.2}$Zn$_{0.2}$O is synthesized by annealing equimolar mixtures of the parent binary oxides MgO, CoO, CuO, NiO, and ZnO to 1000 K and quenching to 295 K. X-ray diffraction shows HEO crystallizes in a single-phase rocksalt structure. The cations randomly occupy the $(000)$ site, while the oxygen sublattice is ordered. Lattice dynamical (LD) studies on amorphous Si ($\alpha$-Si) have shown that structural disorder can induce localized phonon modes (`locons') beyond a high-frequency mobility edge in the vibrational density-of-states (VDOS). Locons are characterized by eigenvectors which decay exponentially and a participation ratio $\mbox{(PR)}<0.1$. We have used the General Utility Lattice Program to study the optical properties and phonon localization in HEO. Previous LD studies on the elastic constants of ternary and quaternary oxides have obtained satisfactory agreement with experiment by neglecting cation-cation interactions and modelling cation-oxygen and oxygen-oxygen bonds with the Buckingham potential. Polarization effects are modelled using a shell model (SM) for oxygen; all cations are treated as point charges. In this work, we instead treat every atom with the SM: new Buckingham parameters for the binary oxides were obtained by fitting to experimental crystal structures, dielectric constants, and phonon frequencies. Agreement between the simulated VDOS and inelastic neutron scattering data is reasonable and improves upon existing models, which use a combination of the Buckingham potential and point charge approximation. Phonon mode localization was studied by calculating the PR of a 4096-atom supercell of HEO. Despite the strongly-disordered cation sublattice, it was determined that only of 0.5% modes are locons. This is roughly 10% of the number of locons in a similarly-sized cluster of $\alpha$-Si. Furthermore, it was shown that the number of locons increases if sulfur atoms are randomly substituted into the oxygen sublattice.
Understanding and controlling the liquid to crystal transformation is a central topic for numerous natural phenomena and technological applications. The first step of crystallization is the birth of critical nuclei. Their size, structure and rate at which critical nuclei appear and grow are fundamental parameters for understanding and controlling crystallization. Although nucleation rates can be measured experimentally in a few systems due to the very small nucleus size (nm) and either a too short or too long lifetime, it is extremely difficult to understand and describe the microscopic mechanism of nucleation, which remains elusive. To this end, computer simulation techniques provide, in principle, a suitable tool to dig deeper into this process. At least three main methods are available to obtain crystal nucleation rates via molecular dynamics simulation: 1) the mean lifetime method, 2) enhanced-sampling methods and 3) the seeding method.
The Classical Nucleation Theory (CNT) is one of the most well-known models to describe the nucleation process. This theory assumes that the formation of crystal nuclei takes place as a result of thermal fluctuations in a supercooled liquid (SCL). If an embryo overcomes a certain threshold size, it becomes a critical nucleus that spontaneously grows until it meets other growing crystals and the liquid solidifies. According to this theory, the interplay between the supercooled liquid/nucleus interfacial free energy, γ, and the difference between the chemical potentials of the crystal phase and the supercooled liquid describes the thermodynamics of crystal nucleation. The third key property is the effective diffusion coefficient, which controls the atomic transport rate at the liquid/crystal interface. The independent determination of these three quantities allows CNT calculations and comparison with experimentally determined or simulated nucleation rates. Owing to the scarcity of direct measurements of these properties, often questioned the validity and accuracy of the CNT. In this work, we were able to deeply supercool Zinc Selenide (ZnSe), and determine spontaneous homogeneous steady-state nucleation rates by molecular dynamics simulations (MD) using the mean lifetime method. At moderate supercoolings, where the nucleation rates are much smaller, we used the seeding method to compute the nucleation rates by the classical nucleation theory formalism, J_CNT, without any fitting parameter, using the physical properties obtained by MD simulations: the melting temperature, density, melting enthalpy, diffusion coefficient, and the critical nucleus size, combined with two expressions for the thermodynamic driving force. The values of γ calculated by the CNT expression using the MD simulation data, via both the seeding method and the mean lifetime method at moderate and deep supercoolings show a weak temperature dependence, which is in line with the Diffuse Interface Theory. The extrapolated values of γ, from the spontaneous nucleation regime to the seeding nucleation region cover the range of values of γ calculated via the seeding method and the CNT formalism. Finally, the J_CNT extrapolated from moderate supercoolings to deep supercoolings are in good agreement with the J_MD. These results confirm the validity of the CNT.
Understanding the kinetics and thermodynamics of the crystallization processes involved in carbon-rich materials is a critical knowledge gap that hinders a realistic assessment of the risks and benefits of potential climate-change-mitigation strategies [1]. Toward this end, we investigated the thermal and aqueous stabilities of single-phase and multi-phase mixtures of calcium carbonate and magnesian carbonate, including both laboratory-synthesized and biogenic sources. Building on earlier work from our group [2], we use a suite of materials characterization techniques (including infrared spectroscopy, differential scanning calorimetry, and thermogravimetric analyses) to track changes to the solid phases over time after thermal treatments and/or exposure to water-based solutions. Our results are framed in the context of how to design experiments that help to identify - and ultimately reduce - the uncertainties and associated risks associated with climate mitigation strategies that rely on controlling carbonate mineral formation.
[1] Basic Energy Sciences Roundtable: Foundational Science for Carbon Dioxide Removal Technologies (Brochure). United States: 2022. Web. doi:10.2172/1868525.
[2] B. Gao and K. M. Poduska. Solids 2022. 3(4) 684-696. doi: 10.3390/solids3040042.
The p-doping of organic semiconductors (OSCs) for tuning their electronic structure in opto-electronic applications is typically done by adding strong molecular acceptors as dopants to initiate charge transfer. I will summarize the current understanding of the phenomena observed upon molecularly p-doping conjugated polymers (CPs) and molecules (COMs), where two different competing scenarios have been identified [1]: (i) integer charge transfer between OSC dopant forming ion pairs (IPAs) and (ii), fractional charge transfer, where ground-state charge transfer complexes (CPXs) between the OSC and dopant are formed. For prototypical OSCs such as poly(3-hexylthiophene) (P3HT) [2] and various oligothiophenes of different chain length [3], I will present recent findings on the role of microstructure, dopant strength, and conjugation length on the respective doping scenarios, from which chemical design strategies for improved molecular dopants emerged and are tested to suppress CPX formation [4].
[1] Salzmann et al., Acc. Chem. Res. 49, 370 (2016); [2] Hase et al., J. Phys. Chem. C 122, 25893 (2018), Hase et al., J. Phys. Mater. 6, 014004 (2023); [3] Liu et al., Angew. Chem. Int. Ed. 59, 7146 (2020); [4] Charoughchi et al., submitted.
We discuss a systematic error in time-resolved optical conductivity measurements that becomes important at high pump intensities. We show that common optical nonlinearities can distort the photoconductivity depth profile, and by extension distort the photoconductivity spectrum. We show evidence that this distortion is present in existing measurements on $\text{K}_{3}\text{C}_{60}$, and describe how it may create the appearance of photoinduced superconductivity where none exists. Similar errors may emerge in other pump-probe spectroscopy measurements, and we discuss how to correct for them.
What is a quantum black hole? How does it form and how long does it last? I will provide an answer to these questions via an effective equation that describes gravitational collapse of dust with quantum corrections. Solving this equation reveals that black holes end in a shock wave after a time of order mass squared.
I will discuss a class of time-dependent, asymptotically flat and spherically symmetric metrics which model gravitational collapse in quantum gravity developed by myself and the other listed authors. Motivating the work was the intuition that quantum gravity should not exhibit curvature singularities and indeed, the metrics lead to singularity resolution with horizon formation and evaporation following a matter bounce. A noteworthy result of this metric is that we can recover the Hawking evaporation time M^3 for the lifetime of the black hole.
In general, black holes interact with external matter and fields. A four-dimensional static black hole within a static external axisymmetric gravitational field can be described by a Weyl solution of the Einstein equations. These results can be extended to higher dimensions using the generalized Weyl form. Various studies have been devoted to investigate the properties of the distorted black holes so far. These include a distorted five dimensional Schwarzschild-Tangherlini black hole, a distorted five dimensional Reissner-Nordstrom black hole and a distorted black ring. In this talk, we consider five-dimensional Weyl solutions, which are characterized by two independent axially symmetric harmonic functions in three-dimensional flat space. Using this method, we investigate distortions of a vacuum five-dimensional black hole with a “bubble' (the black hole exterior has nontrivial topology).
In recent years, with the progress in gravitational wave astronomy and subsequent importance of binary black hole mergers, there has been an increased focus on numerical simulations of these events. However, the most common surface of interest in black holes—the event horizon—is difficult to track numerically, as it is defined teleologically from future boundary conditions. Instead, the focus is on the quasi-local alternative to the event horizon, marginally outer trapped surfaces (MOTSs)—the apparent horizon being the outermost of these (in most cases). Our group has previously discussed the self-intersecting MOTSs we have found inside the apparent horizons of various black hole spacetimes. However (and unsurprisingly given how rotation often complicates analysis), the formalism used to calculate these MOTS for static black hole geometries does not hold when considering rotating black holes. This talk will focus on a formalism we have developed which generalizes the previous methods to rotating black holes (of arbitrary dimension) and provide an example of using this formalism to calculate the “MOTSodesic” equations—an analogue of the geodesic equations for MOTSs—in the Kerr spacetime. Applications of this method will be discussed in the talk by Kam To Billy Chan.
Self-intersecting marginally outer-trapped surfaces (MOTSs) have been found to play a vital role in binary black hole merger processes through numerical simulations [Pook-Kolb et. al. arXiv:1903.05626]. The search for such exotic MOTSs can also be found in analytical black hole solutions, such as the simplest (Schwarzschild) black hole [Booth et. al., arXiv:2005.05350]. Ongoing work continues to investigate the physical implications of the self-intersecting behaviour in spherically-symmetric spacetimes [Hennigar et. al., arXiv:2111.09373]. The previous techniques for finding self-intersecting MOTSs are restricted to non-rotating spacetimes. This talk makes use of the extension of the MOTS-finding method to rotating (axisymmetric) spacetimes for any dimension that was developed in [Booth et. al., arXiv:2210.15685] and which is presented at this congress in the talk by Sarah Muth. Such spacetimes are astrophysically relevant, as black holes found in our universe are expected to carry angular momentum. It is shown that the MOTSs found bears many similarities with those found in spherically-symmetric spacetimes, while exhibiting previously unseen behaviours.
For the last few decades and especially since the first detection of gravitational waves, black hole mergers have been a core research area in general relativity. However, the process by which two black hole horizons merge is only now starting to be well-understood. In numerical studies of apparent horizon evolution, self-intersecting marginally outer-trapped surfaces (MOTS) were found and play a key role [Pook-Kolb et. al. arXiv:1903.05626]. Later an infinite number of self-intersecting MOTSs were found in Painleve-Gullstrand slices of the Schwarzschild solution [Booth et. al., arXiv:2005.05350]. Further work has shown that their existence is robust and not simply an artifact of that coordinate system [Hennigar et. al., arXiv:2111.09373]. This talk presents results found when examining the maximal extension to the Schwarzschild black hole in Kruskal-Szekeres coordinates. In this system, two separate universes dynamically connect through a worm-hole and pass through a moment of time-symmetry before the worm-hole pinches off and they disconnect. In these time slices, self-intersecting MOTS are found which, among other things, straddle the Einstein-Rosen bridge extending into both universes. Of particular interest is the behavior around the moment of time symmetry, as this provides insight into how MOTS evolve in numerical solutions which start from time-symmetric initial data.
The notion of wave-particle duality is fundamental in the quantum mechanical description of matter. This duality asserts that matter sometimes behaves like a particle and sometimes behaves like a wave, called de Broglie waves. Recent advances in methods to coherently manipulate de Broglie waves of atoms have enabled a new generation of atom interferometers with unique capability to address outstanding fundamental science challenges. The method has emerged as a tool capable of addressing a diverse set of questions in gravitational physics and quantum physics, and as a technology for advanced sensors for navigation and for measurement of the Earth’s gravitational field. We will discuss an experiment consisting of a tungsten mass and atomic wave packets separated by about 25cm. In this experiment, the relative phase of the interfering wave packets is shown to depend on the gravitational interaction in a way which is analogous to the so-called Aharonov-Bohm effect for charged particles. We will describe the relevance of these results to observation of quantum superpositions of Newtonian gravitational fields. Future science and technology applications will also be described, including the detection of dark matter, detection of gravitational waves at frequencies below 1 Hz and satellite geodesy.
Session I: Biopolymers in Confined Environments
I will present a unique quantitative single-molecule imaging platform called CLiC (Convex Lens-induced Confinement) which enables simultaneous measurements of the size, mRNA-payload, and dynamic properties of mRNA-based therapies and vaccines in controlled, cell-like conditions (Kamanzi et al, ACS Nano 2021). Here, we apply single-molecule biophysics to help characterize and understand the mechanisms of action of emerging classes of therapeutics and vaccines. By isolating and imaging freely diffusing particles in solution as well as during reagent-exchange, such as in response to a change in solution pH, we can emulate and explore dynamics in a controlled setting which are relevant to understanding complex dynamics inside cells and as well as inside manufacturing devices. Over the long term and in collaboration with health scientists, we are working towards correlating detailed multi-scale data sets, including single-particle measurements made in vitro as well as in cells and tissues, with genomic and proteomic analyses of the same samples, as well as clinical results, to create a through-line of understanding of drug/vaccine effectiveness from the microscopic to clinical scale. Our inspiration is to innovate and use nanoscale tools to obtain new biophysical insights into how and why medicines/vaccines work to enable and optimize their rational design and engineering. This talk builds off our recent publication in ACS Nano (Kamanzi et al, 2021) which established our measurement platform, and describes our ongoing collaboration with health scientists and unpublished data sets on single-particle dynamics and mRNA-LNP properties acquired at our new labs in MSL-UBC during the pandemic.
Even though dilute (unentangled) polymer solutions cannot act as gel-like sieving media, it has been shown that they can be used to separate DNA molecules in capillary electrophoresis. The separation then comes from sporadic and independent polyelectrolyte-polymer collisions. Here we explore such collisions in nanochannels (i.e., channels that are smaller than the normal size of the polymers), a situation where a charged analyte is forced to migrate "through" isolated uncharged molecules during electrophoresis. We use Langevin dynamics (LD) simulations to investigate the nature of these collisions and their effect on the net movement of both polymer chains. We identify several types of collisions, including some that are unique to nanochannels. These results suggest a few potential applications for the analysis of biomolecules.
In recent years, nanofluidic devices have proven extremely useful for characterizing the physical behaviour of biopolymers such as DNA confined to narrow channels and micron-sized cavities. Insight gleaned from experiments using nanochannels is valuable for applications such as optical mapping of elongated DNA. Likewise, studies of multiple DNA molecules in nanocavities have provided insight into the confinement-enhanced entropic force that tends to induce polymer segregation, an effect that likely contributes to segregation of chromosomes in replicating prokaryotes. While simple theoretical models can be used to explain the basic aspects of such behaviour, the experiments are often carried out under conditions where the system lies outside clearly defined scaling regimes. This can give rise to pronounced quantitative discrepancies between theory and experiment. In such cases, computer simulations can provide an effective means to bridge the divide between the theoretical predictions and experimental results. In this talk, I present the results of recent Monte Carlo simulation studies, most of which have been inspired by recent experiments on confined DNA. I examine the effects of channel shape and width on the tendency for single semiflexible chains to form structures such as backfolds and knots. I also examine polymer segregation behaviour of two-chain systems confined to channels or elongated cavities. A key aspect of this work is the explicit calculation of the variation of the configurational free energy with respect to some relevant system parameter such as knot size or inter-polymer overlap. Theoretical treatments typically employ analytical approximations of free energy functions. While the explicitly calculated free energy functions yield qualitatively similar scaling behaviour, the discrepancies between calculated and theoretical scaling exponents can be appreciable. Quantifying these discrepancies should be of value in the interpretation of experimental results.
Innovation in materials science and engineering resides in our ability to control the structure of materials at the nanoscale in order to design advanced materials with outstanding functional properties (electrical, optical, magnetic, photocatalytic, etc.). One of the most powerful means to arrange matter at the nanoscale is to use laser produced plasmas due to their exceptional ability to provide simultaneously ions and neutral atoms with various energies in a non-equilibrium environment. Moreover, the possibility to perform growth in a reactive environment such as oxygen or to operate in a double-beam configuration offers an additional flexibility to control the stoichiometry of oxide materials, the dopant content and the surface quality. In this presentation, we will focus on the use of pulsed laser deposition for the growth of various oxide materials in the form of thin films, including undoped and doped vanadium dioxide and titanium oxide. They are exploited for the development of the next generation of photonic devices or for advanced environmental applications such as water treatment.
The field of nanotechnology has rapidly expanded over the past few decades due to the unique physical, chemical, mechanical, and electrical properties of nanoscale materials. Today, nanomaterials are applied in numerous fields, including catalysis, drug delivery, and microelectronics, among others. Plasma-based methods have shown great potential for use in the synthesis of nanomaterials via bottom-up or top-down approaches. The plasma-liquid system is a relatively novel field of research that has shown high efficiency in synthesizing nanomaterials. In this system, the plasma is either i) generated in a gas phase that is in contact with the liquid or ii) generated directly in the liquid (with or without bubble assistance).
In this communication, we will focus on the production of nanomaterials using in-liquid discharges, more particularly those eroding the electrodes in a controlled way. First, we will show that the produced particles are highly sensitive to both, electrode nature and liquid composition. In a second part, we will introduce a novel plasma-liquid system in which a spark discharge is used to generate plasma in a liquid that is in contact with another liquid (combination of type (i) and type (ii) systems). A brief review of the discharge electrical and optical characteristics, we will provide the synthesis conditions, i.e. those leading to a spark discharge between a pin electrode immersed in a dielectric liquid (heptane) and the surface of a conductive solution (water + metal salts). This configuration guarantees an interaction between the high-density plasma (spark in liquid heptane) and the solution that contains metal ions, and so, we used it herein to synthesize metal nanoparticles as well as binary and ternary nanoalloys.
Since its inception in 1999, Plasmionique has been carrying out collaborative research with Canadian Universities, national laboratories as well as international groups and companies. Such collaborations have allowed Plasmionique to remain at forefront of technological development and fulfill its mission of proliferating and commercializing plasma technology as an environmentally clean substitute for many challenging problems related to Advanced Surface Engineering, Material Synthesis, and Thin Film Processing. In this talk, we will present some examples to highlight the diversity of the applications that plasma technology could offer. Examples of topics discussed include, the synthesis of various allotropes of carbon, such as CNT [1], graphene [2], diamond [3] ; surface engineering of forestry products [4] ; thin film synthesis of multiferroic materials using conventional and hybrid [5] PVD techniques for memory [6] and neuromorphic engineering applications[7] ; biomaterial surface engineering for deposition of antibacterial coatings [8] ; DLC hard coating on implants for protection against corrosion and erosion [9] ; implantation of short-life ß-emitting radioisotopes in medical implants [10] and controlling the corrosion rate of biodegradable materials.
1- J.B. Kpetsu, et al., Nanoscale Res Lett (2010) 5:539–544
2- P. Vachon, et al., J. Phys. D: Appl. Phys. 54 (2021) 295202 (13pp)
3- A. Sarkissian, et al., CAP/COMP/CASCA 2004 Congress, June 13, 2004, Winnipeg
4- S. Babaei, et al.,et al, Plasma Process Polym. 2020;17:e2000091
5- D. Benetti, et al., Scientific RepoRts | 7: 2503 | DOI:10.1038/s41598-017-02284-0
6- F. Ambriz-Vargas, et al., Appl. Phys. Lett. 110, 093106 (2017)
7- G. Kolhatkar, et al., ACS Appl. Electron. Mater. 2019, 1, 828−835
8- L. Bonilla-Gameros, et al., Nanomedicine : Nanotechnology,Biology and Medicine, 24(2020)102142
9- G. Morand, et al., Surf Interface Anal. 2021;53:658–671.
10- F. Marion, et al., Plasma Sources Sci. Technol. 18 (2009) 015014
Nanocomposite (NC) thin-films are widely studied due to the multifunctional properties they can develop (optical, electrical, mechanical). A lot of methods are under development with a real attraction for processes at atmospheric pressure, such as dielectric barrier discharge (DBD).
Recently, a new process of nanoparticles injection in plasmas has been developed [1]. This method consists in synthesizing the nanoparticles prior to their injection in the plasma in a low frequency pulsed injection regime. However, the impacts of the liquid pulsed injection on the DBD physics are still opening questions.
This work aims to study a pulsed-liquid-assisted DBD deposition process. In contrast with the continuous nebulization of solutions, pulsed injection causes a sudden increase of the quantity of precursor as droplets in the inter-dielectric space – the average velocity being in the 10 m/s range. We observed that depending on the process parameters (injection times, pulse frequency, continuous gas flow rate, etc.), the discharge stability is modified. These parameters are also critical for transport and evaporation of the droplets and so on the thin film deposition (here ppHMDSO). For example, by varying the different parameters of the pulsed-liquid-assisted DBD, we observe that the deposit can consist in different phases (liquid and solid) as a function of the time residency of the aerosol and the thickness of the deposited layer.
[1] Kahn, M., Champouret, Y., Clergereaux, R., Vahlas, C. & Mingotaud, A.-F. Process for the preparation of nanoparticles. (2016).
Nitrogen doped graphene, or N-graphene, is a promising material for a wide range of applications such as supercapacitors, optoelectronic devices, and biosensors. Nitrogen plasmas have been proved to be an excellent path to generate N-graphene from polycrystalline monolayer graphene films grown by chemical vapor deposition (CVD). In this study, CVD graphene has been exposed to low-frequency Townsend dielectric barrier discharge operated in nitrogen at atmospheric pressure. In such conditions, the discharge is weakly ionized, and the neutral gas temperature is close to 300 K. In addition, plasma-graphene interactions are dominated by plasma-generated N atoms and metastable N2(A) states, with the latter acting as a 6 eV energy reservoir. To investigate the mechanisms of nitrogen incorporation by the plasma-based process, Hyperspectral Raman IMAging (RIMA) and X-ray Photoelectron Spectroscopy (XPS) have been performed over different processing time. A clear defects generation is observed from the Raman signature with a transition towards amorphization for longer discharge exposure times. From the high spatial resolution of RIMA, different Raman dynamics can be seen at the grain domains (GD) versus at the boundaries (GB) of CVD graphene. It is found that there is a selective nitrogen incorporation at GDs, a feature linked to preferential healing of plasma-generated defects near GB. N-uptake is further discussed using the model proposed by Robert-Bigras et al. in which defects generation plays a critical role in the N-incorporation kinetics.
Uncovering the nature of dark matter is one of the most important goals of particle physics. Light bosonic particles, such as the dark photon, are well-motivated candidates: they are generally long lived, weakly-interacting, and naturally produced in the early universe. LAMPOST (Light A' Multilayer Periodic Optical SNSPD Target) experiment searches for dark photon dark matter in the eV mass range, via coherent conversion of dark photon to photon in a multilayer dielectric haloscope, which are subsequently collected with superconducting nanowire single-photon detector (SNSPD).
I this talk, I will report on the recent progress of the LAMPOST experiment. In a prototype experiment, we achieve efficient photon detection with a dark count rate (DCR) of ∼ $6 \times 10^{−6}$ counts/s. We find no evidence for dark photon dark matter in the mass range of ∼ 0.7-0.8 eV with kinetic mixing $\epsilon \geq 10^{−12}$, improving existing limits in the mass range. I will also show some recent progress in experimental design and performances of SNSPDs, and how these could allow us to probe significant new parameter space for dark photon and axion dark matter in the meV to 10 eV mass range.
SENSEI (Sub-Electron Noise Skipper Experimental Instrument) is a direct detection dark matter experiment with detectors operating at Fermilab and at the SNOLAB underground facility. The experiment consists of silicon Skipper-CCD sensors that make multiple non-destructive measurements of the charge contained in each pixel, reducing the readout noise to a level that allows for resolution of single electrons. This low energy threshold, along with low rates of events which may contain up to four electrons, results in competitive sensitivity for low-mass dark matter candidates which interact with electrons over a wide range of dark matter masses. This presentation will give an overview of the SENSEI experiment and the current status after the successful commissioning of the first batch of science-grade sensors at SNOLAB.
In the presence of radiation from bright astrophysical sources at radio frequencies, axion dark matter can undergo stimulated decay to two nearly back-to-back photons, meaning that bright sources could have counterimages in other parts of the sky. The counterimages will be spectrally distinct from backgrounds, taking the form of a narrow radio line centered at half the axion mass with a spectral width determined by Doppler broadening in the dark matter halo. The morphology of these images can be nontrivial, with blurring due to the geometry of the source and image as well as spatial smearing due to the galactic kinematics of axion dark matter. I will show that the axion decay-induced counterimages of galactic sources may be bright enough to be detectable with ongoing observations from the FAST radio telescope as well as archival data from CHIME and other radio surveys.
The Super Cryogenic Dark Matter Search (SuperCDMS) is a direct detection experiment, optimized for low-mass dark matter searches. Comprised of silicon and germanium crystal bolometers, the experiment utilizes transition-edge sensor (TES) technology to measure small heat signals that result from particle interactions with the bulk crystal. While the experiment is small compared to ton-scale experiments, the low energy threshold of these detectors enables searches for low-mass dark matter. More recently, a gram-scale SuperCDMS prototype detector was developed (HVeV), achieving eV-scale resolutions, and resolving single electron-hole events thanks to the high voltage (HV) applied across the detectors, which amplifies ionizing events. Traditional direct detection searches have relied on dark matter nuclear recoils as their signal. Electron-recoil dark matter (ERDM) is another avenue for dark matter to possibly interact with the Standard Model, and has gained interest recently in searches for light dark matter (LDM) candidates. In this talk, I will present recent updates from Run 4 of the HVeV program at NEXUS (Northwestern EXperimental Underground Site) in Fermilab, probing ERDM candidates such as dark photons, axion-like particles, as well as generic LDM electron-scattering signals.
The inclusion of thermodynamic pressure has been one of the major developments in black hole thermodynamics in recent years. By incorporating pressure, black holes are now known to exhibit behaviour corresponding to that seen in a broad variety of chemical systems, including liquid-gas type transitions, reentrant phase behaviour, polymer-like transitions, superfluid phase behaviour, and more. Consequently the subject has come to be known as Black Hole Chemistry. While black hole triple points — analogous to the ice-water-steam triple point — were discovered several years ago, only recently has it been shown that black holes can have multicritical points, in which four or more phases coalesce at a single temperature and pressure. This phenomenon — seen in colloids and polymers — can take place in Einstein gravity for multiply rotating black holes, as well as in charged black holes in non-linear electrodynamics, Lovelock gravity, and Generalized Quasitopological Gravity. I will describe how multicriticality arises in black holes and how the Gibbs Phase Rule governs such behaviour.
Relativistic quantum metrology is a framework that not only accounts for both relativistic and quantum effects when performing measurements and estimations, but further improves upon classical estimation protocols by exploiting quantum relativistic properties of a given system.
Here I present recent developments in the Fisher information analysis associated with black hole spacetimes. I review recent work in relativistic quantum metrology that examined Fisher information for estimating thermal parameters in (2+1)-dimensional AdS and the static BTZ black hole spacetimes. Treating Unruh-DeWitt detectors coupled to a massless scalar field as probes in an open quantum systems framework, I extend these recent results to the (2+1)-dimensional rotating black hole spacetime. We find that varying the angular momentum of the BTZ black hole leads to dramatic change in the Fisher information provided the appropriate black hole and detector parameters.
During simulations of a binary black hole collision, the final (post-merger) black hole horizon exhibits a decaying oscillation. There is also an observable gravitational wave signal from this black hole ringdown. Then it is natural to think that the oscillation generates the gravitational wave signal. However, this is not the case. By definition the black hole horizon (either event or apparent) cannot send signals to infinity. Instead, both the ringdown and signal must correlate with evolving, near-horizon gravitational fields which send signals both out to infinity as well as into the black hole. What then can an evolving horizon geometry tell us about the surrounding spacetime? Quantifying an answer to this question requires not only the Einstein equations but also a careful consideration of “physically reasonable” initial and boundary conditions. In this talk I will discuss recent progress that we have made on this problem.
We derive a "classical-quantum" approximation scheme for a broad class of bipartite quantum systems. In this approximation, one subsystem's evolution is governed by classical equations of motion with quantum corrections, and the other subsystem evolves quantum mechanically with equations of motion informed by the classical degrees of freedom. Similar approximations are common when discussing the backreaction of quantum fields on curved spacetime, as in Hawking radiation around black holes or the generation of primordial perturbations in inflation. We derive an estimate for the growth rate of entanglement between the subsystems, which allows us to predict the "scrambling time": the amount of time required for the subsystems to become significantly entangled. We illustrate the general formalism by numerically studying the fully quantum, fully classical, and classical-quantum dynamics of system of two oscillators with non-linear coupling.
Marginally outer trapped tubes are one of the essential tools to understand the dynamical evolution of Black Holes. In this talk, I will present a new symplectic formalism that applies to various spacetimes containing a BH. This framework allows studying charges, flux laws, and higher multiple moments. All this is directly linked to the study of gravitational waves.
This talk reviews selected topics of the Fundamental Symmetries sector of Nuclear Physics from the theoretical point of view. It focuses on three themes of interest to the Canadian experimental community: electric dipole moments, neutral currents, and beta decays. Lepton flavor violation, where major new international experiments are about to come online, will also be discussed.
Experimental tests of fundamental symmetries using nuclei and other particles subject to the strong nuclear force have led to the discovery of parity (P) violation and the discovery of charge-parity (CP) violation. It is believed that additional sources of CP-violation may be needed to explain the apparent scarcity of antimatter in the observable universe. A particularly sensitive and unambiguous signature of both time-reversal- (T) and CP-violation would be the existence of an electric dipole moment (EDM). The next generation of EDM searches in a variety of complimentary systems (neutrons, atoms, and molecules) will have unprecedented sensitivity to physics beyond the Standard Model. This talk will focus on current and planned experiments that use radioactive isotopes with pear-shaped nuclei. This uncommon nuclear structure significantly amplifies the observable effect of T, P, & CP-violation originating within the nuclear medium when compared to isotopes with relatively undeformed nuclei such as Mercury-199. Certain isotopes of Radium (Ra) and Protactinium (Pa) are both expected to have greatly enhanced sensitivity to symmetry violations and will be produced in abundance at the Facility for Rare Isotope Beams currently operating at Michigan State University. I will describe the current status of ongoing searches and the prospects for next generation searches for time-reversal violation possibly using radioactive molecules to further enhance the new physics sensitivity in the FRIB-era.
The MOLLER experiment at Jefferson Lab aims for an ultra-precise determination of the weak mixing angle $\sin^2\theta_W$ by measuring the parity-violating asymmetry $A_{\rm PV}$ in polarized electron-electron (Moller) scattering. For the approved 88 calendar week run, the proposed accuracy on $A_{\rm PV}$ is 0.7 parts per billion corresponding to an overall relative measurement accuracy of 2.4% for the electron's weak charge and 0.1% for the weak mixing angle. The measurement will enhance our understanding of fundamental symmetries of the electroweak interaction and provide a powerful search for physics Beyond the Standard Model. MOLLER represents a 4th generation parity violation experiment at Jefferson Lab and has an experienced collaboration working closely with integrated lab management team. The project is fully funded and on schedule for assembly in Hall A starting in early 2025. This talk will give an introduction to MOLLER physics motivations and reach, present details of the apparatus and experimental techniques, and conclude with a brief progress update on status and plans.
The MOLLER (Measurement Of a Lepton Lepton Electroweak Reaction) experiment, in preparation at Jefferson Lab, aims to constrain physics beyond the Standard Model using parity-violating Moller scattering at 11 GeV. The parity-violating asymmetry between the cross-sections for right- and left-handed helicity beam electrons scattered from the atomic electrons in a liquid hydrogen target is expected to be 35.6 ppb and MOLLER aims for 0.73 ppb precision. The measured asymmetry will be used to determine the weak charge of the electron to a fractional accuracy of 2.4%. Among the most challenging aspects of the experiment will be the detection of the small asymmetry in the detector signal. To prepare for production running, we must fully characterize the MOLLER main detector system through a combination of simulation and beam tests. This talk will provide an overview of the main detector system with a focus on radiation testing of our integrating electronics.
Topological semimetals display a range of novel transport phenomena, including enormous magnetoresistance and mobilities. Using Raman spectroscopy we have uncovered a novel mechanism for phonons to play a central role in this phenomena. Specifically we demonstrate the phonon-electron scattering time far exceeds the phonon-phonon. As such the momentum and energy typically lost to the lattice is returned to the electron bath. I will also briefly discuss the key material properties that make this discovery possible.
Spectroscopic techniques have made remarkable progress in the past decades have played a critical role in advancing our understanding of quantum and topological materials. However, the interpretation of the spectroscopic data and information extraction processes can be highly nontrivial. In this symposium talk, we introduce machine learning as an auxiliary technique for various experiments that can lead to our improved understanding of quantum phenomena. We show that it can enhance the identification of nuanced magnetic effects at topological insulator interfaces [1], and directly be used to predict materials’ topological classes using simple spectra indicators [2]. Beyond resolution improvement or classification, we show that machine learning can also be used to predict materials properties that are challenging to obtain by conventional methods, such as phonon density-of-states [3] and phonon dispersion relations [4], or extracting hidden information in time-resolved data [5]. We highlight the importance of the representations and envision a few more challenging problems that can benefit from machine learning [6], from strongly correlated systems to finding topological materials that are ready for room-temperature devices.
[1] https://aip.scitation.org/doi/10.1063/5.0078814
[2] https://onlinelibrary.wiley.com/doi/abs/10.1002/adma.202204113
[3] https://onlinelibrary.wiley.com/doi/10.1002/advs.202004214
[4] https://arxiv.org/abs/2301.02197
[5] https://onlinelibrary.wiley.com/doi/10.1002/adma.202206997
[6] https://aip.scitation.org/doi/10.1063/5.0049111
Topological semimetals can host novel fermionic particles whose intriguing interactions and many-body phases can be studied experimentally. I will discuss the particularly exciting class of Rarita-Schwinger-Weyl semimetals hosting spin-3/2 electrons with linear dispersion at a four-fold band crossing point, realized experimentally in quantum materials in the last years. I will combine symmetry considerations, perturbative renormalization group analysis, and mean-field theory to discern several exotic interacting phases that are prone to emerge in the strongly correlated regime.
One intriguing feature of 2D hyperbolic-lattice models is that their band theories live in hypertoric Brillouin zones. The high-dimensional band structures and the dimensional mismatch between real and momentum spaces present uncharted territory beyond Euclidean topological phases. This work investigates topological phases exhibited by hyperbolic Haldane models, which are generalizations of the graphene Haldane model to various regular hyperbolic lattices. A comprehensive symmetry analysis is performed to constrain the multiple independent first and second Chern numbers arising from the high-dimensional bands. Our extensive analysis of both real- and momentum-space models shows frequent occurrence of topological gaps, most of which characterized by first Chern numbers of 1 and some of 2. Importantly, the numerically computed first Chern numbers respect the predicted symmetry constraints and agree with real-space topological markers, implying a direct connection to observables such as the number of chiral edge modes. With our large repertoire of models, we further demonstrate that the topology of hyperbolic Haldane models is trivialized by strong curvature of the underlying lattices.
Opening remarks
Dr. Phil Kaye graduated in the first PhD cohort from Waterloo’s Institute for Quantum Computing in 2007. From 2004 to 2018, he served in a variety of roles with the Government of Canada’s Communications Security Establishment, primarily as a trusted advisor on the impacts of quantum technologies. From 2004 to 2010, he was the Program Reporter for the Canadian Institute for Advanced Research’s Quantum Information Processing Program. In 2007, Phil co-authored a seminal textbook on quantum algorithms (“An Introduction to Quantum Computing”, Kaye, Laflamme, Mosca, 2007). From 2018 to 2020, he worked for D-Wave Systems as Program Director, Corporate Affairs. In 2019 he co-founded and chaired Quantum Industry Canada (QIC), a consortium representing over 24 Canadian quantum technology companies. Presently, Phil is leading NRC’s Applied Quantum Computing Challenge program. In his spare time, Phil pilots an airplane that he built in his garage, plays the guitar and composes music.
Dr. Rezaee earned his PhD in Physics from the University of Tennessee, Knoxville, in 2015, and subsequently held postdoc positions at Texas A&M University and the University of Ottawa. While at the University of Ottawa, Dr. Rezaee played a crucial role in establishing the Joint Centre for Extreme Photonics (JCEP) lab, a collaborative initiative with the NRC. His academic pursuits revolve around ground-breaking quantum light sources, diamond-based quantum sensing, and quantum simulation. Beyond academia, Dr. Rezaee has founded three quantum hardware startups in both Canada and the USA. While doing so, he also successfully completed the Creative Destruction Lab-QML programs at the Rotman School of Business and participated in Y Combinator's W19 cohort. Driven by an unwavering passion for quantum technologies, Dr. Rezaee continues to help bridge the gap between cutting-edge science and transformative commercial ventures in his current role as Mitacs' national team lead for quantum technologies.
Dr. Nipun Vats is the Assistant Deputy Minister, Science and Research Sector, at the Department of Innovation, Science and Economic Development Canada. In this role, he is responsible for leading the development of federal policy and investments in post-secondary research.
He has held a variety of positions within the Canadian federal government, including in the Privy Council Office and the Department of Finance, and as Secretary to a National Advisory Panel on Sustainable Energy Science and Technology. He has also served as the lead federal official in the successful negotiation of the Canadian Free Trade Agreement.
In this talk, we will discuss a model of quantum gravity in which dynamical spacetime arises as a collective phenomenon of underlying quantum matter. In the model, the pattern of entanglement formed across local Hilbert spaces determines the dimension, topology and geometry of an emergent spacetime. After discussing the general structure of the model, we will describe the dynamics of a semi-classical solution that describes a (3+1)-dimensional de Sitter-like spacetime with the Lorentzian signature. Small fluctuations around the semi-classical solution include the propagating gapless graviton.
Session II: Superbiomolecular Assemblies
Nucleic acids are the most basic molecules of life, being tasked with storing and transmitting genetic information in all living organisms. Both DNA and RNA are composed of fundamental building blocks that each include a nucleobase (A, G, C, T/U), sugar ([deoxy]ribose), and phosphate moiety. To enhance nucleic acid programmability and stability, and aid the formation of functional 3D shapes, nucleotides are commonly modified in nature. Indeed, DNA nucleobases are methylated to control gene expression, while the identification of over 130 distinct modifications in RNA has led to the emerging field of epitranscriptomics. Furthermore, the ease of synthesis of nucleic acids functionalized at any nucleobase, sugar, or phosphate site, as well as the ability of modifications to impact pairing, chemical stability, conformation, and interactions with proteins, has led to the development of a wealth of unique modifications with far-reaching applications. For example, modified nucleic acids have been designed for medicinal uses such as drugs, vaccines, bioprobes, antimicrobials and tissue engineering, as well as for nanomaterials to build nanowires, nanomachines and nanorobots. Unfortunately, the lack of known structure–function relationships for a range of modified nucleic acids raises questions such as why does nature introduce modifications and how can modifications be used to their full potential in valued applications. This talk will provide a survey of some of the recent topics of interest in my lab that use computer modeling to gain a fundamental understanding of the diverse chemistry of modified nucleic acids. The information gained from computer simulations fills knowledge gaps by providing a greater understanding of the role of nucleic acid modifications in nature and improving the design of original modified nucleotides for novel applications.
Hypoxia is a characteristic pathophysiological property of advanced solid tumours which influences aggressiveness and resistance to treatment. Real-time measurement of tumour oxygenation is thus vital for stratifying treatment plans by hypoxic severity and monitoring variations in partial pressure of oxygen (pO$_2$) caused by high energy X-ray and other photonic therapies. Azobenzene photoswitches present a novel form of oxygen sensing predicated on their photophysical properties. Upon irradiation with light, azobenzenes undergo reversible geometric isomerization between stable trans and metastable cis isomers. The rate of cis-trans thermal relaxation is a first-order process sensitive to the molecular environment, which translates into sensor functionalities. In this work, we investigate a novel bio-inspired azobenzene photoswitch for oxygen sensitivity in solution.
A biomimetic material, FePc(PAP)$_2$ was synthesized by coordination of 4-phenylazopyridine (PAP) to iron (II) phthalocyanine (FePc). As a model system for oxygen sensing, FePc is capable of binding oxygen similarly to heme-porphyrin in blood. Solutions were purged with argon gas or flowed with oxygen gas to modulate pO$_2$. Isomerization kinetics were measured by pump-probe isomerization spectroscopy, wherein photoisomerization was initiated by irradiation with a 600 mW 365 nm LED, and then recovery of the $\pi$-$\pi^*$ absorption band was monitored as a function of time with a spectrophotometer. In addition, density functional theory (DFT) was used to theoretically calculate the activation barrier between cis and trans isomers, which can be related to isomerization rates in the presence or absence of oxygen.
To validate our experimental setup, cis-trans isomerization rates of methyl orange and methyl red photoswitches were measured to be insensitive to oxygen, as expected from literature. As a control, the isomerization lifetime of PAP was found to be several hours in ambient oxygenation. DFT calculations predict that the isomerization rate of a PAP-porphyrin system is an order of magnitude faster than PAP. As a proof-of-principle demonstration of a new molecular sensor for evaluating tumour oxygenation, the isomerization rates of PAP and FePc(PAP)$_2$ were experimentally and computationally determined as a function of oxygen concentration and will be reported in this work.
Understanding and controlling structural organization mechanisms is a key challenge in producing synthetic materials that mimic the complexity seen in organisms. This talk will present recent advances in controlling the local organization of colloidal building blocks, and a "pre-assembly" approach to produce hierarchically-structured materials.
A low-temperature plasma (LTP) is being advanced as an alternative radiation source that offers unique chemical properties owned by a variety of reactive plasma species (RPS), such as radicals, electrons, and excited species, delivered and formed in media upon exposure. Our current research explores the possibility of implementing DNA and its damage as a probe for specific plasma diagnostics such as RPS formation and transient local heating. Both LTP characteristics have been analyzed based upon the detection of plasma-induced strand breaks and DNA denaturation. Our previous studies proved that DNA can be utilized as a probe for RPS, particularly for reactive oxygen and nitrogen species that cause strand breaks in aqueous DNA. Moreover, the yield of strand breaks can be varied by tuning plasma parameters because of DNA’s susceptibility to all RPS. Recently we observed previously undetected DNA denaturation in addition to the DNA strand breaks present upon plasma irradiation. Thus, our primary focus has been to determine whether DNA denaturation, known to occur during heating, may be a reliable indicator of the plasma’s elevated gas temperature. In parallel, we performed measurements of LTP gas temperature using a conventional temperature sensor. Surprisingly, we observed denaturation at the combination of plasma parameters that form the jet with a temperature much below the thermal decomposition of DNA. To understand this effect, we implemented a physics-guided neural network model to predict the formation of strand breaks and denaturation and their yields for a given combination of LTP parameters. Using predictive modeling, we obtained the evolution of these two types of DNA damage as a function of voltage (and power), frequency, flow rate, and irradiation time. Based on our findings we suggested that denaturation of DNA can be attributed to transient local heating of the aqueous DNA, (“hotspots”), while bulk heating was not observed.
Within the past decade micro-plasma jets in contact with liquids have been the focus of international research. They have shown great potential in applications ranging from surface treatment to medicine. To be able to control these jets for precise application, a fundamental understanding of the underlying processes is required. For this, detailed diagnostics need to be performed, which are challenged by the plasma jet’s high gradients, multiphase transport processes and interfaces of plasma and liquid or solid.
Most conventional plasma diagnostics fail in cases of non-equilibrium processes at atmospheric pressure. Ultrafast laser spectroscopy, however, permits the diagnostic of fundamental plasma properties such as reduced electric field or flow properties and gas composition at timescales much shorter than collisional processes.
The talk presents current development in the field of ultrafast laser diagnostics and the challenges that single shot measurements have.
A compromise to gain information from single shot measurements and high signal to noise from averaging measurements can be gained from data post processing or advanced averaging methods.
Thomson scattering (TS), the elastic scattering of light photons by charged particles, is a powerful diagnostic for the measurements of electron properties (density and temperature) in low-temperature plasmas (LTP). It is in fact one of the few diagnostics capable of providing simultaneously electron density (ne) and electron temperature (Te) information at the nanosecond timescale. As a result of the implementation of this diagnostic, many insights have been gained on electron kinetics in diverse low temperature discharges. In most of the situations, TS in LTP is encountered in the non-collective (or incoherent) regime, meaning that scattering signals from individual charged particles are added together. Besides, because ions are generally in thermal equilibrium with the neutrals constituting the background gas, TS is essentially giving information about the hot electrons. However, for high density plasmas (typically ne > 1017 cm-3), the collective (or coherent) TS regime is generally observed. In the collective regime. light photons are scattered off plasma waves (instead of individual charged particles). In such a configuration two different spectral features are observed: electron and ion features, which result from scattering off the so-called electron plasma waves (EPW) and ion acoustic waves (IAW), respectively. While the ion feature is observed near the probe laser spectral location, the electron feature is observed far from it. Conversely, scattering off IAW results in stronger collected signals than scattering off EPW. Probing simultaneously electron and ion features of a high density plasma would in principle provide a plethora of information regarding the plasma conditions: ne, Te, Ti (ion temperature), Z (average charge state), vei (electron-ion relative drift velocity) and V (fluid velocity).
We show through forward modeling the feasibility of implementing such a diagnostic for laser-produced tin droplet plasmas generated during the ablation of 30-80 µm tin droplets by a 10 ns Nd:YAG laser emitting at 1064 nm. Such plasmas are currently employed as extreme ultraviolet light sources (at 13.5 nm ± 1%) for the semiconductor industry.
Non-equilibrium effects are ubiquitous in laboratory plasmas and need to be considered to optimize the reactor performance for specific applications. In the low temperature plasma (LTP) community, there are on-going discussions on how to define reaction mechanisms and verify them. Such efforts would allow going toward predictive modelling and accelerate innovation. In this contribution, we will discuss a couple of cases illustrating different non-equilibrium effects which play a direct role in the yield of plasma (reactive) species. While external electric and magnetic fields come first to mind in controlling non-equilibrium plasma properties, we will focus more specifically on flow and wall effects. These effects are usually hard to quantify and generate additional challenges for constructing a plasma chemistry model and validating it. A better understanding (and/or control) of them would allow making significant steps forward in the development of predictive models. The current state-of-the-art will be outlined and steps toward the definition of reaction mechanisms discussed.
High energy neutrinos from cosmic sources are one of the most exciting subjects for study in particle physics. They allow access to energy ranges otherwise unobtainable and since neutrinos point back to their origin, they allow deep insights into the sources of the highest energy processes in the universe.
The P-ONE collaboration is aiming to construct a large scale ocean based neutrino observatory in the Canadian Pacific Ocean to provide new capabilities and added active volume to the existing, highly successful observatories around the world. We will report on the progress of designing and constructing a prototype sensor array for deployment in the ocean in the coming years.
Advanced LIGO and Advanced Virgo have confidently detected dozens of gravitational wave (GW) signals from colliding black holes and neutron stars. As these GW detectors improve and more are added to the global network, the expected rate of detected events will increase (with the cube of the sensitive range) and our ability to constrain the properties, including likely sky location, will improve. I will discuss the challenges for extracting a high expected rate of GW signals from noisy gravitational wave detector data and an emerging suite of machine learning methods developed to better distinguish true astrophysical signals from non-stationary LIGO detector noise. I’ll give my perspective on the implications for GW candidate alerts and future multi-messenger discoveries during the next international GW network observing run (expected to start in May 2023).
The planned upgrade of the Large Hadron Collider to quadruple the luminosity requires a substantial corresponding upgrade to the ATLAS detector in order to continue to keep up with the challenging experimental conditions that high luminosity imposes. Canada is participating in a wide range of these planned upgrades, with a particular focus on a new silicon strip detector and upgraded electronics for the liquid argon calorimeter. Recent progress and achievements will be discussed, as well as prospects for the physics reach of the upgraded detector.
Quantum chemistry has been identified as one of the prime applications for quantum computers. At present, the majority of quantum algorithm developments have the Noisy Intermediate Scale Quantum (NISQ) architecture in mind, for which it is important to design quantum circuits with low circuit depth to minimize noise and error propagation. In this presentation, I will present a modular circuit which allows for short circuit depths while allowing for a quantum chemical interpretation in terms of resonating valence bond structures. I will discuss applications in small molecular systems. Joint work with Ehsan Ghasempouri and Gerhard Dueck.
The search for the invisible dark matter particle is complicated due to the uncertainties in its distribution in our Galaxy. An accurate determination of the dark matter phase space distribution in the Solar neighborhood is crucial for the correct analysis and interpretation of data from dark matter direct detection experiments. Massive satellites such as the Large Magellanic Cloud can impact the dark matter halo of the Milky Way, and boost the dark matter velocity distribution in the Solar neighborhood. I will present the local dark matter distribution of Milky Way-like galaxies extracted from state-of-the-art cosmological simulations, and discuss their implications for direct dark matter searches. I will also discuss how the dark matter component of the Large Magellanic Cloud can alter the results.
I will give an overview of pseudo-Dirac dark matter, a scenario where a small Majorana mass splits charged Dirac dark matter into two nearly degenerate states. A longtime favourite of model-builders, this dark matter candidate has a rich phenomenology that still has yet to be fully characterized. I will discuss a few mechanisms for producing this kind of dark matter in the early universe, and will show various ways in which this candidate will manifest itself in the subsequent cosmology, astrophysical systems, and terrestrial experiments.
Antimatter and gravity are subjects of two of the biggest mysteries in physics: How can we explain the observed excess of matter over antimatter in the universe? And, how can the theories of gravity and quantum mechanics be unified? Antihydrogen, as the simplest purely antimatter atomic system, is a natural candidate for experimentally testing some fundamental theories related to these questions. For example, CPT (Charge-Parity-Time) symmetry predicts that the spectra of hydrogen and antihydrogen should be identical. Because the hydrogen spectrum is one of the best understood in physics, similar measurements of antihydrogen can provide a precise test of this symmetry. In addition, because antihydrogen is electrically neutral it can be used as a probe of the gravitational interaction between matter and antimatter. If the weak equivalence principle in general relativity holds, then the gravitational mass of antimatter should be identical to that of matter but so far there have been no direct free-fall style experiments to test this.
The ALPHA antihydrogen experiment at CERN’s Antiproton Decelerator has made major strides in the trapping and spectroscopy of antihydrogen. In recent years, the ALPHA collaboration has turned its attention toward the weak equivalence principle with the construction of a new apparatus, known as ALPHA-g, that aims to measure the gravitational acceleration of antihydrogen. In this experiment, antihydrogen atoms are magnetically confined and then allowed to escape up or down. The up-down balance of atoms that escape will allow a measurement of the gravitational acceleration of antihydrogen. ALPHA-g has been successfully commissioned and the first measurement campaign was completed in 2022. This talk will discuss the details of the ALPHA-g apparatus, the experimental methodology, and the latest results of the experiment.
The TRIUMF UltraCold Advanced Neutron (TUCAN) Collaboration is developing a new ultracold neutron (UCN) source for installation at TRIUMF. High energy neutrons will be produced by directing protons from the TRIUMF cyclotron onto a tungsten target. The neutrons will undergo moderation in two steps to reduce their energy, first in a heavy water then in a liquid deuterium moderator. The moderated neutrons then enter a superfluid helium volume where they will be converted into UCN through superthermal processes. The goal for the source is to produce the world's highest density UCN source surpassing current UCN source densities by at least one order of magnitude.
As UCN can be stored in material containers for hundreds of seconds they are ideal for experiments on the fundamental properties of neutrons. To take advantage of this the first experiment planned for this UCN source is a measurement of the neutron electric dipole moment (nEDM). For this experiment UCNs will be confined to a material bottle where they will precess at a rate that is proportional to their electric and magnetic dipole moments and the applied fields. By precisely measuring the difference in the precession frequency between parallel and anti-parallel field configurations the nEDM can be determined. According to current models we expect to have $1.43\times 10^{6}$ UCN detected per measurement cycle which should allow us to reach our goal statistical accuracy of $1\times 10^{-27}$ e-cm in $400$ measurement days. This is approximately 20 times more precise than the current world's best measurement that was done by the nEDM Collaboration at the Paul Scherrer Institut of $1.8\times 10^{-26}$ e-cm (90% CL) which had $1.5\times 10^{4}$ UCN per cycle, and is competitive with their planned future experiment n2EDM that anticipates $1.21\times 10^{5}$ UCN per measurement cycle.
I will describe the planned UCN source and nEDM experiment, as well as the current status of the efforts.
The pursuit of fundamental interactions requires ever increasing precision in theory and experiment. Ion-trapping techniques have been deployed and pioneered to investigate radioactive nuclides at the TITAN-TRIUMF facility. Experiments include precision mass spectrometry of superallowed $\beta$ emitters to investigate isospin symmetry and to test the unitarity of the quark-mixing matrix. To further these studies, a redesigned Penning-trap system has been commissioned to achieve precisions as low as $\delta m/ m \sim$ 10-10. In this talk, I will contextualize the new Penning trap and other technical developments for studies of fundamental symmetries.
Majorana zero modes appear at the edges of topological superconducting wires as part of the bulk-boundary correspondence in these systems. Thanks to topology, Majoranas are robust against weak perturbations and this makes them promising candidates for qubit building blocks. In Majorana-based qubits quantum information is stored non-locally, avoiding many sources of decoherence. In such qubits logical operations amount to coupling and exchanging Majoranas in space. This means that in order to perform quantum operations we need to learn how to manipulate Majorana modes while reducing diabatic errors.
In this talk we will discuss Majorana chains, how to improve their reliability and how to manipulate them safely on a wire.
Topological nanowires, topological materials confined in one dimension (1D), hold great promise for robust and scalable quantum computing and low-dissipation interconnect applications, which will transform current computing technologies. To do so, research in topological nanowires must continue to improve their synthesis and properties.
In this talk, I will discuss my group’s efforts to develop a high throughput and precision synthesis method to fabricate 1D topological systems (APL Materials 10, 080904 (2022)). I will highlight our studies on topological crystalline insulator SnTe nanowires and topological metal MoP nanowires and discuss their potential applications. Using SnTe nanowires as weak links in Josephson junction devices, we discover a novel superconducting phase (npj Quantum Materials 6, 61 (2021)). With MoP nanowires, we show that the resistivity scaling of MoP nanowires is superior to those of the state-of-the-art Cu interconnects and Cu alternative metals, presenting MoP as a breakthrough metal for the low-resistance interconnect applications (Advanced Materials doi:10.1002/adma.202208965 (2023)).
The scaling of interconnect wiring in integrated circuits leads to increasing resistivity of Cu wires and degrades the chip power-performance significantly. Current research on alternative interconnect conductors is largely limited to conventional metals for mitigating the growing line resistance. Here we explore topological conductors as a potential solution. Using CoSi and NbAs as examples, we find that, through the dominant surface-state conduction, the resistivity in topological semimetals reduces with decreasing feature sizes in the nanometer scale. This trend holds even in the presence of mild disorder and grain boundaries, in sharp contrast to conventional metals. We will present detailed first-principles calculations and report experimental evidence for unconventional resistivity scaling in CoSi thin films, showing resistivity significantly below that of ideal bulk single crystals. We will conclude with a set of guidelines to screen topological semimetals for beyond-Cu interconnects and a list of key next steps.
Acknowledgements: Hsin Lin, Ion Garate, Gengchiau Liang, Nick Lanzillo, Utkarsh Bajpai, Shang-Wei Lien, Yi-Hsin Tu, Sushant Kumar, Ravishankar Sundararaman, Christian Lavoie, Oki Gunawan, Asir Khan, Guy Cohen, John Bruley, Vesna Stanic, Jean Jordan-Sweet, Peter Kerns, Teodor Todorov, Nathan Marchack, Cheng-Yi Huang, Chuang-Han Hsu, Tay-Rong Chang, Arun Bansil.
Weyl semimetals (WSMs) are materials whose low-energy excitations are Weyl fermions. Since its first observation in 2015, much work has gone into understanding the various properties of the WSM, most notably the Fermi arc -- a surface projection of the Berry flux connecting the WSM's zero-energy points. Here, we study the effects of tunnelling on the band structure and Fermi arc of a time-reversal broken WSM. When coupled to a simple non-magnetic parabolic band, the WSM's chiral arc state lowers in energy and forms, together with a previously extended state, a noticeable spin-dependent asymmetry in the interface spectrum in the vicinity of the Weyl nodes reminiscent of tunnelling in a Dirac cone. We study these effects with a lattice model which we solve numerically on a finite sample and analytically using an ansatz on an infinite sample, with both continuum and lattice frameworks. Our model agrees very well with the numerical simulation as it accurately describes the behaviour of the chiral state, from its energy asymmetry to the spin canting at the interface. We also find that the tunnelling effectively increases the Fermi arc length, allowing for the presence of interface states beyond the bare Weyl nodes in agreement with previous work. These additional states may also carry current along the interface and we propose methods to detect them experimentally.
A quantum physicist by training, Dr. Martin Laforest spent his career ensuring quantum technologies have a disruptive, yet positive impact on industry and society. Martin is currently managing partner for Quantacet, an early stage, quantum-focused investment fund and the director of Quantum Strategy for ACET, a Sherbrooke-based deep tech incubator offering specific mentoring tailored to quantum enterprises. Martin also serves as a technical advisor for DistriQ, Sherbrooke’s quantum innovation hub. Before moving to Sherbrooke, Martin was the senior product manager for ISARA Corporation, a quantum-safe security company. Martin also spent eight years promoting the impacts of quantum technologies to students, governments, companies and investors for the Institute for Quantum Computing at the University of Waterloo where he also received his PhD.
Udson Mendes has a PhD in Physics from the University of Campinas in Brazil. He was a postdoctoral fellow at the Laboratoire Pierre Aigrain at the École Normale Supérieure de Paris, and then at the Institut Quantique at the Université de Sherbrooke. Dr. Mendes’ research has been focusing on the development of quantum technologies ranging from quantum hardware to quantum algorithms. Since joining CMC, he created the world’s first cost-sharing fabrication service for superconducting devices and helped to train over 170 high qualified personnel in CMC’s quantum workshops. Moreover, Dr. Mendes leverages his expertise to lead a team of quantum scientists working on applications ranging from cybersecurity to protein design to cancer diagnosis.
Nicholas obtained his Ph.D. in Physics from Simon Fraser University, where his research focused on the numerical and phenomenological modeling of impurities in superconductors. In 2021, he joined Photonic, a full-stack quantum computing company based in British Columbia, as its first Quantum Software Engineer, leading the development of a laboratory measurement and control system. Realizing the need to take a simulation-driven approach to quantum computer design, he went on to establish and lead the Quantum Software and Simulations team. His team, comprising several Software Engineers and Quantum Software Engineers, develops a diverse range of simulation and design tools to accelerate the development of Photonic's quantum computers.
Catalina holds a MSc. in Electronics from Los Andes University and Engineering Diploma from IMT Atlantique in France, with a research focus on autonomous systems. She’s currently Quantum Community Manager at Xanadu, where she helps build the community around PennyLane. Today she’s working with professors from around the world, helping them include quantum programming in their courses. In the past, Catalina worked at IBM, where she was an IBM Quantum Ambassador.
Session III: Active Soft Matter
A remarkable diversity of morphologies exists among flagellated bacteria and, more broadly, motile microorganisms. To understand some of the consequences of these design choices, we numerically simulate the swimming motion of flagellated bacteria and model squirmers using a boundary element method. We show that interactions with solid surfaces bounding their fluid environment are particularly sensitive to parameters such as the cell body aspect ration, the length, number and placement of flagella on the cell, and the effective stiffness of the flagellar hook. The behaviour of a bacteria-like swimmer near surfaces can be tuned by choosing particular configurations and varying the motor torque. We then characterize the interaction of swimmers with neutrally buoyant spherical particles in unbounded fluid. Interestingly, we find that large particles (e.g., 10 times the radius of the swimmer) can have a larger net displacement due to an encounter with a swimmer than smaller particles at the same impact parameter. This has implications for the effective enhancement of the diffusion coefficient of suspended particles in a bacteria-laden fluid. Based on numerical results, we estimate the effective diffusivity of a particle in a dilute bath of swimmers and show that there is a non-monotonic dependence on particle radius. Similarly, we show that the effective diffusivity of a swimmer scattering in a suspension of particles varies non-monotonically with particle radius. As with interactions with a planar surface, the details are highly dependent on the chosen swimmer, allowing the enhancement of diffusion to selectively affect particles of a specific size more or less.
The material state of embryonic tissues emerges from the collective interactions of cells. Most tissues are soft active materials that can flow or deform. This deformability is shown to be important for proper embryonic development. However, cell and tissue mechanics are experimentally difficult to probe in developing animals. Here, I will discuss our research developing computational and theoretical models to investigate how tissue material properties affect cellular functions and coordination. I will present verifiable mathematical models and predictions that we developed for various developmental processes.
Colloids are mesoscopic particles that enable a systematic study of inter-particle interactions in soft materials. The depletion interaction is an attractive effective interaction that can be tuned by polymer additives, while the amplitude and frequency of an external electric field can be used to tune the dipolar interaction. Using these two interactions simultaneously, we create multi-tunable colloids where weak depletion results in increase crystalline order while stronger depletion increases disorder and results in novel gel states [1]. With these “dipolar-depletion” gels, we examine the onset of irreversibility and find strategies to accelerate aging.
[1] Shivani Semwal, Cassandra Clowe-Coish, Ivan Saika-Voivod, Anand Yethiraj, “Tunable colloids with dipolar and depletion interactions: towards field-switchable crystals and gels.”, Physical Review X 12, 041021 (2022).
Burst-mode ultrafast laser-materials treatments use high-repetition-rate (>MHz) delivery of femtosecond laser pulses. This takes advantage of characteristically tiny residual heat left in a substrate through individual femtosecond-laser-matter interaction. At the same time, the approach opens the door to manipulating the accumulation of that same tiny heat from rapid repetition. This mode of fluence-delivery can, for instance, transition brittle materials like glasses to ductile states, then cut aggressively while ductile and not susceptible to fracture, before the material naturally returns to its brittle state.
In solid dielectrics, isolated sub-picosecond laser pulses first create a limited plasma from nonlinear ionization, then they increase that plasma through collisional ionization. Used in burst-mode, the hypothesis is that some residual ionization persists for a few nanoseconds, meaning that subsequent pulses need not re-initiate dielectric breakdown. Instead, they see linear absorption in a state comparable to a metal or semiconductor. In effect, the plasma is ‘simmered’ continuously throughout a burst, controlling the mode and amount of absorption.
We report studies of the persistence of the plasma state in fused silica within a burst of ~60 pulses, each of 300 fs duration, arriving with an intra-burst repetition rate of 200 MHz (5ns separation). We measure -- pulse-by-pulse during the burst -- the partition of energy into specular scattering, diffuse scattering, transmission through the sample, and absorption of laser energy. With this, we determine the decay of the plasma created by one pulse, until the arrival of the next pulse 5 ns later, and we characterize the subsequent re-growth of the plasma.
In this picture, the absorption of any given pulse depends on the recent history of irradiation. The material response is therefore non-local in time, which we can then frame as a material susceptibility that depends on the frequency of the intra-burst repetition rate.
Filamentary plasma structures aligned with magnetic fields are ubiquitous in various space and laboratory plasma environments. In numerous magnetic confinement devices, such coherent structures called blobs or blob-filaments, are intermittently formed in the boundary layer region of the device and transported across magnetic field lines through ExB convective motion. These structures can be much more efficient at transporting particles and energy than standard diffusive processes, therefore it is important to understand their propagation and stability. The magnetized plasma pressure filaments are often created in pairs or bundles, therefore filament-filament interaction is important for purposes of estimating their lifetime. One other feature of these structures, is the presence of internal steep pressure gradients, with density and temperature gradient scale lengths on the order of the cross-field filament size. This provides a free energy source for driving spontaneous low frequency excitations such as drift waves and vortices. It is the purpose of this study to understand the nonlinear saturated state of small scale (few electron skin depths) magnetized plasma pressure filaments that undergo drift wave turbulence driven by their internal pressure gradients. Experiments were designed to form controlled plasma pressure filament structures within a large linear magnetized plasma device; for this purpose the upgraded Large Plasma Device (LAPD) operated by the Basic Plasma Science Facility at UCLA was used. The setup consists of single or multiple biased probe-mounted cerium hexaboride (CeB6) crystal cathodes that inject low energy electrons along a strong magnetic field into a pre-existing cold afterglow plasma, thus forming plasma pressure filaments. Langmuir probes inserted in the plasma measure the low frequency (~10-20 kHz) gradient-driven fluctuations. A statistical study of the fluctuations reveals amplitude distributions that are skewed, which is a signature of intermittency in the transport dynamics. Large amplitude temperature fluctuation bursts have been analyzed and are related to spatiotemporal structures which propagate azimuthally and radially outward from the filaments. Details on the time scales of density, temperature and vorticity mixing in the interacting filaments will be presented along with fluid and kinetic simulation modeling results.
Plasma flow and acceleration in the magnetic nozzle with converging-diverging magnetic configuration are important for applications in electric propulsion and fusion systems such as open mirrors and tokamak divertors. We report on some features of plasma acceleration in the magnetic nozzle that have been revealed in recent analytical and computational studies. The non-monotonic magnetic field with a local maximum of the magnetic field is necessary for forming the quasineutral accelerating potential structure with a unique velocity profile entirely determined by the magnetic field. The explicit form of the solution can be obtained in the form of the Lambert function. The fluid model has been further extended to include the effects of warm ions with anisotropic ion pressure. It is shown that the perpendicular ion pressure enhances plasma acceleration due to the mirror force. The kinetic effects have been investigated using the quasineutral hybrid model with kinetic ions and isothermal Boltzmann electrons. It is shown that in the cold ions limit the velocity profile agrees well with the analytical theory. The full kinetic simulations, including the ions and electrons within the quasi- two dimensional paraxial model, further confirmed these results. Further generalization includes the role of the induced azimuthal magnetic field and plasma rotation, i.e., coupling with Alfven wave dynamics. It is shown that the inhomogeneous magnetic field couples the axial plasma flow with the evolution of the azimuthal magnetic field and plasma rotation resembling the problem of the magnetically driven flow in astrophysical jets and winds. The role of the Alfven, slow, and fast magnetosonic point singularities in plasma acceleration is discussed.
Long-lived particles (LLPs) are well-motivated signatures that can appear in many models of physics beyond the Standard Model. The Detection ability of LLPs at current accelerator-based experiments is restricted, as they may decay outside of the tracking acceptance of these experiments, especially for LLPs with masses above GeV and lifetimes at the limit set by Big Bang Nucleosynthesis, ∼10$^7$–10$^8$ m. In order to directly detect the decays of LLPs across a broad range of masses and lifetimes, MATHUSLA experiment is proposed for the HL-LHC at CERN to be located on the surface above the CMS experiment, with a decay volume of 100m x 100m x 30m instrumented with plastic scintillators and SiPM readout. LLPs that decay within this volume are reconstructed by tracking their decay products and finding a displaced vertex. This talk presents the physics cases and development progress of MATHUSLA experiment.
Silicon photomultiplier (SiPM) technology displaced photomultiplier tubes in the design of next-generation experiments in particle physics. This presentation will focus on astroparticle physics experiments that will use liquid argon or liquid xenon with SiPM photo-detectors for rare-event searches such as dark matter, neutrinoless double beta decay, solar neutrinos, supernova neutrinos, and coherent elastic neutrino-nucleus scattering. The photo-detector requirements for these experiments will be discussed, including ultraviolet photon detection efficiency (either direct sensitivity or with a wavelength-shifter), low radioactivity, and low noise rates to enable low thresholds. This talk will also feature the latest developments in photon-to-digital converter (PDC) technology, where signals from each photodiode are digitized in situ, and its proposed applications in future experiments.
The MoEDAL experiment deployed at IP8 on the LHC ring was the first dedicated search experiment to take data at the LHC in 2010. It was designed to search for Highly Ionizing Particle (HIP) avatars of new physics such as magnetic monopoles, dyons, Q-balls, multiply charged particles, massive slowly moving charged particles and long-lived massive charge SUSY particles. We shall report on our search at LHC’s Run-2 for Magnetic monopoles and dyons produced in p-p and photon-fusion and detail our most recent result in this arena: the search for magnetic monopoles via the Schwinger Mechanism in Pb-Pb collisions, recently published in Nature. The MoEDAL detector will be reinstalled for LHC’s Run-3 to continue the search for electrically and magnetically charged HIPs. As part of this effort we will initiate the search for massive long-very lived SUSY particles to which MoEDAL has a competitive sensitivity. An upgrade to MoEDAL, the MoEDAL Apparatus for Penetrating Particles (MAPP), approved by CERN’s Research Board is now the LHC’s newest detector. The MAPP detector, positioned in UA83, expands the physics reach of MoEDAL to include sensitivity to feebly-charged particles with charge, or effective charge, as low as 10-3 e (where e is the electron charge). Also, the MAPP detector In conjunction with MoEDAL’s trapping detector gives us a unique sensitivity to extremely long-lived charged particles. MAPP also has some sensitivity to long-lived neutral particles. Additionally, we will very briefly present on the plans for the MAPP-2 upgrade to the MoEDAL-MAPP experiment for the High Luminosity LHC (HL-LHC). We envisage that this detector will be deployed in the UGC1 gallery near to IP8. This phase of the experiment is designed to maximize MoEDAL-MAPP’s sensitivity to very long-lived neutral messengers of physics beyond the Standard Model.
One of the exciting new frontiers in cosmology and structure formation is the Epoch of Reionization (EoR), a period when the radiation from the early stars and galaxies ionized almost all gas in the Universe. This epoch forms an important evolutionary link between the smooth matter distribution at early times and the highly complex structures seen today. Gaining insights into this epoch has been quite challenging because the current generation of telescopes are only able to probe the tail end of this process. Fortunately, a whole slew of instruments that have been specifically designed to study the high-redshift Universe (JWST, ALMA, Roman Space Telescope, HERA, SKA, CCAT-p, SPHEREx), are about to come online. This will unleash a flood of observational data that will usher the study of EoR into a new, high-precision era. It is, therefore, imperative that theoretical/numerical models achieve sufficient accuracy and physical fidelity to meaningfully interpret this new data. In this talk, I will introduce the THESAN simulation framework that is designed to efficiently leverage current and upcoming high redshift observations to constrain the physics of reionization. The multi-scale nature of the process is tackled by coupling large volume (~100s Mpc) simulations designed to study the large-scale statistical properties of the intergalactic medium (IGM) that is undergoing reionization, with high-resolution (~ 10 pc) simulations that zoom-in on single galaxies which are ideal for predicting the resolved properties of the sources responsible for it. I will briefly discuss applications from the first set of papers, including predictions for high redshift galaxy properties, the galaxy-IGM connection, Ly-α transmission and back reaction of reionization on galaxy formation. I will then highlight the potential for using line intensity mapping of spectral lines originating from the interstellar medium (ISM) of galaxies and the 21 cm emission from the neutral hydrogen gas in the Universe to constrain galaxy formation and cosmology. I will finish by highlighting how this numerical framework, coupled with accurate observational predictions promises important and potentially transformative changes in our understanding of the primitive Universe.
The multimessenger binary neutron star merger GW170817 and subsequent LIGO-Virgo gravitational-wave discoveries are shedding new light on the ultra-dense matter inside neutron stars. With densities and pressures several times greater than those in atomic nuclei, neutron star cores harbour the most extreme matter in the Universe. Its composition remains an open question: does it consist entirely of hadrons, like neutrons and protons, or does a more exotic state, like quark matter, prevail at the highest densities? I will describe what gravitational-wave observations are revealing about the neutron star interior, and how future-generation observatories will revolutionize our understanding of ultra-dense matter.
Just over 65 years ago Burbidge, Burbidge, Fowler, and Hoyle (B2FH) charted the initial roadmap for nuclear astrophysics. This seminal work recognized that explaining the origins of the heavy elements such as lead, gold, and uranium requires at least two types of neutron capture nucleosynthesis processes with each having distinct astrophysical sites. At the time of B2FH the rapid neutron capture process (r-process) showed itself to be related to explosive astrophysical events largely via the signature of exotic, neutron-rich nuclei in the Solar abundances. Fast forward to today and we have now seen heavy element formation in the act via the impact of lanthanide elements on the observed light curve from the GW170817 merger of two neutron stars. Therefore, nowadays nucleosynthesis studies have several distinct types of observational information to assimilate, presenting the opportunity to make big leaps in our understanding of r-process sites. However, this requires careful consideration of the nuclear physics uncertainties associated with the vastly uncharted territory of neutron-rich nuclei. With both experimental and theoretical efforts providing key inputs for theoretical r-process studies, in this talk I will discuss how nuclear physics campaigns will play a central role in deciphering observables of heavy element production over the next decade.
Justin Furlotte is a Data Scientist with Fiddlehead Technology in Moncton, New Brunswick. His academic background included a BSc in Mathematics-Physics from the University of New Brunswick, followed by a MSc in Mathematics at the University of British Columbia, where he researched the quantum Hall effect and quantum lattice systems. Justin has also previously worked with a thermal analysis company called C-Therm Technologies in Fredericton, New Brunswick, performing computational physics as a Research Scientist. Today, Justin still uses mathematics on a regular basis and spends most of his time creating statistical forecasts on the sales data of large clients in the food and beverage industry.
With a career path spanning over 20 years across several continents, I followed and adapted to the opportunities as they arose. Beginning from an applied physics base, I have worked in; defense, solved product heat treatment problems using 1st principles physics, destroyed products, destroyed plasma coating machines, then designed and built them, developed thin film coating material solutions from cutting tools to solar panels to erosion-corrosion coatings in gas turbine engines. The path to success has been a constant battle of destruction and redesign to test new concepts and bring them to market.
This process of creative destruction got me interested in the innovation process and teams, then management, then complex systems.
Now I am involved in two very different but complimentary start-up companies, one in plasma physics that helps other companies grow, and one leveraging bleeding edge developments in theoretical and applied physics to apply a general physics solution to any problem. The interesting part is how the different experiences have required different physics skills sets, but there is one core feature from my physics training I have needed every step of the way - this I will share with you.
Today we stand at an inflection point for society, one where we can accelerate the innovative growth for humanity with a minimum of harm or hit a Fermi bottleneck. Let’s focus on the former but be mindful of the latter.
Medical physicists are health care professionals with specialized training in the medical applications of physics. Their work often involves the use of x-rays, ultrasound, magnetic and electric fields, infra-red and ultraviolet light, heat and lasers in diagnosis and therapy. Medical physicists work in hospital diagnostic imaging departments, cancer treatment facilities, hospital-based research establishments, universities, government, and industry. The majority of medical physicists work in radiation therapy as clinical medical physicists and their role within this particular field will be highlighted. The education pathway to becoming a medical physicist will be discussed, including CAMPEP requirements for certification.
Building on our accurate measurement of the $\beta$ direction's asymmetry with respect to decaying polarized $^{37}$K [B. Fenker PRL 120 062502], we plan further measurements of the momenta of the recoiling progeny nucleus in coincidence. $^{37}$K's decay to its isobaric analog state has similar sensitivity to unknown physics compared to neutron decay, while a nuclear structure feature where the d$_{3/2}$ unpaired proton naturally produces a tiny nuclear magnetic moment keeps known higher-order corrections small. The angular distribution of the outgoing leptons is predicted from their helicity combined with angular momentum conservation, and we've realized one of our experiments would be the most direct measurement of the $\nu$ helicity since the Brookhaven 1958 measurement. Adding $\gamma$-ray detection with high-Z GAGG scintillators enables our search for a time reversal-breaking correlation of $\beta$, $\nu$, and $\gamma$ momenta in radiative $\beta$ decay, sensitive to a hypothetical dark strongly interacting sector. Time reversal-breaking interactions in the final nucleus in isospin-hindered $\beta$ decay compete with the Coulomb interaction instead of the strong interaction, potentially enhancing sensitivity by 1000x to make it complementary to neutron EDM and neutron resonance time reversal tests. We are beginning a program to measure isospin breaking in isospin-hindered $^{47}$K and $^{45}$K decay to determine our sensitivity. $^{47}$K decay, since parent and progeny are near closed shells so there are few final states, may exhaust the expected matrix element size in analog-antianalog isospin mixing.
The nEXO experiment is a proposed next-generation liquid xenon detector to search for neutrino-less double beta decay (0νββ) of 136Xe. The experiment will use a 5-tonne liquid xenon monolithic single-phase time projection chamber enriched to 90% 136Xe. Ionization electrons and scintillation photons from energy deposits in the Xe will be recorded by a segmented anode place and a large SiPM array. This talk will present recent progress in the detector design, an improved modelling of signal readout and the development of a deep neural network based data analysis architecture to improve signal/background separation. These developments result in a 90% CL 0νββ halflife sensitivity of $1.35\times10^{28}$ yrs in 10 years of data taking.
Probing electroweak physics at low energies plays an important role in the search for physics beyond the Standard Model. The exchange of Z bosons between an atom’s electrons and quarks induce an incredibly small atomic transition which can be probed via an atomic parity-violation (APV) experiment. APV measurements are sensitive as searches for leptoquarks and additional neutral gauge bosons and provide complementary results to higher-energy experiments. APV effects scales with the proton number ~Z^3. The extraction of electroweak physics from the observed signal requires atomic theory which is currently only available for alkali configurations. This makes neutral francium an ideal candidate for such experiments. Our goal is to measure APV effects using 10^6-10^7 laser-trapped neutral francium atoms at ultra cold temperatures. To this end , we have established an online neutral atom trap at the ISAC radioactive beam facility at TRIUMF in Vancouver. In this talk, I will discuss our progress towards an APV experiment in francium with a look at our recent observation of the highly forbidden 7s-8s magnetic dipole transition and our new detection scheme, bringing the observation of APV into reach.
Funding supported by NSERC and TRIUMF via NRC, and the Universities of Manitoba and Maryland.
Several high profile quantum algorithms have failed in the last decade, meaning that a better classical algorithm has been found. This has been especially pronounced in the field of quantum machine learning. While some methods have known bounds and are definitely faster than classical algorithms, the practicalities of finding a good working quantum algorithm capable of effecting real change remain a main goal in the field. I cover the issues and cover the current status of the field in an attempt to summarize the current issues and future outlook.
While photons are poised to play a key role for a wide range of quantum technologies, several experimental barriers still need to be overcome for most practical applications. In this talk, I will first present a brief overview of the advantages and drawbacks of using photons for quantum information, before discussing some important research directions currently being pursued in order to address these challenges.
Artificial intelligence plays an increasing role in many situations in our everyday lives. Its immense power finds applications in various fields, recently also including the field of quantum many-body physics. Artificial neural networks have led to improved numerical studies of qubit systems, increasing our understanding of these systems, which build the foundation of quantum computers and quantum simulators. In this talk, I will summarize recent breakthroughs achieved with artificial neural networks in quantum physics and provide an outlook of what to expect in the near future.
Resource theories provide a unifying framework to characterize the usefulness of quantum objects with respect to specified tasks. In this talk I will present the main ideas, showing that such a framework is quite general, and seemingly different phenomena can be all described within it. I will also chart some promising directions for future developments in this area of quantum information.
While qubit is the basic unit in most quantum information devices and applications, there is another class of quantum system that offers infinite states per degree of freedom. Bosonic systems, in this respect, are everywhere and provide loads of practical advantages. In this short talk, I will introduce the basics and features of bosonic quantum technologies, and try to convince you that we should go beyond qubits in the coming decade
The quantum computing stack is the sequence of transformations that must be performed for the high-level description of a quantum algorithm to be executed on a (concrete or hypothetical) quantum computer. In this talk I will discuss old and new developments in the field and comment on the role that the quantum stack can play in the advent of practical quantum computing.
Coherent scattering of photons in a dilute vapour of alkali atoms provides a strong link between the quantum information stored in the photonic and collective spin Hilbert spaces. In our lab we are looking at the mapping of photonic quantum states into and out of collective spins. By continuously scattering, we are creating highly correlated beams exhibiting EPR entanglement as well as quadrature and intensity squeezing below the standard quantum limit.
Coherent scattering of photons in a dilute vapour of alkali atoms provides a strong link between the quantum information stored in the photonic and collective spin Hilbert spaces. In our lab we are looking at the mapping of photonic quantum states into and out of collective spins. By continuously scattering, we are creating highly correlated beams exhibiting EPR entanglement as well as quadrature and intensity squeezing below the standard quantum limit.
Session IV: Physical bioenergetics: Energy fluxes, budgets, and constraints in cells
Bacteria are often assumed to allocate cellular resources to maximize their exponential growth rate. This postulate, derived from studies of Escherichia coli, is commonly interpreted as an economic principle, in which the cell balances supply of and demand for “metabolic currencies” such as amino acids during steady-state growth. However, testing these predictions has been a major experimental challenge. Here, we show that Bacillus subtilis, another model bacterial organism, deviates from this growth maximization paradigm. To this end, we modulated the rate of rRNA and ribosome synthesis by controlling the cellular GTP concentration. In nutrient-limited conditions, perturbations to ribosome production always reduced the growth rate. In stark contrast, under inhibition of translation with antibiotics, increased ribosome production led to faster growth. Using proteomics and LC/MS, we trace this submaximal growth to a reduction in GTP level upon translation inhibition, which leads to overproduction of metabolic enzymes at the expense of ribosomal proteins. We conclude that different organisms follow organism-specific resource allocation principles, perhaps as a consequence of evolution.
Perturbation experiments—where the response of a system of interest is observed after exposure to drugs or disruptions—are commonly used to identify interactions in biochemical reaction networks. However, it is often the case that the data is only analysed for its deterministic averages, and analysis techniques also rely on specific knowledge of each perturbation’s targets. We use constraints on interaction topology between the correlation and variation of molecular responses in two-component systems to analyse large-scale drug perturbation studies, in the absence of specific knowledge of the perturbations. We further show how analysis of variability in deterministic molecular responses is affected by non-linearity, stochasticity, and finite-sampling of perturbations.
Drug resistance is a global health threat that is undermining the advances of modern medicine. Non-genetic forms of drug resistance have been established over the last two decades to play an important role in drug resistance. However, the interplay between non-genetic and genetic forms of drug resistance is largely unknown, as are the evolutionary dynamics in fluctuating drug conditions.
Recently, we have shown using deterministic models and stochastic simulations that non-genetic drug resistance enhances the survival of a cell population undergoing drug treatment, while hindering the genetic evolution of drug resistance due to competition between non-genetically and genetically resistant subpopulations. This effect is enhanced in fluctuating drug conditions compared to constant drug conditions.
We are testing these predictions in evolution experiments on genetically engineered yeast harbouring synthetic drug resistance gene circuits. Synthetic resistance gene circuits are well characterized, mimic natural gene networks, and allow gene expression mean and “noise” (i.e., cell-to-cell variability among genetically identical cells) to be precisely controlled and quantified. Preliminary results from these evolution experiments in fluctuating drug conditions demonstrate that gene expression evolves to optimize growth rates, and, counterintuitively, that expression noise levels are reduced in fluctuating compared to constant drug conditions.
Overall, these investigations on quantitative model systems are enhancing our fundamental understanding of drug resistance evolution, which is essential to prolong and extend our armamentarium against drug-resistant infections.
The ionosphere, an ionized part of the Earth’s atmosphere, affects radio waves passing through it. The ionosphere and structures in them can cause disruptions in communication, position, navigation, and timing (CPNT) systems that rely on radio signals. These effects are scale dependent and driven by plasma turbulence (irregularities) in the ionosphere. The impact of ionospheric plasma turbulence on CPNT systems is significant and ranges from correctable/manageable errors to catastrophic failure of CPNT systems. For most applications, these effects can be broadly categorized into deterministic and stochastic. This talk will outline the impact of plasma turbulence on CPNT systems and methods to mitigate some of these detrimental effects on these critical systems. The talk will also discuss the use of these impacted signals in fundamental research on plasma turbulence and ionospheric irregularities.
Plasma Immersion Ion Implantation (PIII) is a powerful high-fluence ion implantation technique in which the target to be implanted is immersed in a plasma containing the desired ion species. PIII finds a wide variety of applications in semiconductor processing. A more recent area of application for our PIII technology is treatment of candidate materials for Plasma Facing Components (PFCs) intended for use in plasma fusion devices such as the ITER tokamak. PIII can be used to simulate the high fluence ion bombardment encountered in plasma fusion devices, and therefore provides a useful tool for PFC testing. This talk will discuss various fundamental aspects of PIII which are relevant to the PFC testing problem, and present recent results in this area.
Plasma Immersion Ion Implantation (PIII) consists in immersing in a plasma a negatively biased target (or electrode) with high voltage (HV) pulse in order to drive ions into the target and change the target surface structure and/or composition. This process has broad applications in the field of materials processing as well as semiconductor manufacturing. Improving PIII operational efficiency depends on a precise control of the ion fluence which itself relies on a rigorous empirical knowledge of the plasma behaviour during the HV pulses and in close proximity (~1 mm) to the electrode surface. The aim of this research is to study the behaviour of plasma parameters (electron density, electron and ion temperature, plasma potential and ion velocity) in a low-temperature inductively coupled plasma (ICP) chamber used for PIII. In order to obtain spatially resolved information with minimal plasma disturbance, Laser-Induced Fluorescence (LIF) was chosen to study the ion velocity distribution function. LIF measurements of the ion velocity distribution function during PIII have never been done, and will provide crucial insight into poorly known plasma dynamics. By monitoring the ion velocity in the region around the pulsed electrode, technologies such as semiconductor processing may become more efficient, less wasteful, and even more precise.
Ion temperature measurements were made in the bulk plasma during steady state operation for a range of power and pressure values (350-500W and 0.8-2 mTorr). It was found that ion temperature increases with increasing pressure. This is counter-intuitive considering increased pressure means more neutral gas particles, which would imply more collisions between ions and neutrals, thereby reducing ion temperature. LIF was also used to perform spatially resolved measurements of the ion velocity distribution function in the vicinity of the pulsed HV electrode in order to measure the average ion velocity near the electrode, deduce the sheath structure and measure the Bohm velocity, Cs. It was found that the ion velocity reaches Cs at 2 mm from the electrode surface. This falls within the theoretical estimate of the sheath length according to the electron density and temperature measured by means of Langmuir probes. This result is significant since the ion velocity and sheath length are essential parameters in an ICP used for PIII. Future experiments will focus on time-resolved measurements of the plasma under PIII relevant conditions.
Plasma discharges contains two distinct zones having different physical properties, namely the quasi-neutral bulk plasma and the sheath where the quasi-neutrality does not hold, separated by an intermediate transition zone called pre-sheath [1]. In particular, the sheath has a strong impact on the entire gas discharge since it is where the plasma interacts with the boundaries. The plasma-sheath transition is still a subject of active research today mainly due to its complex structure [2,3]. The modelling of an entire plasma discharge including the dynamics of sheaths is crucial to understand the behaviour of different plasmas such as nano-particle creation in sputtering magnetron discharge [4], also observed in the coldest region of tokamaks [5].
In this context a new and reliable numerical model for low-temperature plasma discharges including the sheaths is currently under development. Although kinetic models and Particle-In-Cell (PIC) methods [6, 7] are often preferred for their fidelity, they are limited by numerical constraints on the simulation time and memory requirements due to the high number of macro-particles necessary to accurately simulate high density plasmas and the sheaths.
Fluid approaches are limited by the model accuracy itself, but are less demanding in computational resources and is still capable of giving insights of the main physical phenomenon.
In this work, we focus on 1D plasma fluid model adapted for the simulation of medium to high pressure ($10^{-1}$ - $10^{2}$Pa) direct-current (DC) argon discharges.
In particular, a non quasi-neutral drift-diffusion model of two charged species – ions and electrons was developed aiming at correctly modelling the sheaths. The results are compared with PIC simulation outputs. Our results emphasize for the first time the importance of the ion temperature profile when their collisionality in the sheaths is not negligible.
References
[1] Langmuir I, Proceedings of the National Academy of Sciences 14 627–637 (1928)
[2] Hershkowitz N, Physics of Plasmas 12 055502 (2005)
[3] Riemann K, Plasma Sources Science and Technology 18 014006 (2008)
[4] Arnas C et al., Phys. Plasmas 26, 053706 (2019)
[5] Arnas C et al., Plasma Physics and Controlled Fusion 52 124007 (2010)
[6] Hagelaar G et al., Journal of Applied Physics 93, 67 (2003)
[7] Sahu R et al., Phys. Plasmas 27, 113505 (2020)
Microwave plasmas are hugely-studied plasmas, they have characteristics that make them unique, they can be generated for low and high-pressures, they have relatively high densities of charged particles, and can be generated in different cavity geometries. It has been proven that pulsing a microwave discharge can be beneficial for multiple application. Indeed, power interruption reduces gas heating and create one more tuning parameter for the plasma. To investigate microwaves plasmas parameters, most OES diagnostic methods rely on the use of a collisional radiative model. These kind of models assume apparent steady state of the plasma to determine key plasmas parameters from optical emission spectroscopy measurements. With pulsed plasma, the steady state hypothesis can not always be made.so collisional radiative models can’t be used to study these plasmas. A method relying on line trapping of argon 4p-4s transitions was developed to determine 4s argon level densities without assuming steady state. To verify this method, both OAS measurements and the line ratios method were performed on a surface wave plasma with pressure ranging from 500 mTorr to the atmospheric pressure. This method was then used to study relatively two microwave pulsed plasmas: a time reversal plasma and a pulsed Tiago torch.
Cancer incidence is on the rise in Canada, and metastasis is often associated with lowered life expectancy. Bone, especially the spine, is the common site of metastasis for breast, lung and prostate cancers. Treatments for these tumors rely on heavy doses of chemotherapeutic agents and invasive surgical procedures, which usually extend onto healthy tissue. This difficult procedure often requires bone reconstruction and graft, but also leaves high risks of open wound infection. The introduction of a cold plasma treatment promises to be a novel therapy that to aid surgical intervention. While empirical plasma medicine shows promising results, the reaction mechanism between plasma and tissues, proper treatment dosage and reactive species composition to reach hormesis are still unknown at large. Therefore, a plasma-bio interaction platform which combines a 3D-bioprinted tissue model to an automated cold plasma source is proposed. To ensure biocompatibility of the treatment, highly sensitive diagnostic techniques are necessary. By exploiting the thermo-optic effect on a fibre Bragg grating, measurements in the shift of the reflected wavelength exposed to a plasma source was used to estimate the temperature. This technique, coupled to the plasma jet, brings a novel approach for temperature characterization. It accurately shows its capability to attain a maximum temperature up to 40 °C inside the effluent while interacting with a dielectric surface. Similarly, colorimetric assays for nitrite and hydrogen peroxide detection have also confirmed that these long-lived species can be tailored through the electric pulse duration, the distance, the duration of treatment and the surrounding conditions. These results, combined with promising 2D in vitro treatment of MDA-MB-231 breast cancer cell line, show great potential toward tailoring of the plasma for personalized medicine.
The neutron lifetime from beta decay, τ , is a significant value for predictions in particle physics and cosmology. It is used to verify the unitarity of the Cabbibo-Kobayashi-Maskawa (CKM) matrix, the weak force quark mixing matrix in the Standard Model, and for evaluating the abundances of light elements such as Helium-4, created during big bang nucleosynthesis. Furthermore, there is a 3.6 σ discrepancy of neutron lifetime results from beam experiments (τ beam = 887.7 ± 1.2 ± 1.9s), and ultracold neutron (UCN) trap experiments (τ trap = 877.75± 0.28(+ 0.22/− 0.16s)). The measurements should agree, since beam experiments measure daughter particles from beta decay, and trap experiments measure surviving neutrons. The discrepancy may be evidence of Physics beyond the Standard Model or an undiscovered systematic effect. A more precise value of the neutron lifetime from beam or trap experiments provides more constraint on the predictions in particle physics and cosmology that are dependent on neutron lifetime. PENeLOPE (Precision Experiment on the Neutron Lifetime Operating with Proton Extraction), developed by Technical University of Munich, Germany, is a UCN magneto-gravitational trap experiment with a goal of determining the neutron lifetime to a precision of 0.1s. In this presentation, I will briefly discuss the motivation for the measurement, how UCN are trapped in PENeLOPE, and how the experiment cycle of PENeLOPE is optimized to reach a sensitivity of 0.1s.
Cosmological dark matter remains an important unsolved problem in physics. Direct detection using liquid argon offers exciting discovery potential to the “neutrino fog” with sensitivity to spin-independent WIMP-nucleon cross sections below $10^{-48}\,\mbox{cm}^{2}$. A program of phased deployment of ever more sensitive detectors will be described, including the upgraded DEAP-3600 experiment at SNOLAB, the DarkSide-20k experiment at Grans Sasso Laboratory, and ARGO, a multi-hundred tonne future detector at SNOLAB. We discuss control of important backgrounds throughout the program and highlight some of the technologies to reduce those backgrounds including surface coatings, low-radon assembly, and readout and electronics.
In the Fall of 2019, the NEWS-G experiment used its latest detector, a 140 cm diameter Spherical Proportional Counter (SPC) to search for low-mass dark matter at the Laboratoire souterrain de Modane (LSM), in France. SPCs are metallic spheres filled with gas, with a high voltage anode at the centre that attracts and amplifies ionization charges coming from atomic recoils. Having the sphere filled with pure methane, hydrogen was used as the target to produce new limits on the proton spin-dependent cross-section around masses of 1 GeV.
This talk will first introduce the NEWS-G experiment and describe the commissioning at the LSM with the shielding used, the SPC detection principle and the new multi-anode sensor. It will then focus on the calibrations using a UV laser and argon-37, as well as the background discrimination methods to remove alpha-induced events and spurious pulses coming from the electronics. Finally, it will explain the profile likelihood ratio method that was used in order to derive constraints on WIMP mass and cross-section.
Measurement of the charged-pion branching ratio to electrons versus muons, Re/μ, is extremely sensitive to a wide variety of new physics effects. The precision of the SM prediction for Re/μ is ~1 part in 10^4, 15 times more precise than the current experimental result. A next-generation experiment, PIONEER, is aiming at reducing the precision gap between theory and experiment, testing lepton flavor universality at an unprecedented level and probing new physics mass scales up to the PeV range. Additionally PIONEER is aiming at a 3 to 10-fold improvement in the pion beta decay, π+ → π0e+ν(γ) measurement which determines |V_ud| in a theoretically pristine manner. This measurement would shed new lights on existing tensions in the CKM matrix unitarity.
PIONEER will use a combination of new detector technologies based on LGAD silicon tracking target, a deep, and high solid angle coverage LXe calorimeter featuring excellent energy and time resolution. I’ll discuss PIONEER’s detector concept and goals in light of previous experimental designs and achievements.
An update of the R&D associated with upgrading the SuperKEKB e+e− collider with polarized electron beams is presented. The Chiral Belle physics program enables a set of unique precision measurements using the Belle II detector. It includes a set of measurements of $\sin^2\theta_W$ via separate left-right asymmetry ($A_{LR}$) measurements in $e^+e^−$ annihilations to pairs of electrons, muons, taus, charm and b-quarks at 10GeV that yield a precision matching that of the LEP/SLC world average that uniquely probes the running of $\sin^2\theta_W$ with high precision. It will also provide the highest precision measurements of neutral current universality ratios, and precision measurements of tau lepton properties, including the tau g-2, as probes for new physics. After reviewing developments on the physics potential, this presentation will report on developments related to provision of the polarized source, the new components of the accelerator lattice that rotate the electron spin from transverse to longitudinal at the interaction point, and polarimetry of the electron beam.
After reviewing some key hints and puzzles from the early
universe, I will introduce recent joint work with Neil Turok
suggesting a rigid and predictive new approach to addressing them.
Our universe seems to be dominated by radiation at early times, and
positive vacuum energy at late times. Taking the symmetry and
analyticity properties of such a spacetime seriously leads to a new
formula for the gravitational entropy of our universe, and a picture
in which the Big Bang may be regarded as a kind of mirror.
I will explain how this line of thought suggests new explanations for
a number of observed properties of the universe, including: its
homogeneity, isotropy and flatness; the arrow of time (i.e. the fact
that entropy increases away from the bang); the nature of dark
matter (which, in this picture, is a right-handed neutrino, radiated
from the early universe like Hawking radiation from a black hole); the
origin of the primordial perturbations; and even the existence of
three generations of standard model fermions. I will discuss some
observational predictions that will be tested in the coming decade,
and some key open questions.
Van Roosbroeck’s equations constitute a versatile tool to determine the dynamics of electrons under time- and space-dependent perturbations. Extensively utilized in ordinary semiconductors, their potential to model devices made from topological materials remains untapped. In this talk, we will adapt van Roosbroeck’s equations to theoretically study the bulk response of a Weyl semimetal to an ultrafast and spatially localized light pulse in the presence of a quantizing magnetic field. We predict a transient oscillatory photovoltage that originates from the chiral anomaly. The oscillations take place at the plasma frequency (THz range) and are damped by intervalley scattering and dielectric relaxation. Our results illustrate the ability of van Roosbroeck’s equations to unveil the interplay between electronic band topology and ultrafast carrier dynamics in microelectronic devices.
A quantum computer attains computational advantage when outperforming the best classical computers running the best-known algorithms on well-defined tasks. We report quantum computational advantage using Borealis, a photonic processor offering dynamic programmability on all gates implemented. We carry out Gaussian boson sampling (GBS) on 216 squeezed modes entangled with three-dimensional connectivity, using a time-multiplexed and photon-number-resolving architecture. On average, it would take more than 9,000 years for the best available algorithms and supercomputers to produce, using exact methods, a single sample from the programmed distribution, whereas Borealis requires only 36 μs. This runtime advantage is over 50 million times as extreme as that reported from earlier photonic machines. Ours constitutes a very large GBS experiment, registering events with up to 219 photons and a mean photon number of 125. This work is a critical milestone on the path to a practical quantum computer, validating key technological features of photonics as a platform for this goal.
Tissue material properties can change drastically during embryonic development, reminiscent of rigidity transitions in physics. However, measuring the transitions or learning how to control the transitions is challenging experimentally. Theoretical and computational models provide new powerful tools to offer hypotheses on how to control the transitions. In this talk, I will introduce background on a commonly used tissue model, vertex models. I will highlight recent studies on the role of collective tissue mechanics in development and disease. I will then present our research on developing computational models to study the tissue material properties and their impact on cellular functions and coordination thereof.
Many physics research innovations have made their way to very successful commercial products that have transformed our day to day lives. In recent years more and more researchers are looking into the aspect of how their fundamental and/or applied research results can be commercialized. In this talk I will be presenting various phases related to the transition from research lab to industry, including the skill sets necessary for success in physics careers in industry and in commercialization of a product. I will be sharing some of the success stories of our Thin Films & Photonics Research Group (GCMP).
Mike has a Bachelor of Science degree from the University of New Brunswick. His post-graduate work focussed primarily on molecular physics and included both a Masters degree from the University of New Brunswick and a PhD from the University of Waterloo. After graduation, Mike’s career diversified working first in astro-physics while doing a post-doctoral fellowship at NASA’s Jet Propulsion Lab. Following this position, Mike moved into the field of nuclear physics in Chalk River Ontario with Bubble Technology Industries (BTI) as a research scientist. Mike joined the Green Imaging Technologies (GIT) in September 2015 as a Principal Research Scientist. Mike works closely with GIT’s research team innovating new NMR techniques and tools for our clients. In this talk, Mike will discuss how he ended up with such a diversified career in Physics, share some of the things he has learned from over 20 years experience working in physics research and development and talk some about his current work in NMR for the energy industry.
Chaired by Daniel Cluff
Patrick Reid, Moltex Clean Energy
Justin Furlotte, Fiddlehead Technology
Troy vom Braucke, GP Plasma
Jonathan Dysart, Horizon Health
Daniel Cluff, Deep Mining
Pandurang Ashrit, Universite de Moncton
Michael Dick, Green Imaging Technologies
Neutron beta decay is a fundamental nuclear process that provides a means
to perform precision measurements that test the limits of our present under-
standing of the weak interaction described by the Standard Model of particle
physics and puts constraints on physics beyond the Standard Model. The Nab
experiment will measure ‘a’, the electron-neutrino angular correlation parameter,
to a precision of δa/a ∼ 10−3 and ‘b’, the Fierz interference term, to a precision
of δb = 3 · 10−3. The Nab experiment implements large area segmented silicon
detectors to measure the proton momentum and the electron energy to reconstruct
a and b. The Nab silicon detectors were being characterized with protons and
electron sources prior to installation into the Nab experiment at the SNS at
ORNL. This talk will present an overview and status of the Nab experiment
and focus on preliminary measurements of the electronic response of the Nab
detector pixels and the reconstructed energies of the incident radiation using
proton and electron sources under various experimental conditions performed
at the University of Manitoba. The reconstructed proton energy was measured
while varying the detector temperature, the observed pixel location, the detec-
tor bias voltage, and the proton accelerating potential, respectively. The proton
rates in neighbouring detector pixels, during an incremental deflection of the
proton beam across the pixel boundary, were also measured.
In the past few years, the prospect of probing fundamental symmetries with radioactive molecules has generated significant interest in the field of low-energy, high-precision tests of the Standard Model of particle physics. Indeed, tailored molecules containing short-lived radioactive atoms are predicted to be especially sensitive to violations of fundamental symmetries such as a permanent electric dipole moment (EDM) of an electron, nuclear spin-dependent parity violation, or nuclear moments violating both parity (P) and time reversal symmetry (T).
In light of these intriguing physics opportunities, our RadMol collaboration aims to establish a new laboratory dedicated to fundamental physics research using radioactive molecules. Coupled to TRIUMF's radioactive ion beam facilities ISAC and ARIEL, this laboratory will strongly benefit from TRIUMF's unique capabilities in rare-isotope production, especially in its upcoming multi-beam operation. The initial science focus of RadMol will be on molecular electric dipole moments with unprecedented sensitivity to nuclear time-reversal breaking Schiff moments. This talk will present the experimental program of our new radioactive molecule laboratory at TRIUMF, including the most recent results from molecular beam development at TRIUMF.
Low-energy precision electro-weak physics tests are advocated as part of the search for physics beyond the Standard Model. We are working towards a measurement of atomic parity violation (APV) in francium (Z = 87), the heaviest alkali, in a magneto-optical trap (MOT) online to ISAC at TRIUMF. The transition of interest in Fr is between the 7S and 8S states, where the parity violating (PV) observable will be the interference between a parity-conserving “Stark-induced” E1 amplitude, created by applying a dc electric field to mix S and P states, and the vastly weaker PV amplitude. The presence of a M1 amplitude poses additional challenges as it also can interfere with the Stark-induced E1 and mimic a PV signal. Using a cavity with nearly 4000x power buildup, we observed the faint M1 transition, which is about 13 orders of magnitude weaker than an allowed E1 transition. To characterize it to higher precision, we are deploying a highly efficient detection scheme involving bursts of light from a cycling transition. I will report on these developments and review the M1 results obtained so far.
This work is supported by NSERC, NRC, University of Manitoba, and University of Maryland
ALPHA-g has completed a successful run in 2022 in the pursuit of measuring the gravitational mass of antihydrogen. This apparatus was designed to test whether antimatter follows Einstein’s Weak Equivalence Principle (WEP), where the acceleration due to gravity that a body experiences is independent of its structure or composition. A measurement of the gravitational mass of antimatter has never been done before, as previous experiments used charged particles, which meant the experiments were dominated by electromagnetic forces. The ALPHA-g apparatus uses electrically neutral antihydrogen atoms produced in a vertical Penning-Malmberg trap and trapped in a magnetic minimum trap. By measuring the antihydrogen annihilation positions after a controlled magnetic release of the atoms the gravitational mass of antihydrogen can be determined. Annihilation positions are reconstructed using a radial time projection chamber (rTPC) surrounding the trapping volume. To accurately determine vertical annihilation positions, precise detector calibrations are needed.
A laser calibration system was developed and used to gather drift time data in the rTPC, which results in vertical position information, and can be used to monitor changes in pressure, temperature, and magnetic field. In particular, we can calculate the Lorentz angle which is then used in reconstruction to accurately determine the annihilation positions. Simulations are also required to determine the expected drift time and Lorentz angle. Using Geant4 and Garfield++ toolkits, we can simulate these observables from electrons drifting through the gas portion of the ALPHA-g detector. In this talk I will discuss the laser calibration system for the rTPC and the results of the drift time and Lorentz angle data taken over the course of the 2022 run period. I will further discuss how these results are used in the reconstruction of antihydrogen annihilations by comparing with simulation, and how this calibration will be implemented in future ALPHA-g measurements.
Ultracold neutrons (UCNs) are a powerful tool for probing fundamental physics, enabling precision measurements in a variety of research areas, such as beta decay, electric dipole moments, and gravitational quantum states. To advance these experimental efforts it is necessary to develop new, high-density UCN sources capable of providing order-of-magnitude improvements in statistical sensitivity. The TRIUMF UltraCold Advanced Neutron (TUCAN) collaboration is building a new spallation-driven superthermal UCN source using superfluid helium, which will enable a new generation of UCN-based precision experiments. The performance of this source will depend on the storage lifetime of UCNs in the superfluid volume, which is expected to have a temperature-dependence given by $\tau^{-1} = BT^7$. In this talk, I will present the results of experimental efforts to measure this dependence using a prototype UCN source.
Motivated by fundamental symmetry tests, a non-zero measurement of a permanent electric dipole moment (EDM) would represent a clear signal of the violation of the CP symmetries. The imbalance in the matter and antimatter observed in our Universe is believed to arise from such violations, although the amount that is present in the Standard Model (SM) is insufficient. Many extensions to the SM predict EDMs much larger than the SM itself (<<$10^{-30}$ e cm) that could be within experimental reach. Experimentally, EMDs of nuclei in atoms or molecules are only accessible through the Schiff moment that measures the difference in the charge and dipole distributions. To relate the Schiff moment to the underlying EDM, a nuclear structure model must be used. To date, the upper limit of the EDM of $^{199}Hg$ remains as the most stringent.
In order to guide nuclear structure models required for the calculation of the Schiff moment of $^{199}Hg$, we have undertaken detailed inelastic scattering reactions of $^{198,200}Hg$ in order to map the distribution of both E2 and E3 in these nuclei since the Schiff moment is proportional to the product of the nuclear deformation parameters $\beta_2\beta_3$. Performing an experiment for $^{199}Hg$ is challenging, as such several experiments on $^{198,200}Hg$ were performed at the Maier-Leibnitz Laboratorium of the Ludwig-Maximilians Universität München. A 22 MeV deuteron beam bombarded the targets of the compound of $^{198,200}Hg^{32}S$, and the scattered particles that were separated using the quadruple three-dipole (Q3D) magnetic spectrograph. Very high-statistics data sets were collected from this reaction, resulting in the observation of a considerable number of new states. The cross section angular distributions are used to provide information on the spin and parities, and ultimately will be used to determine the excitation matrix elements.
Details of the analysis of the $^{198}Hg(d,d’)$ reaction to date will be given.
[1] T. E. Chupp, P. Fierlinger, M.J. Ramsey-Musolf, and J.T. Singh. Electric Dipole Moments of Atoms, Molecules, nuclei, and Particles. https://doi.org/10.1103/RevModPhys.91.015001, Jan 2019.
Over the last years, artificial neural networks have been explored as powerful and systematically tuneable ansatz to represent quantum wave functions. Such numerical models can tomographically reconstruct quantum states and operator expectation values from a finite amount of measurements. At the same time, artificial neural networks can find the ground state wave function of a given Hamiltonian via variational energy minimization.
While both approaches experience individual limitations, combining them leads to significant enhancements in the variational ground state search by naturally finding an improved network initialization from a limited amount of measurement data. Additional specific modifications of the network model and its implementation can further optimize the performance of variational simulations for quantum many-body systems, providing significant insights into their behaviour.
In this talk, I will discuss the representation of quantum states with artificial neural networks and demonstrate achievable enhancements by adapting network models, optimization procedures, and data generation processes.
Viewing neural quantum state tomography (NQST) as a flexible method for capturing classical snapshots of experimentally prepared quantum states opens doors to many applications of it in quantum simulation. In this talk we first review "Neural Error Mitigation" (Nat Mach Intell 4, 2022) for improving predictions of various observables obtained via quantum simulation of quantum states of interest in quantum chemistry and quantum electrodynamics. We then show that incorporating classical shadow tomography in NQST significantly improves its learning of complex quantum states, and numerically demonstrate this advantage through case studies in atomic and condensed-matter physics.
In the past couple of years, machine learning has permeated many areas of physics and found numerous applications in condensed matter and chemistry. In particular, we have witnessed remarkable progress toward developing computational methods using neural networks as variational estimators. Variational representations of quantum states abound and have successfully been used to guess ground-state properties of quantum many-body systems. Some are based on partial physical insight (Jastrow, Gutzwiller projected, and fractional quantum Hall states, for instance), and others operate as a black box that may contain information about the underlying structure of entanglement and correlations (tensor networks) and offer the advantage of a large set of variational parameters that can be efficiently optimized. However, using variational approaches to study excited states and, in particular, calculating the excitation spectrum, remains a challenge.
In this talk, I present two variational methods to calculate the dynamical properties and spectral functions of quantum many-body systems in the frequency domain: The first one consists of encoding the Green's function of the problem in the form of a neural network. We introduce a natural gradient descent approach to solve linear systems of equations and use Monte Carlo to obtain the dynamical correlation function. The second approach is based on a Chebyshev expansion of the spectral function and a neural network representation for the wave functions. The Chebyshev moments are obtained by recursively applying the Hamiltonian and projecting on the space of variational states. I will present results for the one-dimensional and two-dimensional Heisenberg model on the square lattice and compare to those obtained by other methods.
References:
1.“Chebyshev expansion of spectral functions using restricted Boltzmann machines”; D. Hendry, Hongwei Chen, Phillip Weinberg, A. E. Feiguin; Phys. Rev. B 104, 205130 (2021)
2.“A machine learning approach to dynamical properties of quantum many-body systems”; Douglas Hendry, Adrian E. Feiguin; Phys. Rev. B 100, 245123 (2019).
3.“Systematic improvement of neural network quantum states using a Lanczos recursion”; Hongwei Chen, Douglas Hendry, Phillip Weinberg, Adrian E. Feiguin; NeurIPS 2022 (Accepted). arXiv: 2206.14307
4.“Neural network representation for minimally entangled typical thermal states”; Douglas Hendry, Hongwei Chen, Adrian Feiguin. Phys. Rev. B 106, 165111 (2022).
SUPPORT: NSF Grant No. DMR-2120501
Pre-Recorded
The University of Waterloo's graduate program in Quantum Information has been delivered as a collaboration between the Institute for Quantum Computing (IQC) and seven departments since 2010. We will discuss the structure and success of the program, as well as recent additions including three Masters'-level laboratory courses and parallel programs for undergraduate students.
The University of Calgary has formed a strategic partnership with the Government of Alberta, and Mphasis, an information technology company, to establish Quantum City. One of the main goals of the Quantum City initiative is to create new talent development programs, to attract talent, researchers, and students to Calgary. In this spirit, the University of Calgary has launched the first-ever professional master’s in quantum computing: a 12-month program, with 8 months in class and a 4-month internship.
This unique graduate scholarship training program is hosted by the QMI and co-delivered by faculty at three BC universities (SFU, UBC and UVic) in collaboration with Quantum Computing industry partners. It integrates quantum hardware and software courses, hands-on workshops, professional development and a paid industrial internship.
We present progress towards an ultra-low phase noise microwave synthesizer, critical for achieving high-precision quantum gravimeters and gyroscopes based on cold-atom interferometry. The microwave synthesizer is used both for laser cooling ⁸⁷Rb atoms and inducing ground-state Raman transitions that function as momentum-transfer pulses in our atom interferometer. During these pulses, the phase of the Raman laser is directly imprinted on the atomic wavefunction. Thus, for high-precision quantum measurements, a very low noise is desired for the microwave signal phase that is transferred to the atoms. Our synthesizer design generates two independent microwave signals: one at 6.6 GHz that acts as a repump frequency for laser cooling, and one at 6.834 GHz in accordance with the ⁸⁷Rb ground state hyperfine splitting. Both of these signals are derived from an ultra-stable 100 MHz OXCO (ovenized crystal oscillator) and a PLDRO (phase-locked dielectric resonator oscillator) operating at 3.35 GHz. The two microwave signals are combined and sent to an electro-optic phase modulator to generate the desired optical frequencies in our 780 nm laser system. Preliminary measurements of the microwave power spectral density at 6.7 GHz yield a phase noise of −81 dB·rad²/Hz at an offset of 10 Hz. For a Mach-Zehnder-type atom interferometer with a free-fall time of T = 100 ms, we estimate a root-mean-squared phase noise of 4.8 mrad—corresponding to a sensitivity of 3×10⁻⁹ g per shot in a quantum gravimeter.
We demonstrate a method for stabilizing a diode laser using a frequency-offset locking scheme and commercial electronics. Our 1560 nm diode laser is slaved to an ultra-stable master laser operating at 780 nm by frequency-doubling the slave laser and measuring its optical beatnote with the master on a high-speed photodiode. This RF beatnote is fed through a broadband variable divider and a frequency-to-voltage converter with a high degree of linearity. An analog proportional-integrator circuit then uses the corresponding voltage signal to control the slave laser’s frequency with a tunable offset in the range of ~100 MHz to a few GHz. The main advantage of this method is its simplicity, versatility, and scalability. For example, minor modifications of the same architecture will enable us to realize an optical phase lock between two lasers. This locking system will be deployed on a laser-cooling experiment to realize a quantum gravimeter based on matter-wave interferometry.
Multi-frequency Raman generation (MRG) is a high order stimulated Raman process that can produce ultrashort laser pulses with high intensities. In experimental realizations of MRG, phenomena arise such as a single sideband shifted to a lower frequency on each of the Raman order peaks. These phenomena are not explained by previous theory. We derive analytic expressions for properties of MRG, such as the spectrum, to determine the processes leading to the experimental phenomena. These processes predict experimental changes to reduce or enhance the sidebands. Our theory makes use of the Dawson function and its many useful properties such as its equivalence to the Hilbert transform of a Gaussian function and its simple behaviour for very small and large values. This technique allows us to obtain analytic and perturbative results rather than the numerical results usually obtained in MRG theory.
The TRIUMF polarizer facility provides nuclear-spin-polarized radioactive isotopes via collinear optical pumping for physical and biomedical science$^{[1]}$. Recently, more exotic isotopes, such as $^{32}$Na and $^{230,232}$Ac, with production rates below ~1000 s$^{-1}$, are demanded to be highly spin-polarized to study nuclear structure and develop radiopharmaceuticals for cancer treatment. The traditional fluorescence detection method is insufficiently sensitive for measuring the hyperfine structures of these isotopes required to produce spin-polarized beams.
In this work, we try to develop a more sensitive detection mechanism compatible with our existing collinear geometry. The radioisotopes will undergo a two-step resonant ionization, first to an excited state and then to a high-energy Rydberg state, and subsequently be ionized by an intense electric field. Using charge particle detection instead of photon detection will significantly improve detection efficiency. Here we compare several different approaches to ionizer designs$^{[2, 3]}$: a homogeneous set of electrodes that surround the atomic beam, and a heterogeneous mix of electrodes and meshes of wire grids. All designs aim to achieve low energy spread and high detection selectivity by providing an energy signature to produced ions that distinguish them from background ions.
We simulated these designs and compared the potentials and fields that the beam would experience. The plots we generated confirmed that the mesh-based design had significantly smaller radial variations in potential and field. Numerical calculations showed that the spread in electric potential on and off-axis was two-to-three orders of magnitude lower than for the other designs. Moving forward, we will build the mesh-based geometry and test its efficiency compared to the other designs, eventually deploying the best geometry in experiments to determine the hyperfine spectra of critical low-production isotopes.
[1] C. D. P. Levy et al., “A polarized beams project at ISAC”, Nuclear Physics A 701, 253c-258c (2002).
[2] K. Stratmann et al., “High-resolution field ionizer for state-selective detection of Rydberg atoms in fast-beam laser spectroscopy’, Rev. Sci. Instrum. 65, 1847–1852 (1994).
[3] A. R. Vernon et al., “Laser spectroscopy of indium Rydberg atom bunches by electric field ionization”, Sci. Rep. 10, 12306 (2020).
Nonlinear laser fiber amplification is a powerful technique known for generating high-energy, ultrashort pulses efficiently and compactly, finding applications in various fields. In this study, our objective is to develop and optimize a two-color nonlinear amplification system, which will serve as a crucial component for future multi-frequency Raman generation (MRG) experiments. The traditional two-color chirped pulse amplification (CPA) method has limitations such as gain narrowing and compressibility. To overcome these drawbacks, we focus on the construction of a two-color laser system using nonlinear amplification techniques. Initially, a single-color broad spectrum is generated using a gain-managed nonlinear amplifier (GMNA). By selectively removing the central portion of the spectrum through the implementation of notch filters, a two-color configuration is created. This modified spectrum is then employed as a seed for a nonlinear amplifier, where self-phase modulation (SPM) is utilized to broaden the spectral content of each color while maintaining high-quality pulses. The resulting pulses can be easily compressed through a simple grating compressor. The optimization process involves carefully selecting parameters such as fiber length, pump power and direction, and the size and placement of the center notch colors to control the extent of spectral broadening. Simulations based on the gain-rate equation will be conducted to study the performance of the system, which will be subsequently validated through experimental verification. By developing this two-color nonlinear amplification system, we aim to overcome the limitations of traditional two-color CPA methods and provide a suitable platform for future MRG experiments.
We present our progress towards developing a trapped ion quantum information processor and describe our robust hardware and software architecture. Our platform for storing and processing quantum information is trapped Barium ions. Because of long-lived ground and metastable atomic states and transitions in the visible wavelengths, Ba$^+$ offers exciting possibilities to encode quantum information in flexible ways and to employ low-loss, waveguide-based optical engineering for high-precision and programmable controls. We discuss our progress towards high efficiency isotope-selective loading of ions, especially $^{133}$Ba$^+$ that is radioactive (t$_{1/2}$=10.6 years) and hence can only be used in miniscule quantities, in a surface electrode trap. Furthermore, we remark on generating long chains of Barium ions, cooling them, and individually addressing them by a waveguide based optical addressing system with ultra-low (<1E-4) relative intensity crosstalk for precise and programmable control for individual Ba$^+$ qubits. In the long run, we expect the processor to be an open-access system for academic use.
We acknowledge CFREF, University of Waterloo, NSERC, and Canada Research Chairs program for funding.
We investigate the transport properties of charge carrier disordered organic
semiconductors with a focus on the determination and analysis of charge carrier
mobility. By understanding that charge transport is due to incoherent hopping of
charge carriers across localized states, we use a model that relates mobility to charge
carrier (not small polarons) hopping by thermal activation. We consider the
Miller–Abrahams expression to describe the hopping rate of charge carriers and
employ kinetic Monte Carlo simulation methods to generate data from which we can
analyze charge carrier mobility as a function of applied electric field, temperature,
localization length, and spatial and energetic disorder parameters. Based on our
results, we discuss the effects of these parameters on charge carrier mobility. Our
results show the importance of the spatial disorder parameter and localization
length in the effects of electric field dependence on charge carrier mobility, and we
also evaluate the value of localization length that has been mostly considered as
0.1b, where b is the lattice parameter.
This study focused on investigating whether ball milling and cold rolling can improve the hydrogen absorption and desorption kinetics of magnesium hydride (MgH2) and reduce its process temperature. Despite having a high hydrogen storage capacity, good reversibility, and low cost, MgH2 has not been widely used due to its high temperature of operation and slow rate of hydrogen absorption and desorption. Four forms of MgH2 were investigated, including unprocessed, ball milled for 15 and 20 minutes, and cold-rolled 5 times. The experiments aimed to identify the temperature at which the MgH2 forms absorb and desorb within a temperature range of 25 to 450 degrees Celsius. Results showed that both ball milling and cold rolling improved the hydrogen absorption and desorption kinetics of MgH2 and lowered the required process temperature. Cold rolling was found to be more effective than ball milling in improving MgH2's storage capacity and had a greater impact on hydrogen absorption and desorption kinetics. The study concludes that ball milling and cold rolling have the potential to improve hydrogen storage performance, with further optimization depending on the specific application and desired characteristics.
In electron-doped Strontium Titanate (SrTiO3), ferroelectricity can coexist simultaneously with metallicity. Absent any electrons, the ferroelectric domains will orient themselves into the so-called “Kittel Domains” in order to minimize their free energy. The impact of free electrons on their behaviour remains under active investigation with research suggesting that electron density plays a role in the orientation of the domain walls (e.g. tilt relative to the normal of a thin-film surface). We model a thin-film ferroelectric metal through a self-consistent Landau-Ginzburg-Devonshire free energy, and electron-phonon Hamiltonian. In particular, we consider the coupling of the t2g orbitals with the polarization and their gradients under cubic symmetry, and contrast the behaviour with an uncoupled free electron gas. We are particularly interested in the impact of the electrons on the formation and behaviour of domain walls, and whether they can be tuned to achieve desirable electronic properties (e.g. conductive surfaces or wires) through manipulable characteristics of the material (e.g. film width, external potential, electron density).
We present the results of an extensive study of the phase diagram and spin wave excitations for a general spin model on a hexagonal AB-stacked kagome lattice. Depending on the strength of the spin-orbit coupling (SOC), some spin and lattice rotations may become decoupled, leading to considerably larger symmetry groups than typical magnetic groups. Thus, we provide a detailed symmetry description of the magnetic Hamiltonian in the limit of negligible, weak, and intermediate strength of SOC. The spin symmetry in these three cases has a strong effect on the splittings observed in the spin excitation spectra and is therefore relevant to the interpretations of future experimental studies. We further identify a large number of self-duality transformations that map the Hamiltonian onto itself. These transformations describe the symmetry of the parameter space and provide exact mappings between the properties of different magnetic orders. Finally, we discuss the physical relevance of our findings in the context of Mn$_3X$ compounds.
We synthesized a green-fluorescent conjugated polymer (CP) referred to as “Atums Green”. This organic-soluble polymer had a molecular weight up to 50 kDa and featured a strong green fluorescence both in solution and in the solid state. Photophysical studies were done to explore its application in laser photonics in the green band. The PL emission has an absolute quantum efficiency as high as 98% and the time-resolved photoluminescence showed a mainly single exponential decay with a time constant of 0.74 ns, whereas in solid films the mean decay times were non-exponential and on the order of 250 ps. Atums Green moreover demonstrated superluminescence and solution-based lasing in a bulk cavity tunable between 500 and 540 nm with pump energies up to 60 μJ for pump pulses of ≈1.8 mJ. Injecting Atums Green into a microcapillary generated a set of whispering gallery lasing modes separated by 1.08 nm. The lasing output was confirmed by threshold measurements and from interference using a spatial light modulator. Solid state lasing was currently prevented due to photobleaching effects that occurred under atmosphere. We finally used Atums Green as the green component of a set of blended 3-color CP microspheres. Atums Green was mixed in various proportions with red-emitting MEH-PPV and blue-emitting MEH-PPP and then both solvent-emulsification and microfluidic methods were used to generate a set of bright fluorescent microspheres whose emission covered a wide gamut of the perceived color spectrum.
When a Brownian particle moves too rapidly for the medium to effectively absorb its kinetic energy, the standard Einstein theory of diffusion with a constant viscous friction becomes invalidated. A natural description of this kind of Brownian dynamics is to take the friction as a decreasing even function of the particle's velocity. The stochastic equation of motion is formulated within this approach, in which a broad class of physically relevant functions describing the velocity-dependent friction is considered. An analytical formula for the diffusion coefficient $D$ is derived. It is shown that $D$ as a function of temperature $T$ may exhibit only three scaling types: (i) $D \propto T$, corresponding to the standard Einstein relation with velocity-independent friction; (ii) $D \propto T^{\alpha + 1}$, corresponding to a power-law decrease of the friction coefficient with the velocity of the particle, $\gamma(v) \propto 1/v^{2\alpha}$ at high $v$; (iii) $D \propto 1/\sqrt{T - T_c}$, corresponding to a Gaussian relation between friction coefficient and velocity.
London dispersion is a weak, attractive, intermolecular force that occurs due to interactions between instantaneous dipole moments. While individual dispersion contributions are small, they are the dominating attractive force between non-polar species and determine many properties of interest. Standard methods in density-functional theory do not account for dispersion contributions, so a correction such as the exchange-hole dipole moment (XDM) or many-body dispersion (MBD) models must be added. Recent literature has discussed the importance of many-body effects on dispersion, and attention has turned to which methods accurately capture them. By studying systems of interacting quantum harmonic oscillators from first principles, we directly compare computed dispersion coefficients and energies from XDM and MBD. While the results are similar at large separations, MBD is found to be susceptible to a polarization catastrophe at short range. Additionally, the self-consistent screening formalism used in MBD is shown to be surprisingly sensitive to the choice of input polarizabilities. Connection is made to interactions between noble gas atoms, as well as to the methane and benzene dimers, and to two layered materials, graphite and MoS2, for which similar results to the oscillator models were obtained.
The fourth-generation synchrotron radiation light source has the outstanding advantages such as low divergence and high brightness, facilitating high spatial and energy resolution X-ray spectroscopy studies and the detection of “light-in-light-out” photon-hungry spectroscopy. The proposed high-resolution soft X-ray spectroscopy beamlines of Shenzhen Industrial Light Source (SILF) will set up multi-functional experimental platforms such as ARPES, Nano-ARPES, PEEM, RIXS, XAS, XMCD, STXM and APXPS.
The unique structure of two-dimensional (2D) Dirac crystals, with electronic bands linear in the proximity of the Brillouin-zone boundary and the Fermi energy, creates anomalous situations where small Fermi-energy perturbations critically affect the electron-related lattice properties of these systems.[1] We have studied the interaction of these electrons with acoustic phonons, where the phonon frequency is also linear in their wavenumber. We show that in these systems considering higher-order electron-phonon interaction terms is essential to understand many critical crystal properties, including the dielectric function and the thermal conductivity, which we will present as a function of temperature in the special case of graphene.
[1] Kazemian and Fanchini, J. Phys.: Condens. Matter 35 325601 (2023)
Solar-like stars oscillate as a result of sound and gravity waves that propagate through the sphere; the waves allow us to then probe the stellar interior for information on its physical properties. These stars will evolve off the main sequence to the red giant branch (RBG) and subsequently either to the red clump or secondary red clump stages depending on their mass. Additionally, some solar-like stars, that we have yet to understand, have low-amplitude (ℓ=1) oscillation modes, dubbed “depressed” stars. Asteroseismology allows us to disentangle the classifications of these stellar evolutionary stages as red giant star populations, on the Hertzsprung-Russell diagram, tend to overlap between these regions. With the amount of currently available data, it is necessary to automate the classification process. Using a machine learning-based method, I worked to automate this disentanglement by using seismic data from stellar oscillations, since oscillatory patterns are characteristic of stellar age, to further sort these stars according to their evolutionary history. In this research, I have performed the classification of about 18,000 evolved stars, observed during the Kepler mission, based on their oscillation patterns; this is the largest sample of red giants that has been classified automatically and will allow for better studying of the interior dynamics of evolving solar-like stars.
This report presents a review of the Touschek lifetime in fourth-generation accelerator machines. Specifically, the report focuses on the Møller scattering differential cross section and the loss rate of electrons within a bunch of electrons defined by longitudinal potential wells.
When electrons in a bunch move towards each other, they can interact and scatter away due to Møller scattering. Electron-electron interactions transfer momentum from the transverse plane into the longitudinal direction. If the exchanged momentum exceeds the acceptance momentum exchange threshold in the longitudinal direction, the electrons may either be left behind or pushed out of the bunch. Beam loss due to Møller scattering is a dominant effect in damping rings, ultra-low emittance storage rings.
The energy-dependent effect of Møller scattering in accelerator machines was first observed by Bruno Touschek and his colleagues in 1963. However, the observed effect was inconsistent with the asymptotic solutions at the time. To maximize the beam lifetime, it is preferable to tune the accelerator machine to have a Touschek effect dominant beam lifetime. By studying the longitudinal and transverse motions, one can calculate the Touschek effect contribution to the beam's lifetime and even decrease the scattering rate.
Overall, this report highlights the importance of understanding Møller scattering and the Touschek lifetime in fourth-generation accelerator machines and the experimental methods to increase the beam's life time in fourth generation light sources.
The aim of this research project is to evaluate the functionality of our instruments for performing non-linear elastic measurements and establish best practices for transient-wave dynamic acousto-elastic testing (TW-DAET). TW-DAET employs a pump and probe configuration. We perturb a sample with a low-frequency pulse (50 kHz pump), then probe the system with a high-frequency pulse (300-1000 kHz probe) to measure the non-linear effects induced by the perturbation. We focus on ultrasonic transducers and elastic wave propagation in inhomogeneous materials. This work was inspired by previous studies in geophysics, and its applications span several disciplines, such as medical physics and material science.
Previous work investigated whether the frequency of the perturbation pulse is related to the magnitude of the induced non-linear response. This work was inconclusive because the elastic wave frequency before and after propagating through the material was inconsistent. This unexpected result led us to two hypotheses: (1) the examined material possesses the capacity for frequency conversion, or (2) flaws in the experimental setup led to misleading results. To investigate these hypotheses, we conducted control experiments to establish the capabilities and limitations of our instruments. Before examining frequency conversion, it was essential to establish our setup's ability to generate and measure desired frequencies in the range of 50 kHz to 1 MHz. Using ultrasonic transducers to trigger wave propagation in various solid materials, we develop best practices and optimal operating parameters when coupling media to new samples.
The significance of this research lies in the understanding of how ultrasonic transducers couple with different materials and how this may affect non-linear elastic measurements. Although the motivation for this research lies in non-linear elasticity, these understandings apply to a diverse variety of fields. This contribution to the field of physics and instrumentation will lead to improved protocols for non-linear elastic data collection, ultimately enhancing our ability to measure and understand elastic wave propagation.
Quantum dots (QDs) are solids confined at the nanoscale in all directions, which often enables them to exhibit photoluminescence (PL) even if their long-range crystalline counterparts do not. QD-PL is essential to explain the different roles of confinement in these nano-objects. To gain insight into the luminescence of individual QDs, optical probes potentially capable of resolving the emission signal from individual nano-objects are required, which avoids the effect of radiative energy transfer between neighboring QDs, or to the environment. To this end, we developed a hyperspectral scanning near-field optical microscopy (SNOM) PL imaging system. SNOM utilizes evanescent radiation to generate optical excitation and/or capture luminescence signals at lateral resolution beyond the diffraction limit that restricts the optical resolution of plane-wave propagating radiation. Our hyperspectral imaging apparatus was tested on calcium-zinc oxide luminescent QDs embedded in commercial scotch tape to make it fluorescent. Investigation of this scotch tape including Rutherford backscattering, scanning electron microscopy, and energy dispersive x-ray spectroscopy, were performed to determine the tape morphology and composition which was found to be (Ca0.95Zn0.05O):(C8H10O)20 consistent with literature reports of CaZnO QDs embedded in a polymer matrix (i.e., the tape itself). Using our scanning hyperspectral system, PL spectra from the tape were recorded using 405-nm excitation on a 10x10 um area at 200 nm pixel size, and the PL emission peak was found at 560±10 nm, which is significantly different from the 590–620 nm range expected from “macroscopic” PL measurements. The observed PL emission wavelengths are in line with the results from CaZnO as reported in the literature. With a deeper understanding of the root causes of the differences between nanoscale and “macroscopic” PL measurements, our hyperspectral tool will invaluably further our knowledge on the relationship between quantum and dielectric confinements as a function of QD diameter, distribution, and luminescence intensity.
De nombreuses technologies d'ultra-haute précisions sont limitées par un phénomène fondamental : les fluctuations associées à la dissipation mécanique dans les matériaux amorphes. Ceux-ci sont présents dans les couches isolantes des dispositifs supraconducteurs et dans les miroirs diélectriques des cavités optiques quantiques, d’horloges atomiques, et des détecteurs d’ondes gravitationnelles. Dans ce dernier contexte, notre groupe participe à la recherche sur le développement de matériaux présentant le meilleur compromis entre contraste d’indice de réfraction, faible absorbance et faible dissipation mécanique interne. En effet, depuis la première détection de fusion de trous noirs en 2015, les observatoires d'ondes gravitationnelles ouvrent une nouvelle fenêtre sur le fonctionnement de l'Univers. Plus d'une centaine d'événements de fusion d'objets compacts ont été identifiés, à un taux d'environ un par semaine. Mais leur sensibilité dans leur domaine de fréquence le plus élevé reste limitée par le phénomène décrit plus haut.
Nous tentons différentes approches : variation des paramètres de dépôt, dopage, changements de composition, autres stratégies de fabrication. La modélisation nous permet en outre de comprendre les mécanismes à l’origine de la dissipation et donc des fluctuations. Un point commun qui se dégage de ces travaux est que les matériaux amorphes qui présentent le moins de dissipation mécanique sont ceux qui sont les mieux relaxés et dont la configuration à courte et moyenne portée ressemble le plus à la structure de leur correspondant cristallin.
The physics of strongly interacting fermionic systems is an interesting topic in nuclear physics. The Hubbard model is one of the simplest yet insightful models that we use to study the strongly interacting fermions. We perform benchmark calculations of ground state energies for the repulsive and attractive Hubbard model using the Auxilary Field Quantum Monte Carlo method, and further tune the model to study the universal properties at the unitary limit. Evidence from ultracold atom experiments is another source that provides feedback to understand the strongly interacting fermion systems that are physically present on Earth. One of our key goals is to map the lattice model to correctly describe the properties of ultracold atoms at the thermodynamic limit so that we can predict the physics of neutron matter such as (extraterrestrial) neutron stars.
The presumption of magic numbers and nuclear shell closures is a fundamental paradigm of our understanding of atomic nuclei. However, far away from the valley of stability, expected properties within these well-established shell closures can significantly differ. A prime example for this so-called shell evolution is the island of inversion around neutron-rich magnesium and sodium isotopes (N=20) [1]. Experimental studies of isotopes in these exotic regions of the nuclide chart are however often challenged by low production yields and short half-lives.
The Multi-Ion Reflection Apparatus for Collinear Laser Spectroscopy (MIRACLS) [2] is a novel experimental technique in which high-resolution collinear laser spectroscopy (CLS) is performed in a multiple-reflection time-of-flight (MR-ToF) device. By trapping and revolving ions multiple thousands of times in an optical detection region (ODR), experimental sensitivity can be significantly improved when compared to conventional, single-passage CLS. This gain in sensitivity allows for the study of radioisotopes in more exotic regions of the nuclear chart.
In order to maximize the gain obtained from this new apparatus, the MIRACLS MR-ToF device requires cooled ion bunches with stringent emittance requirements. To address these needs, a preparation Paul trap was designed, constructed, and commissioned. In this presentation, we will describe the current status of the MIRACLS experiment with an emphasis on its newly commissioned Paul trap. A description of the goals of MIRACLS and its experimental setup will be provided, including the recent commissioning of the Paul trap.
[1] E. K. Warburton, J. A. Becker, and B. A. Brown, Phys. Rev. C 41, 1147 (1990)
[2] S. Sels et al., Nucl. Inst. Meth. Phys. Res. Sec. B, 463, 310–314 (2020)
V. Lagaki et al., Nucl. Inst. Meth. Phys. Res. Sec. A, 165663 (2021)
F. Maier et al., Nucl. Inst. Meth. Phys. Res. Sec. A, 167927 (2023)
Complex plasmas are made of micrometer-sized particles immersed in a weakly ionized gas. Due to their interactions with the surrounding ions and electrons, the microparticles usually acquire negative charges of the order of several thousand elementary charges. Due to microparticles interactions, complex plasmas can form gaseous, liquid and crystalline states. For this reason, they are often used as model systems for soft matter. Thanks to their large size, a direct optical observation of individual particles is possible and enables the study of their dynamics at the kinetic level even in systems where the number of particles is large. In ground-based experiments, gravity is the dominant force restricting the research to vertically compressed, inhomogeneous microparticle clouds, or (quasi) two-dimensional systems, and masking dynamical processes mediated by weaker forces. Under reduced gravity conditions, such as provided on the International Space Station (ISS), this limitations are overcome allowing the study of processes otherwise mask by gravity. In this poster, the research goals for the next generation complex plasma facility COMPACT to be operated onboard the ISS are presented. COMPACT is envisaged as an international multi-purpose and multi-user facility that gives access to the full three-dimensional kinetic properties of the particles.
Reliable measurements of plasma parameters are a good way to confirm if the plasma dynamics fit well with our theoretical models as well as giving insight into the plasma's state. The ion temperature in the plasma cannot be measured from a typical Langmuir probe which makes it hard to estimate. To do so, it is possible to use a Ball-Pen probe (BPP) which has the ability to partially shield electrons thereby reducing the electron flux. By applying a varying voltage on the Ball-Pen probe, a symmetrical I-V curve can be obtained, allowing measurement of the ion temperature by curve fitting the exponential trend due to ionic thermal motion near the electron saturation region of the I-V curve. Other parameters such as the electron temperature, the electron density, the floating potential, and the plasma potential measured by the Ball-Pen probe in the STOR-M tokamak are compared with those obtained from a single Langmuir probe and a triple probe which are already established diagnostics in the STOR-M. It was found that the ion temperature in the plasma edge of the STOR-M is 7±3 eV, which is range comparable to what has been reported previously. More efforts would be needed to further validate ion temperature measurements in the STOR-M. Solutions include increasing the sweeping frequency of the power supply for better statistics as well as improving the mechanical setup of the probe.
NV centers in a diamond crystal consist of a substitutional nitrogen atom next to a lattice vacancy. These commonly appear in two distinct charge states, the neutral NV center (NV${^o}$) and the negatively charged NV center (NV${^-}$). While the more commonly formed state is the NV${^o}$ , the NV${^-}$ center has S = 1 fine structure that has important magnetic field dependent fluorescence properties due to its trapped electron. Fluorescence of the NV${^-}$ center has many applications include bio-labelling, thermometry, magnetometry, and quantum information, among many others. Research to improve the uniformity and replicability of manufactured NV${^-}$ center-containing films is of great importance. Microwave plasma assisted chemical vapor deposition (MPCVD) of diamond with \emph{in situ} nitrogen doping has shown promise in the synthesis of these heteroepitaxially grown centers[1]. Currently the effect of different nitrogen doping times on the growth of NV${^-}$ centers is not well understood.
This poster will present the results of an investigation of varying N${_2}$ doping times during diamond synthesis and how this affects the growth of both NV${^o}$ and NV${^-}$ centers within polycrystalline MPCVD diamond films. Investigation with Raman spectroscopy, photo luminescence spectroscopy and X-ray diffraction were carried out. By increasing or decreasing the N${_2}$ doping time and studying the variation of the intensity of the 637 nm NV${^-}$ photoluminescence (PL) spectral line, we derive a relationship between doping time and density of NV${^-}$ centers.
[1] Ejalonibu, H. A., Sarty, G. E., Bradley, M. P. (2019, April 25). "Optimal parameter(s) for the synthesis of nitrogen-vacancy (NV) centres in polycrystalline diamonds at low pressure" - \emph{Journal of Materials Science: Materials in Electronics.} SpringerLink. https://link.springer.com/article/10.1007/s10854-019-01376-z
Abstract:
The main goal of this research is to obtain a clear and accurate model of the late-time behavior of a quantum-corrected black hole’s radiative emission wave. Specifically, the focus is on late-time tail waveforms, which appear after the exponentially damped signal originating from the ring down phase of a perturbed black hole. This project focused on interpreting the effects of loop quantum corrections on black hole quasi-normal modes and radiative tails. We began with the scalar wave equation and solved for the Regge-Wheeler scalar field potential, which captures the physics of a standard Schwarzschild black hole. This solution allowed us to generate waveforms with different initial variables, such as multipole numbers and radial epsilon exponents. Next, we analyzed the divergent characteristics, oscillatory behavior, and decay rates of the late-time tails for the quantum-corrected black hole and performed a comparison with the Schwarzschild case. This research is part of an ongoing project on gravitational wave emission from quantum-corrected black holes, and how they can be modeled. It is a bid to make detection and recognition of such waveforms possible in future gravitational wave observatories.
Bell's inequalities provide a practical method for testing whether correlations observed between spatially separated parts of a system are compatible with any local hidden variable description. For $2-$ qubit pure states, entanglement and nonlocality as measured by Bell inequality violations are directly related. However, for multiqubit pure states, the much more complex relation between N-qubit entanglement and nonlocality has not yet been explored in much detail. In this work, we analyze the violation of the Svetlichny-Bell inequality by N-qubit generalized GHZ (GGHZ) states, and identify members of this family of states that do not violate the inequality. GGHZ states are a generalization of the well known GHZ state, which is a useful entanglement resource. GGHZ are hence natural candidates to explore for extending various quantum information protocols, like controlled quantum teleportation, to more than three parties. Our results raise interesting questions regarding characterization of genuine multipartite correlations using Bell-type inequalities.
Originally the subject of Star Wars science-fiction, astronomers have discovered planets orbiting twin suns, just like on the fictional planet Tatooine appearing in Star Wars Episode IV: A New Hope. More commonly known as circumbinary planets, these systems are ones in which the planet is in orbit around both binary stars. In these gaseous bodies, tidal forces induce interior gaseous mixing of the stars, of which facilitates an energy transfer that dissipates orbital energy. This orbital energy dissipation results in a decrease of both the binary semi-major axis, ab, and the binary eccentricity, eb. My work focuses on this stage of binary evolution, namely, the tidal circularization (reduced semi-major axis, ab) and migration (reduced eccentricity, eb) of binary stars and the significance of the affects of this stellar evolution on the planetary stability in these circumbinary or “Tatooine” systems. Previous works have not explained how the binary’s tidal migration and circularization affects the stability of the circumbinary planets, as they only considered the gravitational force. Because no circumbinary planets have been detected around binaries with orbital periods less than 7 days (Martin 2018), where tidal circularization is expected to be very efficient (e.g. Zanazzi, 2021), my study will shed light on the deficit of circumbinary planets orbiting short period binaries.
It is known that Schwarzchild geometry exhibits thermodynamic properties and these have a statistical mechanics explanation. An interesting question to ask is if we can study the statistical mechanics of spins on this background. In this presentation we will answer this question in the positive and construct an Ising-like model on black hole space. Then we will numerically study the thermodynamic properties of spins (such as alignment and entropy) for different masses of the black hole and discuss the resultant second order phase transition.
The Light-only Liquid Xenon (LoLX) experiment is designed to study the properties of light emission and transport in liquid xenon (LXe) using silicon photomultipliers (SiPMs). A particular focus of LoLX is to measure and study Cherenkov and scintillation light emission in LXe. LoLX is currently being upgraded to investigate the long-term behaviour and performance of Hamamatsu VUV4 and FBK VUV-HD3 SiPMs. Both models are currently being considered for application in the neutrinoless double beta decay experiment nEXO.
A proposed method to monitor the long-term stability and performance of the aforementioned SiPMs in LXe is to augment the xenon with radioactive $^{127}$Xe (an electron capture source with a half-life of 36.3 days and a Q-value of 662.3 keV). This allows for an $\textit{in-situ}$ calibration and performance characterization while the detector is operational. This poster will introduce the concept and focus on the neutron activation estimates of $^{127}$Xe from $^{\text{nat}}$Xe, as well as the methodology for deploying it in LoLX.
Using quantum field theory, we calculate the total effect on the photon flux in the microwave background due to some photons being gravitationally scattered toward us and others being gravitationally scattered away from us. The scattering is produced by the density fluctuations which act like point masses in a FLRW background, which can be of either sign. The net effect of having masses of either sign is to give a Debye screening of the graviton.
The study of muons is very important as they are at the center of several current discrepancies between the experiments and the theoretical predictions, such as the measurement of anomalous magnetic moment and rare decays of B-meson that involve muons. The best limits set in the charged lepton flavour violation are by the muon sector experiments. This is the time to focus on the experiments that involve muons as they can reveal new secrets. Our work is motivated by two large experiments under preparation, Mu2e and COMET, that will search for the very rare muon-electron conversion near a nucleus N, which is a beyond SM process. I am evaluating the bound muon lifetime for a range of nuclei including aluminum, which will be used as the target material in these experiments. I will also check the existing literature in preparation for the two important experiments.
Dark matter annihilation(DMA) provide an promising avenue to detect dark matter particles. Meanwhile, 21-cm line of hydrogen during cosmic dawn have great potential to reveal the information about the early galaxies and stellar formation process.
In this presentation, we elucidate the study using semi-analytic method to model the dark matter annihilation from global background and structure haloes at redshift $𝑧\sim 20−40$. Our findings reveal that dark matter annihilation inhibits gas collapse in mini halos. By considering other possible effects such as streaming velocity and feedback mechanism. We obtain a more comprehensive result and we subsequently compare with previous results.
Our result suggest that DMA has the ability to significantly alter the observable brightness temperature of 21-cm hydrogen line, and may even affect the early universe's star formation history. This work sheds light on the importance of taking into account the impact of DMA when interpreting the 21cm signal.
The NEWS-G experiment is a dark matter experiment based on gaseous detectors, located at SNO lab. The experiment aims to detect WIMPs by measuring nuclear recoils in noble gases using a spherical proportional counter (SPC) detector, which offers high sensitivity due to its unprecedented low energy threshold. Accurate measurement of the recoil energy requires knowledge of the quenching factor (QF), which quantifies the reduction of ionization due to nuclear recoils compared to electromagnetic interactions. We have already conducted quenching factor (QF) measurements at TUNL using a mixture of Ne + CH4 gas at 2 bar. As part of our future plans, we intend to measure the QF using various gas mixtures and different detector parameters. To facilitate these in-beam QF measurements, we recently carried out a tabletop experiment at Queen's University to study SPC detector characteristics for different detector parameters. Plan for another campaign at TUNL for QF measurement is ongoing and a possibility of conducting such an experiment at UdeM is also underway.
In this poster, the highlights of the tabletop experiment will be presented. In addition, the past measurement, current status, and the future plans of the NEWS-G collaboration in measuring QF with SPC will be summarized.
NEWS-G is an experiment searching for dark matter using the Spherical Proportional Counter (SPC) technique. Such detectors can operate significant mass of target, of order of kgs with meter size spheres, while keeping single ionization electron detection sensitivity. They can be filled with gaseous targets of low atomic mass such as hydrogen, helium, and neon, giving sensitivity to low mass WIMPs down to (0.1GeV).
The poster will show the principle of operations of the SPC and a description of the 140cm diameter detector and compact shielding, installed in the SNOLAB underground facility. It will address the challenges of building such a facility underground, with low radioactivity materials.
The poster will also introduce projects to improve the SPC performance, and expand their reach to coherent elastic neutrino-nucleus scattering (CEvNS)
The use of laser-polarized Xenon-129 exponential ($^{129}$Xe) as a novel contrast agent for MRI has been shown to be effective for functional (1,2) and structural imaging the brain (3) and other organs(4). It was approved by the FDA in December 2022. $^{129}$Xe-based imaging could transform our methods of mapping grey and white matter,(5) perfusion,(3) by improving sensitivity over other MRI methods and reaching beyond the resolution limitations of PET.
To develop this program, two birdcage radiofrequency (RF) coils for the use of simultaneous hyperpolarized $^{129}$Xe MRI and $^{15}$O2 PET imaging for brain perfusion measurements were developed. Birdcage RF coils have been widely used in MRI as their RF homogeneity and SNR exceed that of common linear RF coils.
Two coils were designed for optimal use with a Siemens 3T PET/MRI scanner, one using a low-pass-filter-design, and the other a high-pass-filter-design.
Both high-pass and low-pass coils were tuned to 34.05MHz (inside the PET-insert), with 8 rungs on each coil. The equivalent rung capacitance was calculated using Birdcage Builder software (Penn State, USA), with 242pF rung capacitance for the low-pass-coil and 1275pF rung capacitance for the high-pass-coil. The coil was built to 75mm in length, with a diameter of 45mm.
The low-pass-circuit had a sensitivity of -19.8dB/-27.6dB. The high-pass-circuit had a sensitivity of -22.7dB/29.3dB. Initial phantom scans indicated that both coils have demonstrated good sensitivity, and therefore they can be used in the simultaneous in-vivo [$^{15}$O2] PET and hyperpolarized $^{129}$Xe MRI brain perfusion imaging measurement. To further optimize the sensitivity of both coils, in-vivo PET/MRI measurements will be used.
We were able to build two rat-head-sized $^{129}$Xe RF coils fitting into the animal-sized PET-insert resonating at the $^{129}$Xe resonance frequency at the 3T MRI system. Initial phantom scans indicated that both coils have demonstrated good sensitivity, and therefore they can be used in the simultaneous in-vivo [$^{15}$O2] PET and hyperpolarized $^{129}$Xe MRI brain perfusion imaging measurement.
Screening for breast cancer and disease is a routine and common practice among woman. Early detection of cancerous tumours has been shown to greatly reduce mortality. Commonly screening is performed using two-dimensional ultrasound, or mammographic imaging. A smaller dense breast is difficult to image on a mammogram system, and is more likely to be ultrasonically probed. Moreover, standard 2D ultrasound suffers from user variability, and lacks volumetric information. Any identified suspicious regions are then selected for a biopsy procedure, in order to extract histological information. A prototype medical device has been developed and built at Western University to provide an innovative technique to provide a more point of care (POC) 3D automated breast ultrasound (ABUS) approach. In this design, the breast is surrounded in an acoustic compatible structure, which then allows for ultrasound imaging to be acquired of the underlying breast anatomy. This ABUS device offers a portable, cost-effective, and high-resolution imaging solution. A commercially available ultrasound transducer, the 14L5 by Canon Medical Systems Canada Ltd, was integrated into a motorized translational stage that rests atop an enclosed mechanical frame. Spatially tracked two-dimensional ultrasound images are then passively captured, which are then rendered into a volume. Imaging was performed in phantoms, and linear measurement errors were 0.06±0.09, 0.05±0.06, 0.15±0.07 mm (N=22 each) in lateral, elevational, and axial US directions, respectively. Volumetric reconstruction error was 1.98±1.34% (N=10) in spherical inclusions of known volumes. FWHM measurements in the 3D image resulted in increased resolution uniformity. Images of healthy female volunteers were also acquired that demonstrate whole-breast 3DUS imaging with clear anatomical structures and details. The proposed prototype device show potential as an alternative, accurate, and high-resolution approach for whole-breast 3DUS imaging. These results demonstrate potential utility toward breast cancer screening in increased-risk populations independent of breast density.
The purpose of this poster is to show and discuss aspects of the construction and calibration of a new optical tweezers as well as an FCS setup. Optical tweezers use electromagnetic gradient forces together with radiation pressure to trap microscopic particles within a focused laser beam, and move them as required, making the tool suitable for applications in biological physics at microscopic scales. The Kilfoil lab has previously used optical tweezers to carry out active microrheology on a model system of entangled DNA and an ATP-powered DNA-disentangling enzyme; in combination with particle tracking to measure total position fluctuations, to distinguish the cumulative enzyme-driven non-thermal motions from the thermal motions. Now, we have incorporated components including an acousto-optical deflector for beam steering and a piezoelectric microscope stage for stage driving (with potential to turn the optical trap into a force clamp). This new version of the optical tweezers will be used in our active matter experiments on the same system (which models the cell nucleus), by combining both active microrheology and particle tracking. Another tool that can measure position fluctuations of system components even more mobile than microscopic beads (such as the enzyme itself) is fluorescence correlation spectroscopy (FCS). We are constructing an FCS setup for assisting in such soft and biological material studies.
Our goal is to develop a nano-biosensor using surface-enhanced Raman spectroscopy (SERS) to analyze and measure hemoglobin (Hb) levels, even at low concentrations, with good accuracy and reproducibility. This will facilitate fast and real-time differentiation of Hb disorders, such as sickle cell anemia, without using any labels or fluorophores.
To enhance the sensitivity of the Raman spectrum, noble metal nanoparticles with strong localized surface plasmon resonances are used to amplify the output signals by multiple orders of magnitude, resulting in a significantly stronger Raman spectrum. To achieve this, we utilize advanced gold nanostructured surfaces produced through the pulsed laser ablation technique. This thin film-like gold nanoparticle substrates manufactured by a top-down approach boasts high stability, sensitivity, improved accuracy, and greater precision in measurement than colloidal solution. The uniform interaction between analyte and substrate due to its controlled composition, thickness, and properties enables reliable and reproducible performance. These surfaces are coated with a novel heteroaromatic ligand L, the alpha-lipoic acid derivative of 2-(2-pyridine)imidazo[4,5,f]-1,10-phenanthroline, which selectively senses Hb. The phenanthroline unit of L can form strong coordination bonds with the iron center of the Hb’s heme unit, allowing for precise detection. Our SERS-based assay platform uses the dipping time vs Hb concentration dynamic study model to measure Hb levels. The porphyrin methine bridge-related SERS band at 1550 cm-1 is used to quantify Hb.
The stability of the sensor is monitored for a week by the SERS spectra which remained unchanged. Additionally, the sensor can differentiate between oxy and deoxy forms of Hb and distinguish between normal and abnormal Hb variants by analyzing the variation in SERS characteristic bands in the ‘fingerprint region’. Overall, this innovative approach holds great promise for the development of a lateral flow assay, enabling diagnosis of Hb disorders.
Keywords: Hemoglobin; Ligand functionalization; SERS; Gold nanostructured substrates; Pulsed laser deposition.
In this presentation, we will discuss the continuation of our construction of our Gee-Whiz experiments. These experiments focus specifically on techniques in ultrafast laser physics. We have been developing an experiment in frequency doubling and autocorrelation, both of which make use of an ultrafast laser. The experiment is especially noteworthy at Waterloo because it is part of a new “Gee-Whiz” set of experiments we are developing to help stimulate positive results in line with the expectations laid out by Self Determination Theory. This experiment embodies modeling-based designs similar to those developed by Dr. Natasha Holmes and Dr. Carl Wieman at the University of British Columbia and Cornell University. We are currently surveying our junior and senior physics lab students to understand the impact lab education has on their perspective towards experimental physics and perceived agency and also report on these findings. These attitudinal findings are further discussed elsewhere.
In September 2015, UN member states adopted the Sustainable Development Program known as Agenda 2030. This program defines targets to be reached by 2030 to meet the challenges of the current and future environmental crisis.
The UN's Sustainable Development Goals (SDGs) provide a reference framework for operationalizing sustainable development, including adaptation to climate change, improving global health and reducing social and environmental inequalities. This framework proposes 17 SDGs divided into a number of targets which, taken together, will ensure a more viable future for generations to come.
Universities have a role to play in building a more sustainable future, through knowledge development, education and knowledge transfer on major societal issues. Furthermore, universities can contribute by adopting sustainable approaches throughout the entire research process, from conceptualization to execution.
Our work builds on these concepts by developing tools for more sustainable scientific research, both in terms of the research object and the way research is carried out in the laboratory. Additionally, our objective is to identify barriers and overlooked areas in research when adopting a sustainable development approach. This works aims to brings researchers together to explore and discuss innovative strategies and best practices for incorporating sustainability into research practices. By recognizing the intrinsic connection between research and sustainability, we can foster interdisciplinary collaboration, enhance knowledge transfer, and accelerate the adoption of sustainable principles across various academic disciplines.
In 2019, we, as a group of scholars and community members working in fields as different as Physics, First Peoples Studies, Science Education, Decolonizing Curriculum and Pedagogy, Environmental Science, and Science and Technology Studies, came together to explore ways of decolonizing physics. Funded by the New Frontiers in Research Fund (NFRF), we decided to exemplarily focus on light (rather than on optics, as optics is a physical field and narrows down the concept of light and what can be said about it), because light is ubiquitous in every society, language, and culture. In everyday life, light is a key element that defines familiar aspects like colour and warmth. In physics, light is exploited as the primary carrier of information about nature (e.g., in astronomy), and used as the primary probe for the fundamental properties of matter (e.g., in spectroscopy). Our work is guided by the principles of centring Indigenous concerns and creating meaningful research and educational opportunities that support Indigenous sovereignty, particularly with regard to physics and science. In this talk, I will present the work that has been done so far, as well as the challenges, the changes, the risks, and the rewards that we have been experiencing in and with our project. The talk will take the attendees on a journey of what we have learned, what the project has changed, and what changes we, from our perspective, consider necessary to pursue physics in a non-colonial way.
The start of the COVID-19 pandemic and the first waves of lockdowns coincided with some big changes in how we approach learning on campus. Teleconferencing used to mean an awkward and clumsy Skype call, but now zoom meetings, zoom tutorials and zoom office hours are commonplace. Accommodations for at-home learning and assessments are sometimes expected. Online assessments are notoriously untrustworthy, but they do have benefits from an equity and diversity perspective. In physics we have shown that frequent online assessments result in less of a gender-gap than traditional high-stakes, in-person exams. Bound-paper introductory textbooks were still the norm before 2020, but since the pandemic almost no first-year students purchase paper textbooks. E-books, Open Educational Resources and Online Homework Systems offer students a more animated and interactive experience, and give instructors more opportunity to customize and author content. Many amazing virtual learning experiences have been attempted recently, but are there any that are worth keeping? I’ll also talk about the consequences of the recent virtual learning in high schools to physics education, and how our students have performed on pre-course physics quizzes when they arrived in the Septembers between 2012 and 2022.
The Belle II experiment at the SuperKEKB asymmetric $e^+e^-$ collider in Japan is a state-of-the-art upgrade to the original Belle experiment and is searching for new physics at the Intensity Frontier. Since commencing physics data taking in 2019, SuperKEKB has become the world’s highest luminosity particle collider as Belle II approaches its target integrated luminosity of 50 ab$^{-1}$, which will be 40 times larger than the combined datasets of the previous BaBar and Belle experiments. Enhanced by new dark sector triggers and its clean $e^+e^-$ collision environment, Belle II is pursuing a vast physics program that includes searches for rare decays of heavy hadrons and leptons, precision measurements of Charge-Parity Violation and cross-sections, and dark sector searches. This talk will present highlights of recent Belle II physics results and discuss the experiment's exciting future prospects.
Belle-II is a B-factory experiment on the luminosity frontier. The high luminosity leads to high backgrounds, specifically in the electro-magnetic calorimeter (ECL). The ECL is a subdetector made from CsI scintillators, mostly serving to detect photons and measure their energy. One background comes in the form of hadronic split offs which mimic low energy photons. These occur when a hadron interacts with a nucleus in the calorimeter, ejecting other hadronic matter which can cause further activity in other sections of the ECL. Attempts to discriminate these hadronic split offs using only ECL data have been limited in success. However, the K-Long and Muon Detector (KLM), an outer subdetector used to identify and detect muons and long-lived kaons, made from sandwiched iron plates and resistive plate chambers or scintillator strips, may have the ability to detect some hadronic matter responsible for hadronic split offs. This could allow the background ECL activity to be flagged and discriminated against. This talk summarizes a study done to check the feasibility of using the KLM for such a purpose.
A polarized electron beam is being considered as an upgrade for the SuperKEKB accelerator, which would enable a new precision electroweak physics program at Belle II. For many of the proposed measurements the dominant systematic uncertainty is expected to be the precision with which the average beam polarization is known. A novel technique for measuring beam polarization in $e^+e^-$ collisions, Tau Polarimetry, has been shown to be capable of measuring the average beam polarization to better than half a percent. The demonstration of the capabilities of Tau Polarimetry has been implemented at the BaBar experiment, a precursor experiment to Belle II, and the average beam polarization of it's associated accelerator, PEP-II, precisely measured. This presentation describes the physics underlying Tau Polarimetry, the systematic uncertainties which limit the technique, and the results of the BaBar measurement.
The New Small Wheel (NSW) is the largest major upgrade of the ATLAS Muon Spectrometer and was installed during the Large Hadron Collider (LHC) Long Shutdown 2 (2019-2021). The NSW replaced both of the 9-metre-diameter ‘small’ wheels constituting the part of the Muon Spectrometer closest to the beam line. The NSW is composed of two technologies: MicroMegas and small-Strip Thin Gap Chambers (sTGC). The sTGCs provide the primary triggers for the NSW. The detector layers of the sTGC consist of a wire plane centred between two cathode planes. One cathode plane is segmented into thin strips of constant width and the other into larger pads with variable sizes that define regions of interest for the first-level trigger.
The sTGC detector performance in a high background environment was studied at the CERN Gamma Irradiation Facility (GIF++). From signal strength studies of test beam data, it has been demonstrated that the pads of the sTGC are able to distinguish muon signals in high-background environments and are capable of operating well with background conditions similar to those expected during the High-Luminosity LHC.
A search for a beyond the Standard Model charged Higgs boson through $W\gamma$ resonances is presented, with a focus on the leptonic channel. The final state consists of either an electron or muon accompanied by at least one photon and less than two jets alongside a veto of b-jets is required. The analysis is based on the 139 $fb^{−1}$ of the proton-proton collision data at the centre-of-mass energy of 13 TeV collected by the ATLAS detector within the Large Hadron Collider. A mass range of 100 GeV to 200 GeV is considered for this hypothetical charged Higgs boson. The current status of this analysis will be presented.
Surveys of physics department chairs show that one of the most common threats faced by departments in 2022 were low student enrollments, sometimes putting the whole department in threat of closure. The EP3 Guide (ep3guide.org) provides a set of practices and strategies to help with both the recruitment and the retention of students. In this workshop, we will discuss a scenario from a fictional large department and discuss how the EP3 Guide can be used to address help the department make changes to improve enrollment.
Silicon photomultiplier (SiPM) detectors operated in Geiger mode are recently enabling a wide variety of biophotonics applications due to several advantageous features over traditional photomultiplier tubes. Silicon photomultiplier technology combines highly sensitive photon counting with miniaturized packaging, providing portability, low voltage operation, immunity to magnetic field interference, and low-cost detection. We will discuss our recent advancements in the design, development and opto-electronic characterization of these portable, sensitive, time-resolved biosensors, cable of capturing very low intensity light emissions from biological specimens. Integrating these solid-state single-photon avalanche diode array detectors, we will present a range of promising new biophotonic probes developed in our lab, from analyzing plant photosynthetic disruption of delayed fluorescence due to environmental stress exposure, to high speed pump-probe devices to interrogate the molecular micro-environment of cancer useful in understanding tumorigenesis and evaluation of new cancer therapies.
Inadequate oxygen delivery to the brain is a major cause of cerebral injury. Near-infrared spectroscopy (NIRS) is a portable and non-invasive technique that can detect brain injury by monitoring cerebral oxygenation. However, the use of NIRS for adult neuromonitoring has been stymied by significant signal contamination from their thick (~10mm) extracerebral layers (ECL; scalp and skull). Sensitivity to the adult brain could be improved by combining NIRS with a dual-slope (DS) technique. DS NIRS involves the use of a symmetric optode configuration to obtain an average optical attenuation coefficient that is more sensitive to deeper-lying tissue such as the adult brain. Previous implementation of the DS technique involved combining continuous-wave NIRS (cwNIRS) with frequency-domain NIRS (fdNIRS); however, such approach is costly and complex. Therefore, our objective is to evaluate the accuracy of a purely CW method that applies the DS technique to hyperspectral cwNIRS. Simulations were conducted on a two-layer phantom that mimics the ECL and brain using a finite-element method software for modeling light transport in tissue. The blood oxygenation level of the phantom was varied within the range of low to high cerebral oxygenation and the ECL thickness was varied to mimic the range of ECL thicknesses from infants to adults. Using an in-house hyperspectral fitting algorithm, the DS-cwNIRS data were analysed to recover cerebral oxygenation and the light scattering parameters of the brain. Preliminary results show that the DS-cwNIRS and non-DS approaches estimated cerebral oxygenation with similar accuracy. However, DS-cwNIRS was more accurate in quantifying light scattering (error = 7±4%) than the non-DS technique (error = 17±16%), suggesting that the former is a superior method for estimating brain optical properties. This is important because large errors in the estimated brain optical properties will reduce the accuracy of the estimation of cerebral blood flow, which is critical in neuromonitoring.
The experimental discovery of graphene has largely relied on making it visible by optical microscopes when deposited on silicon wafers coated by a 300-nm SiO2 layer, leading to constructive optical interference in the visible photon energy range [1]. While such a discovery has enabled exciting new areas of research, so many of them do not use graphene on 300-nm SiO2/Si. Thus, methods to image graphene on complex surfaces are of paramount importance. Here, we are targeting biophysics applications in which graphene flakes need to be deposited and imaged on leaves. This is complicated by the structure of the leaves, in which a layer of variable thickness (epidermis) overlaps to random globular objects (chloroplasts) leading to incoherent light scattering. We have devised a method to characterize graphene flakes on the surface of plant leaves via laser scanning confocal optical microscopy (SCOM) in the visible wavelength range (532 nm). Multilayer graphene flakes suspended in water with the aid of a surfactant (ribonucleic acid from Torula Utilis) were deposited on the surface of leaves of Ceratophyllum Demersum, which were imaged cross-sectionally using SCOM. Three-dimensional SCOM images were compared with computer simulations of the same (performed with an ad hoc designed routine running under Python) to model multiple reflections of light from chloroplasts, the leaves’ epidermis, and graphene as a function of the number of layers. These simulations indicate that, depending on the number of layers, graphene does affect the multiple reflections form underlying chloroplasts at different in-depth levels within a leave, from a few tens nm up to several hundred nm, thus providing a method to determine the thickness of the graphene flake. These results are essential to visualize and characterize graphene layers on leaves, further enabling the possible investigation of graphene as an assisting element in the process of photosynthesis.
[1] P. Blake et al. “Making Graphene Visible”. Appl. Phys. Lett. 91, 063124 (2007)
The analysis of human nail clippings to determine the concentration of certain elements is often used to assess exposure to elements and their absorption into the body. When nail clippings are used as a biomarker, they are usually analyzed by a “gold standard” method such as inductively coupled plasma-mass spectrometry (ICP-MS). Our group has investigated the use of a novel portable X-ray fluorescence (pXRF) technique as an alternative approach to assessing elements in nail clippings. The pXRF method allows for rapid and low-cost measurements using a single nail clipping or a series of nail clippings from an individual. Here, we report on results from the toenail clippings of mothers and infants living in New Zealand. Toenail clippings were obtained from participants in the Mother and Infant Nutrition Investigation (MINI). Energy spectra resulting from irradiation of the clippings were analyzed for characteristic X-rays from zinc and selenium. The MINI protocol involved the collection of toenail clippings from mother and infant pairings at three separate time points. Results of elemental analysis from two of these three time points are now available. Following non-destructive assessment of the toenail clippings by pXRF, they were then measured for elemental concentrations using ICP-MS. Results will be presented from both methods, and from both of the available time points. Dietary and environmental indications for the study population will be described. As well, the implications of the results for the use of pXRF to detect different elements in nail clippings will be considered.
general questions and comment session
Mamadou: I am not sure if this break is needed as the talk is already 30 min
To further advance the understanding of key reaction mechanism and paths in stellar nucleosynthesis and probe nuclear structure, experiments with radioactive isotopes in inverse kinematics are a vital tool to get direct information on reaction cross sections and rates. Unfortunately, the low intensities of radioactive isotope beams in relation to stable beams in combination with the extremely small radiative capture or transfer reaction cross sections of these reactions pose difficult experimental challenges. Therefore, it is advantageous to measure not only the light particle and radiation energy released by the reaction but the heavy recoil nucleus as well. With this coincident measurement technique the detector and beam background can be suppressed efficiently. Because of the inverse kinematics the heavy recoil is boosted forward in the direction of the unreacted beam and a clear separation between recoil and beam is necessary.
In this talk I will present an overview of the two devices DRAGON and EMMA installed at TRIUMF’s ISAC facilities to accomplish this with vacuum mode separation by particle mass over charge. To demonstrate the broad capabilities for nuclear reaction studies with these setups, a selection of recent results, planned experiments and upgrades will be highlighted in the second half of the presentation.
Neutron rich Mg isotopes far from stability belong to a region known as the island of inversion where the single particle description of the shell model breaks down, and the predicted configuration of the nuclear states becomes inverted. Nuclei in this region also exhibit collective behaviour in which multiple particle interactions play a significant role in nuclear matrix elements. These matrix elements can be studied through electromagnetic transition rate measurements, which allow for tests of theoretical models using the well-understood electromagnetic transition operators.
In-beam reaction experiments performed at TRIUMF, Canada's particle accelerator centre, allow for precise measurements of nuclei far from stability. Using TIGRESS in conjunction with the TIGRESS Integrated Plunger (TIP) allows for the implementation of Doppler shift techniques to measure transition rates in excited states of nuclei produced in low cross section reactions.
An experiment was performed using TIGRESS and TIP to measure excited state lifetimes in 28Mg using both the Doppler Shift Attenuation and Recoil Distance Methods to be sensitive to both short- and longer-lived states. $^{28}$Mg nuclei were populated using the $^{12}$C($^{18}$O,2p) fusion-evaporation reaction, with charged particles detected using the TIP CsI(Tl) ball, and gamma rays detected using TIGRESS.
Event reconstruction using detector-specific time windows were applied to remove uncorrelated background, while particle identification of light-charged ions was performed using offline fitting of CsI(Tl) waveforms taken during data collection. The resulting spectra demonstrate the successful separation of reaction channels by particle content, essential for studying $^{28}$Mg, as well as show clear evidence of the Doppler effects used to measure excited state lifetimes. The current status of data analysis and the impacts on nuclear physics will be discussed in this talk.
Potassium-40 ($^{40}$K) is a naturally occurring, radioactive isotope impacting understanding of nuclear structure, geological ages spanning timescales as old as the Earth, and rare-event searches including those for dark matter and neutrinoless double-beta decay. The long-lived $^{40}$K radionuclide undergoes electron capture decays to either the excited or ground state of its Ar daughter, of which the latter has previously not been measured, and estimates of its branching ratio are highly variable ($I_{\text{EC}^0}\sim (0-0.8)\%$). In many dark matter searches, $^{40}$K contamination produces a challenging 3 keV background from these electron capture decays in the expected direct-detection signal region, and the poorly understood ground state contribution may affect interpretation of the DAMA/LIBRA dark-matter claim. In geochronology, the common omission of this decay branch impacts ages obtained with K/Ar and $^{40}$Ar/$^{39}$Ar techniques. This rare third-forbidden unique decay additionally provides an estimate for the effective value of the weak axial-vector coupling constant in this regime, with applications to neutrinoless double-beta decay half-life calculations. The KDK ("potassium decay") collaboration has obtained the first measurement of this elusive $^{40}$K branch using a coincidence technique between a high-resolution silicon drift detector to observe X-rays, and a high-efficiency ($\sim 98\%$) Modular Total Absorption Spectrometer (Oak Ridge National Labs) to tag gamma rays, ultimately differentiating ground and excited state electron capture decays of $^{40}$K. With our measurement, the re-evaluated $^{40}$K decay scheme yields $I_{\text{EC}^0} = 0.098\% \stackrel{\mathrm{stat}}{\pm} 0.023\% \stackrel{\mathrm{syst}}{\pm} 0.010\%$. We report on our novel methodology and successful first measurement of this rare $^{40}$K decay, highlighting the multidisciplinary implications of our result.
Nuclei away from the line of stability have been found to demonstrate behavior that is inconsistent with the traditional magic numbers of the spherical shell model. This has led to the concept of the evolution of nuclear shell structure in exotic nuclei, and the neutron-rich calcium isotopes are a key testing ground of these theories; there have been conflicting results from various experiments as to the true nature of a sub-shell closure for neutron-rich nuclei around $^{52}$Ca. An experiment was performed at the ISAC facility of TRIUMF; $^{52}$K, $^{53}$K, and $^{54}$K were delivered to the GRIFFIN gamma-ray spectrometer paired with the SCEPTAR and the ZDS ancillary detectors for beta-tagging, as well as DESCANT for neutron-tagging. Using this powerful combination of detectors, we combine the results to construct level schemes for the isotopes populated in the subsequent beta-decay. Preliminary results from the analysis of the gamma, beta, and neutron spectra will be presented and discussed in the context of shell model calculations in neutron-rich nuclei.
A ubiquitous goal of nuclear physics, within the context of nuclear structure, is to provide an informed characterization of the behaviour of collectivity throughout the chart of nuclides. This initiative continues to present as extraordinarily non-trivial, especially when considering regions of heavy nuclei, as such nuclei are highly unique many-body systems with a complex array of properties. The investigation herein focuses on the study of the structure of 100Ru via the two-neutron transfer reaction, 102Ru(p,t)100Ru, that was performed using the Q3D magnetic spectrograph at the Maier-Leibnitz Laboratory, in Garching, Germany. The removal of the pair of particles from the system provides a direct study of the neutron-pair properties of the states that were observed in the reaction, which yields a more robust understanding of the pairing correlations present in 100Ru. These pairing correlations are a prime diagnostic used to characterize the behaviour of collective states within the context of the shell model, and can therefore be used to investigate how this feature evolves in different Z areas of the chart of nuclides. The study of the excited states of 100Ru extends further in another context, as it can add to the understanding of the double beta decay process of 100Mo to excited states of 100Ru. This investigation has significance with respect to the possibility of using 100Mo as a probe of the neutrinoless double-beta-decay process, which would shed light on the fundamental nature of neutrinos. This topic has the potential to offer high-impact deliverables, arising from the fact that it affects a wide breadth of sub-fields of physics outside that of nuclear structure, such as astrophysics and particle physics. This presentation will highlight the results from the analysis of the 102Ru(p,t)100Ru reaction, along with their significance for fundamental nuclear structure.
Bosonic quantum systems, such as photons, mechanical oscillators and spin ensembles, are promising platforms for implementing quantum technologies. Operating these quantum devices inevitably require interfaces that couple multiple bosonic degrees of freedom (modes). Unfortunately, each platform suffers from respective practical restrictions that limit the type of interface being implemented. In this talk, I will present our recent work in characterizing and engineering general two-mode bosonic interface. I will first introduce a set of unified physical parameters that uniquely specify every interface under single-mode operational constraints. Then I will illustrate an optimal, systematic strategy to engineer arbitrary interface by cascading multiple rounds of fixed, possibly platform restricted, interfaces. If time permits, I will also discuss how the interfaces are applied in quantum information processing.
We develop an approach for the characterization of universal qutrit gates which extends Clifford Randomized Benchmarking (RB). Our extension uses group theoretical and data recovery methods similar to RB. We show that our approach is both feasible and efficient, and compatible with current experimental methods. This extended RB scheme is valuable for three communities. For experimentalists, it provides a reliable method for verifying the correct functioning of their universal qutrit gate set. For RB researchers, it allows the application of well-established techniques in characterizing universal gates, placing our method at the forefront of the field. Additionally, group theory specialists can appreciate the practical application of group theory in the context of RB.
Quantum-classical correspondence plays an important role in understanding the emergence of classical chaos from an underlying quantum mechanics. Here we present several families of quantum dynamics, each parameterized by dimension, that do not approach the classically chaotic dynamics as predicted by Bohr’s correspondence principle. The quantum dynamics take the form of stroboscopic unitary kicks acting on a single spin system, and have the same finite temporal periodicity for all dimensions including the semiclassical regime. This state independent periodicity implies that under these specific dynamics, no initial quantum state fully explores Hilbert space as a state vector or phase space as a quasi-probability distribution. We also consider the stability of these families as a function of the degree of chaos in the classical model. Our study suggests that even in the highly semi classical regime, there are specific parameter values for which a quantum system never behaves classically or displays signatures of chaos.
Motivated by quantum gravity, semiclassical theory, and quantum theory on curved spacetimes, we study the system of an oscillator coupled to two spin-1/2 particles. This model provides a prototype for comparing three types of dynamics: the full quantum theory, the classical oscillator with spin backreaction, and spins propagating on a fixed oscillator background. From calculations of oscillator and entanglement entropy evolution, we find that the three systems give equivalent dynamics for sufficiently weak oscillator-spin couplings but deviate significantly for intermediate couplings. These results suggest that semiclassical dynamics with backreaction does not provide a suitable intermediate regime between quantum gravity and quantum theory on curved spacetime.
Sprays are dynamic collections of droplets dispersed in a gas. They are used in many industrial and agricultural applications such as manufacturing processes, fuel injection, painting, and crop protection. Furthermore, ‘‘Sprays are among the most intellectually
challenging and practically important topics in fluid mechanics” (Fansler, Parrish, 2014), requiring quantitative measurements for experimental verification of theoretical models..
Magnetic Resonance Imaging (MRI) is a non-invasive, three-dimensional imaging technique capable of measuring optically opaque media. The MR signal is directly proportional to the sample density, making the technique most sensitive for the liquid inside the nozzle and in the near-nozzle regions. These are also regions which represent a significant challenge for the most common optical methods used in spray characterization.
We have recently demonstrated the potential of MRI for spray studies (JMR 2016; JMR 2017; Appl.MR 2020). Density and velocity mapping can be performed for water inside ceramic nozzles with a sub-mm resolution. High spray speeds (> 10-20 m/s) in the near-nozzle region require development of magnetization preparation techniques to sensitize nuclear magnetization to parameters of interest. Considerable measurement challenges involve a trade-off between a high spatial resolution and time-of-flight effects caused by sample’s high speeds. Our current research focuses on bulk measurements of dynamic parameters of sprays (velocity distributions, dispersion, etc) in various regions of atomization, with the ultimate objective of translating the measurements to portable NMR setups.
Our lab recently introduced a methodology to determine the average velocity and flow behaviour index of laminar pipe flow using simple magnetic resonance techniques. The knowledge of these two parameters provides the information needed to reconstruct the flow velocity profile. However, as the flow velocity increases, the flow will begin to develop turbulence. For a given fluid moving through a pipe, the flow velocity profile is flatter in the centre of the pipe at turbulent flow rates compared to laminar flow. An effective flow behaviour index may also be used to approximately model the time-averaged velocity profile as a function of Reynolds number as a Newtonian fluid transitions to turbulence. In this presentation I will show the results of testing the utility of such a simplification in monitoring that transition.
Low-field portable magnetic resonance has several advantages over conventional high-field scanners, in that they are low cost, simple to construct, and readily employed outside a dedicated research lab. Numerous magnet designs have been created in recent decades which have been used for material characterization to improve industrial processes, and medical procedures. Portable magnet designs typically employ Neodymium Iron Boron to achieve a high magnetic field. This may be advantageous to increase the magnetic resonance signal but adds to complexity due to the hazards associated with construction and usage.
This presentation will discuss a new magnet design which uses two thin rectangular grade C8 ceramic magnets to create either a large homogeneous measurement volume, or a constant magnetic field gradient of 15 gauss/cm in the measurement volume. Ceramic magnets are inexpensive and may easily be purchased with specific dimensions, making them ideal for magnet design. Additionally, they are naturally corrosion-resistant, making them advantageous for applications outdoors.
The magnets are displaced by a distance to create a 1.8 MHz for 1H (423 gauss) magnetic field over a large volume. Due to the low magnetic field gradient, the corresponding sensitive volume is large, which results in sufficient signal-to-noise to perform a flow velocity profile measurement. As such, we characterize the flow behavior index n’ and the average velocity of water flowing in a tube. Such measurements validate this design’s use for magnetic resonance and lay a foundation for further exploration.
Introduction:
Magnetic resonance imaging of short signal-lifetime samples comes with several challenges1, namely lower signal and the need for short acquisition windows. The apparent transverse relaxation time ($T_2^*$) of water-content in cement paste has been measured2 to be <0.3ms at 3T: this suggests imaging at low field (<0.5T) where $T_2^*$ is expected to be longer, permitting 2D imaging of water penetration in a clay sample. However, proton imaging at low field prohibits the use of low flip-angles if high signal is desired, so a short echo-time (TE) pulse sequence using 90° flip angles was implemented with a water and clay sample at 74mT.
Method:
The x-centric pulse sequence3 consists of acquiring each half of every k-space line separately, from the centre outwards in the readout/kx direction: this halves the acquisition duration and ensures the centre of k-space is acquired first, minimizing signal decay caused by $T_2^*$ relaxation. This pulse sequence was used to image water distribution in a 12mL bentonite clay sample on a 74mT MRI system and compared with the traditional gradient echo (GRE) sequence. Eight $T_2^*$-weighted images were obtained using 8 different TEs=0.5ms…10ms. Bulk relaxation measurements of the longitudinal ($T_1$) and apparent transverse relaxation times were also performed for increasing water content (1mL increments).
Results:
The $T_1$ relaxation was around 10ms and was largely independent of water content; the $T_2^*$ relaxation was proportional to the amount of water in the clay (3 to 5ms). The x-centric pulse sequence was 2.5 times more efficient than GRE. A 2D $T_2^*$ map was generated from eight $T_2^*$-weighted x-centric images: the global mean $T_2^*$ value was 6.4$\pm$3.2ms.
Conclusion:
We have shown that x-centric was able to image the water content in the bentonite clay with minimal $T_2^*$-weighting. To our knowledge, this is the first attempt to image water-content in bentonite clay4. The $T_2^*$ dependence on water content suggests that a $T_2^*$ map also represents a regional water absorption/content map. The short $T_1$ measured here should allow for rapid real-time 2D and 3D imaging of water penetration in porous materials, and the significantly longer $T_2^*$ at this field strength alleviates the imaging issues caused by this fast signal decay.
References:
1 Muir et al. MRC (2013); 2 Sakai et al. OJCE (2017); 3 Ouriadov et al. MRM (2015); 4 Fagan et al. MRI (2005)
An exploratory multinuclear MR and MRI study was performed on lithium-ion battery cells with $^7$Li, $^{19}$F, and $^1$H measurements. A variable field superconducting magnet with a fixed frequency parallel-plate RF probe was employed in the study. The magnet's magnetic field was changed to set the resonance frequency of each nucleus to the fixed RF probe frequency of 33.7 MHz. Two cartridge-like lithium-ion cells, with graphite anodes and LiNi$_{0.5}$Mn$_{0.3}$Co$_{0.2}$O${_2}$ (NMC) cathodes, were interrogated. One cell was pristine and one was charged to a cell voltage of 4.2 V. The results presented demonstrate the great potential of the variable field magnet approach in multinuclear measurement of lithium-ion batteries. These methods open the door for developing faster and simpler methods for detecting, quantifying, and interpreting MR and MRI data from lithium-ion batteries.
Reservoir rocks which trap oil and gas have been extensively studied for decades, due to their importance in the petroleum industry. Pore size is an important petrophysical property controlling fluid storage and fluid transport in reservoir rocks. Many techniques such as scanning electron microscopy (SEM), X-ray, and mercury injection capillary porosimetry (MICP), have been applied to estimate pore size, however, with some limitations, for example sample size, measurement cost, and sample damage. Magnetic resonance (MR) is a very promising technique for interrogating such samples, because it is non-destructive, non-invasive and sensitive to fluid dynamic and environment.
This presentation will discuss a new direct and rapid one-dimensional MR method to estimate the pore size and surface relaxivity of porous materials. MR signal decay rates, from fluids in the pore space, depend on the pore size, the surface relaxivity and molecular self-diffusion as described by Brownstein-Tarr (BT) theory. In the present work, the correlation between MR relaxation behavior and the temperature-dependent self-diffusion coefficient of pore fluids was employed. The MR relaxation lifetime and the relaxation regime of the samples were shifted due to temperature variation. This shift was used to estimate the pore size and surface relaxivity by nonlinear fitting.
Water-saturated glass bead packs were employed in initial experiments at variable temperature. The calculated pore size matches the estimated geometric pore size. The proposed method was applied to determine the pore size of fluid saturated Berea, Buff Berea and Nugget sandstones. The pore sizes determined with three pore geometries are in good agreement with scanning electron microscopy (SEM) and uCT measurements.
The general computation of dynamic properties of materials remains a longstanding, difficult problem within computational physics. Surprisingly, simple models such as the homogeneous electron gas (jellium) play critical roles in application of Density Functional Theory and its time-dependent extensions. Those calculations are impeded by the difficulty of evaluating Feynman diagrams on the real frequency axis that are required to describe screening processes. In this talk I will introduce a diagrammatic Monte Carlo technique based on a partially symbolic computational tool, algorithmic Matsubara integration, that allows us to compute frequency and momentum resolved finite temperature response functions directly in the real frequency domain. Using the obtained data for charge response at moderate electron density we, for the first time, compute the exchange-correlation kernel for jellium by a controlled method and revealed unexpected features in its frequency dependence. To emphasize the wide applicability of the approach I will also summarize other applications of the methodology for computation of diagrammatic expansions in model systems.
Experiments in doped transition metal oxides often show suppression in the single-particle density of states at the Fermi level, but disorder-induced zero-bias anomalies in strongly-correlated systems remain poorly understood. Numerical studies of the Anderson-Hubbard model have identified a zero-bias anomaly that is unique to strongly correlated materials, with a width proportional to the inter-site hopping amplitude $t$.[PRL 101, 086401 (2008)] In ensembles of two-site systems, a zero-bias anomaly with the same parameter dependence also occurs, suggesting a similar physical origin.[PRB 82, 073107 (2010)] We describe how this kinetic-energy-driven zero-bias anomaly in ensembles of two-site systems may be seen in a mesoscopic realization based on double quantum dots. Moreover, the double-quantum-dot measurements provide access not only to the ensemble-average density of states but also to the details of the transitions which give rise to the zero-bias anomaly.
We consider two approaches when calculating the properties of a ferroelectric system with charged
domain walls. These properties include domain wall width, electronic band structure and occupancy,
and the electronic potential energy. Previously, a single parameter, Q, was argued to determine the
crossover of the electron gas from quantum to quasi-classical. However, to obtain this result, two
simplifying approximations were made in the description of the domain wall. When compared with
a more robust approach it appears these approximations are only valid for a low Q value system. We
discuss why these approximations are not always valid depending on the material parameters, i.e.
the Landau theory parameters.
The rigid rotor is a classic problem in quantum mechanics, describing the dynamics of a rigid body with its centre of mass held fixed. It can be viewed as the quantum mechanics of a particle moving in SO(3), the space of all rotations in three dimensions. The particle can move along two types of closed loops: trivial loops that can be adiabatically shrunk to a point and non-trivial loops that cannot. This topology can lead to new consequences. With time-reversal symmetry, a Berry phase of π can be attached to all non-trivial loops. We solve this problem by exploiting the connection between SO(3) and SU(2) spaces. Remarkably, this framework is realized in the low-energy physics of certain quantum magnets. We demonstrate this result in a family of Heisenberg antiferromagnets defined on polygons with an odd number of vertices. At each vertex, we have a spin-S moment that is coupled to its nearest neighbours. Their quantum spectra, at low energies, correspond to spherical top' andsymmetric top' rigid rotors. For integer values of S, we recover traditional rigid rotor spectra. With half-integer-S, we obtain rotor spectra with a Berry phase.
The Super-Kamiokande (SuperK) and Hyper-Kamiokande (HyperK) water Cherenkov detectors for particle and astroparticles consist of photomultiplier tubes (PMTs) that detect Cherenkov light surrounding a large ultra-pure water tank (40m and 70m diameter, respectively).
Water quality is critical because it ensures good water transparency and, as a result, a long Cherenkov light attenuation length compared to detector size. In this case, even charged particles with low energies that produce few photons can be detected efficiently.
When compared to standard water sampling tests, optical measurement has the advantage of monitoring water quality constantly. Thus, by measuring light transmission after passing through a 10m sample of water, one can gain insight into potential contamination sources through time-correlating water quality changes with environmental change.
TRIUMF is developing a high-sensitivity optical water monitoring system that can continuously monitor water quality for the HyperK detector. This system will also be used for a water Cherenkov test experiment (WCTE) at CERN in early 2024, for which we will develop an operation and calibration procedure, as well as analysis tools.
During this talk, I will present the schematics of the water monitoring detector, the work done to build the prototype detector and the optical study of this system.
Silicon PhotoMultipliers (SiPMs) have been adopted in many applications due to their ability to reliably detect single photons with excellent timing resolution. These applications range from detecting scintillation photons in large area particle physics experiments, to light detection for LiDAR or other industry uses. Due to the large internal gain of these devices ($\sim10^6$), a large number of secondary photons are produced during the detection process, which can induce false signals in the SiPM and degrade their timing or energy resolution. The characterization of these secondary photons is important for designing future SiPM devices that mitigate these byproducts. At TRIUMF we developed an instrument to simultaneously stimulate individual micro-cells of SiPMs and measure their secondary emission. The setup features a cooled X-Y stage to enable characterizing emission at a wide range of temperatures (20°c to -187°c) and to match experimental conditions of LXe and LAr common in the next generation of particle physics experiments. The measurements obtained are used alongside an effective transmission model to deduce an absolute spectrium of secondary photons produced during the detection process. In this work we have characterized Hammamstu VUV4 and Fondazione-Bruno-Kessler (FBK) VUV HD3, two candidate SiPM devices for the nEXO neutrinoless double beta decay experiment. And it will also be illustrated how this work is important for the design of a detector concept for dark matter search in silicon using avalanche diode arrays.
MUTE (MUon inTensity codE) is a Python program (https://github.com/wjwoodley/mute) that combines two state-of-the-art codes, MCEq and PROPOSAL, to calculate muon intensities and spectra in deep underground and underwater laboratories. We have previously shown that, using these tools, MUTE can provide forward predictions while accurately characterising the uncertainties arising from hadron production models. In this new study, we expand our analysis by calculating total muon fluxes, and comparing with the current experimental data. The results are in very good agreement with the data, implying MUTE can be a powerful tool for Dark Matter and neutrino experiments to estimate muon-induced backgrounds for future generation detectors. As we have previously shown that the uncertainties on the underground data are smaller than the current theoretical uncertainties, we will discuss the suitability of this data in constraining high-energy neutrino flux calculations. Additionally, we predict the seasonal variations in labs located under flat earth and mountains using topographic maps of the overburdens, which can be of particular interest in studying the annual modulation of Dark Matter candidates. Lastly, MUTE can provide accurate underground angular distributions, which can be compared against experimental data. This can be used as a cross-check to identify any issues in data analyses, such as event misreconstructions or issues with the position of the detector in the mountain map.
In this talk I will present updated results regarding the application of machine learning techniques for noise removal and physics-variable prediction on signals from spherical proportional counters (SPCs) with the NEWS-G experiment. In SPC detectors, a primary ionization, created by a particle interacting with the gas, drifts towards a central anode. When ions approach the anode, the electric field becomes strong enough to trigger secondary ionizations, resulting in an amplified detector signal. Evaluation of these techniques include tests on simulated pulses with added noise and quantifying the impact of noise-removal and single-output prediction on physics goals such as primary ion counting and energy resolution. Successful implementation of this technique will reduce errors on event measurements (energy, drift time, etc.) and lower the analysis threshold, thereby enabling the experiment to search for lower mass dark matter events.
We study the effects of dark matter self-interactions on the local dark matter distribution in selected Milky Way-like galaxies in the EAGLE hydrodynamical simulations. The simulations were run with two different self-interacting dark matter models, a constant and velocity-dependent self-interaction cross-section. We find that the local dark matter velocity distribution of the Milky Way-like halos in the simulations with dark matter self- interactions and baryons are generally similar to those extracted from cold collisionless dark matter simulations with baryons. In both cases, the local dark matter speed distributions agree well with their best fit Maxwellian distributions. Including baryons in the simulations with or without dark matter self-interactions increases the local dark matter density and shifts the dark matter speed distributions to higher speeds. To study the implications for direct detection, we compute the dark matter halo integrals obtained directly from the simulations and compare them to those obtained from the best fit Maxwellian velocity distribution. We find that a Maxwellian distribution provides a good fit to the halo integrals of most halos, without any significant difference between the results of different dark matter self-interaction models.
The NEWS-G experiment at SNOLAB uses spherical proportional counters, or SPCs, to detect weakly interacting massive particles (WIMPs), which are a prime candidate for dark matter. Interactions within the gas-filled sphere create a primary ionization. Then, a radial electric field acting throughout the detector volume collects the electrons towards an anode sensor located at the sphere’s center. This signal is amplified through a Townsend avalanche caused by the electric field. Signals are then processed using a double deconvolution procedure, which enables single electron counting.
The preliminary data analysis from the SNOLAB detector, which began taking data in Fall 2022 with a neon mixture, will be discussed. This will include results of the Argon-37 energy calibration, electron drift time measurements, selection cuts to remove identifiable background sources and measurements of surface and volume background rates. This preliminary analysis provides an important basis for future analysis work by reducing background sources within the data and allowing for a more detailed understanding of the physics processes in the detector.
Join panelists at this lunchtime panel discussion to learn about initiatives being undertaken in Physics departments and Faculties of Science across the country to advance Equity in STEM. These panelists will bring a multidisciplinary perspective across STEM fields, with a student lens and a leadership frame of reference to provide the audience with concrete actions that have led to enhanced Equity, Diversity, Inclusion and Accessibility, not only in Physics departments but also in Faculties of Science in Canada. They will answer questions such as: How do we integrate social justice and STEM? How can we integrate the Equity Ethic into our programs to attract Equity Deserving groups? What are some of the lessons learned from the census of the Physics community in Canada? How do student leaders view the current state of EDIA efforts in Physics? What are some of the lessons learned from Physics departments participating in the APS IDEA project? What are some of the data driven approaches being taken by equity leaders in Faculties of Science to ensure the full participation of equity deserving groups?
Ninan Abraham is Professor of Microbiology and Immunology and past Associate Dean Equity, Diversity and Inclusion in the Faculty of Science at UBC. Kalaichelvi Saravanamuttu is Professor of Chemistry and Chemical Biology and inaugural Associate Dean of Equity, Diversity, Inclusion & Indigeneity in the Faculty of Science at MacMaster University; Steve Dodge is an Associate Professor of Physics and the Faculty Coordinator for the Physics IDEA committee at SFU and Kevin Hewitt is Professor of Physics and the inaugural Associate Dean of Equity and Inclusion in the Faculty of Science at Dalhousie and co-lead its APS IDEA team. Anastasia Smolina is a PhD candidate in Medical Biophysics at the University of Toronto and co-lead CanPhysCounts, the first diversity census of the Physics community in Canada.
We often see new advances and insights emerging from the intersection
of different ideas coming from what appeared to be disconnected research areas.
The theme of my talk will be an ongoing collision between the three topics
listed in my title which has been generating interesting new insights into a
variety of fields, eg, condensed matter physics, quantum field theory and
quantum gravity.
Ever since the first measurements were made of these ghostly particles, neutrinos have been a constant fascination for physicists due to their unusual properties. One such peculiarity is that neutrinos can seemingly change flavours as they propagate — a phenomenon known as neutrino oscillation. The oscillation probabilities are determined by a set of fundamental parameters in the Standard Model. Decades of neutrino experiments designed to probe these parameters have narrowed down much of the phase space, yet many unanswered questions remain: Is there CP-violation in the lepton sector? Which neutrino is the lightest? Are there neutrinos beyond the three generations? The answers to these questions may hold the key to discovering physics beyond the Standard Model and understanding our universe, but answering them requires detectors much more powerful than those currently in operation. In this talk, I will focus on the two next-generation long-baseline neutrino experiments — Hyper-Kamiokande and the Deep Underground Neutrino Experiment (DUNE), and how they will be able to answer these questions. In addition, I will also discuss their wide-ranging physics potential, such as the study of Solar neutrinos, supernova neutrinos, and the search of proton decay.
STrings for Absorption Length in Water (STRAW) is a pathfinder mission
for the proposed Pacific-Ocean Neutrino Experiment (P-ONE). STRAW
was deployed in 2018 with the goal of measuring the attenuation length of
the water. The results of these measurements were published in 2021 and
qualify the site for a large scale neutrino detector. STRAW is located in the
Cascadia Basin, an area off the coast of Vancouver Island. The full P-ONE
array will eventually be deployed to the same location. STRAW continues to
take data, and has long outlasted its original design expectations. This extra
data-taking time has enabled new studies of the sub-sea environment. One
measurement of interest is the identification of atmospheric muons, which
form a background in neutrino experiments, using STRAW. Another measurement
of particular concern is the growth of organic matter on undersea
equipment, a phenomenon known as biofouling. Biological material grows
on the glass of optical modules, thus reducing their light collection efficiency
over time. This talk explores the suitability of the STRAW apparatus for
making these measurements, and how this informs the next phase of P-ONE
which will be deployed in the near future.
The precision measurements of neutrino oscillation parameters and neutrino-nucleus scattering and also unprecedented sensitivity to physics beyond the Standard Model are the goals of the Hyper-K experiment, a next generation long-baseline neutrino experiment. To be able to achieve these high precision and sensitivity these experiments need a reduction on the uncertainties in neutrino fluxes calculations. New measurements of hadron-nucleus interaction are needed to reduce uncertainties of neutrino fluxes. EMPHATIC is a low-cost, table-top-sized, hadron-production experiment located at the Fermilab Test Beam Facility in Chicago that aims to measure hadron scattering and production cross sections that are relevant to neutrino flux predictions. In my presentation I will show measurements of the differential cross-section as a function of scattering angle for kaon carbon interactions with a single charged particle in the final state at beam momenta of 30 GeV/c. These results can be used in current and future long-baseline neutrino experiments, and demonstrate the feasibility of future measurements by the EMPHATIC spectrometer.
Antineutrino scattering on free protons (or neutrino scattering off free neutrons) gives a unique measurement of neutron and proton structure and is a building block for predicting neutrino scattering on more complex nuclei. Previous measurements have to rely on scattering neutrinos off deuterium and then correcting for nuclear effects, or by low-intensity anti-neutrino beams. In this talk, MINERvA will present the first high statistics cross section measurement of the charged current elastic process νμp → μ+n using the plastic scintillator (CH). The carbon background is significantly reduced and constrained with minimal model dependency using the kinematics of the reconstructed neutrons. The result can be directly compared with lattice QCD computations, and to electron scattering off free protons.
The Tokai-to-Kamioka (T2K) long-baseline neutrino experiment measures neutrino-flavor oscillation parameters using the three-flavor oscillation model parameterized by the PMNS matrix. The measurement is performed by sampling the JPARC (anti)neutrino beam by various detectors at a near detector complex before oscillations and at a far detector after oscillations. A critical part of the data analysis is the fit machinery that finds the best compatibility of the model with many parameters (neutrino interaction, flux, detector, and oscillation model parameters) and the neutrino scattering data. T2K uses several approaches to fit the data that are frequently cross-checked against each other. In this talk, the Bayesian analysis approach is presented, which performs a joint near-far detector fit and uses a Markov Chain Monte Carlo sampling.
There is a 10$\sigma$ discrepancy between theory and experiment for the ionization energy of the $1s2s^3S_1$ state of helium [1]. In order to provide an additional check, Clausen et al. [2] have performed measurements for the Rydberg $P$-states of helium from $n = 24$ to $n = 100$ and extrapolated to $n = \infty$ to find the ionization energy. In the present work, we extend previous high-precision variational calculations [3] up to $n = 24$ using triple basis sets in Hylleraas coordinates. With the inclusion of relativistic and QED corrections, the results provide a direct theoretical test against the Clausen measurement at $n = 24$. The results are in excellent agreement, thereby confirming the 10$\sigma$ discrepancy between theory and experiment for the ionization energy of the $1s2s^3S_1$ state of helium.
[1] V. Patkos, V. A. Yerokhin and K. Pachucki, Phys. Rev. A 103, 042809 (2021).
[2] G. Clausen et al. Phys. Rev. Lett. 127, 093001 (2021).
[3] G. W. F. Drake, M. M. Cassar and R. A. Nistor, Phys. Rev. A, 65, 054501 (2002).
The Abraham-Minkowski “controversy” is a debate in physics which began over a century ago, stemming from an ambiguity in defining the momentum of light within a medium. Simple physical arguments lead to a prediction that the momentum of light should either increase or decrease by a factor of the refractive index (compared to its value in the vacuum) upon entering a medium. Experimental attempts to discriminate between the two theories often support one over the other at first glance, but upon deeper consideration cannot refute either. While a resolution to the apparent paradox has been proposed, some physicists remain unconvinced. By measuring the interaction time between light and an atom, we hope to extract information about the momentum imparted to the atom by light, thereby elucidating the momentum of light in a medium.
The two definitions of coherence: quantum and classical, are equivalent under the condition of stationarity and both remain useful for different experimental scenarios. However, as in many scenarios, the boundaries and connections between quantum and classical become unclear without common assumptions. One such scenario is an ultrashort laser pulse. Classical coherence is almost always defined for stationary and ergodic processes, which leads to a confusion between the time and ensemble averages for non-stationary processes, such those that are ultrashort. Quantum mechanical coherence does not require stationarity but it is an ensemble average over field modes rather than instances of the field. This means it cannot be applied to classical pulse shapes, such as those generally used to describe an ultrashort pulse, unless those fields are written as spatial-temporal modes. These modes are linear combinations of the usual monochromatic plane wave modes of the electromagnetic field. We derive a method to generate a set of spatial-temporal modes that describe a generic pulse shape. Further, by considering the coherent and single photon states of spatial-temporal modes, we can discuss the photon composition of laser pulses. This presents interesting implications for models that consider light as photons without being in a photon number state and helps to clarify experimental interpretations.
We present a theoretical model of Electromagnetically Induced Transparency in an ensemble of three-level atoms that are driven by a probe and a control field in a lambda configuration. The ensemble is modelled by a 5-level quantum system with the mean-field interactions between atoms modelled by decoherence terms. The dynamics of the ensemble are calculated by solving the Lindblad Master Equation for the density matrix. From the density matrix, the polarizability and the frequency-dependence of the susceptibility are calculated. The control field induces transparency to the probe field due to interference between multiple pathways. A strong dependence on the density of the ensemble is observed.
The hyperfine structures of the $2^3S_1$ and $2^3P_J$ states of $^7$Be$^{2+}$ and $^9$Be$^{2+}$ are investigated within the framework of the nonrelativistic quantum electrodynamics, including relativistic and radiative corrections up to order $m\alpha^6$. The uncertainties of the calculated hyperfine splittings are on the order of tens of ppm, and for $^9$Be$^{2+}$ our results improve the previous theoretical and experimental values by at least two orders of magnitude. The improved sensitivity of the hyperfine splittings of $^{7,9}$Be$^{2+}$ to the nuclear Zemach radius and electric quadrupole moment opens the way to future measurements to extract the atomic physics values of these two nuclear properties to an accuracy of 5% or better.
Laser-induced breakdown spectroscopy (LIBS) is a real-time spectrochemical technique that involves performing time-dependent optical emission spectroscopy on high-temperature laser-induced microplasmas. The use of a focused laser beam allows one to make sensitive assays of the elemental composition of specimens while requiring only micrograms of analyte mass. Numerous medical and biomedical applications of LIBS have been studied and proposed, including the rapid detection of bacterial infection.
Our group has demonstrated the ability to detect and classify bacterial cells in arbitrary fluid specimens using a centrifugation device to deposit cells on nitrocellulose filters. Bacterial concentrations of 11,000 CFU per laser shot were detectable using 8 mJ pulses from a 1064 nm, 9 ns Nd:YAG laser with a spot size 75 micron in diameter. A partial least squares discriminant analysis on LIBS spectra from specimens of blood and urine spiked with known bacterial pathogens possessed a 98.9% sensitivity and 100% specificity for detection in urine and a 96.3% sensitivity and 98.6% specificity for detection in blood.
An artificial neural network analysis with principle component analysis pre-processing of the LIBS spectrum was used to discriminate three species of bacteria. Use of an 80:20 split cross-validation resulted in an average sensitivity and specificity of 97.2% and 98.6%, respectively, for the discrimination of bacteria in urine. External validation performed on 16 filters gave an average sensitivity of 77.5%. Applying PCA-ANN using an 80:20 split cross-validation for the discrimination of bacteria in blood resulted in 100% sensitivity and specificity. External validation of 19 filters of bacteria in blood yielded an average sensitivity of 82.3%. These results indicate the potential usefulness of LIBS in the clinical setting.
Work supported by the Natural Sciences and Engineering Research Council (NSERC) of Canada.
Purpose: In the context of previous analysis of dynamic nuclear medicine acquisitions, a
lack in available software was noticed: commercial systems are too opaque and do not
allow a sufficiently flexible use. To tackle this challenge, home-made scripts were
devised, which were then packaged for wider use. The goal is two-fold: dissolve
difficulties specific to dynamic nuclear medicine using new and old tools and make these
available to a greater number of scientists in a simple and convivial way. The software
Techniques for the Reliable Use of Medical Physics Images (Tru-M.P.I.) was created
with this endeavour in mind.
Content: Using freely available and open-source Python packages, a Graphical User
Interface (GUI) was created to allow users of various backgrounds and interests to use
the devised tools efficiently.
Within this interface, it is possible to extract a 4-D image from Dicom files and then
segment it according to various schemes, with all the relevant parameters selectable by
the user. The resulting segmentations can be visualized directly, as well as the extracted
Time-Activity Curve (TAC). These segmentations can be deformed, used to compute
error bars, or extract the pharmacokinetic parameters.
Various utilities are also included to offer a better user experience, such as the
possibility to export the results in various formats.
Included Schemes: Segmentation schemes include, so far, an ICM, a filling algorithm,
and a gradient method.
Methods to compute error bars and for deformations include translations, rotations,
expansions, and reflections.
Methods to extract the pharmacokinetic parameters are based on nested sampling, via
the Dynesty package.
Verification: The tool was tested on various dynamic nuclear medicine acquisitions,
namely from phantoms and rats. As testing will progress, further tools and segmentation
schemes will be added, following the current needs of the field.
Future Development: The scripts and GUI will be made available to scientists and
researchers. Feedbacks, suggestions, and enquiries will be welcome and required in
order to improve the current state of the project.
Our group is developing a plastic fiber optic probe dosimeter based on a radiochromic sensor for real-time in vivo dosimetry. The active component of the probe material is a lithium pentacosa -10, 12-diynoate (LiPCDA) coating on the order of microns in thickness. In radiochromic optical dosimeters both sensitivity and active material thickness variations in manufacturing can lead to uncertainty in the dose measurement. Thus, to confidently determine the dose, independent of optical path length variations in the interrogation beam arising from different radiochromic film thicknesses, an inert homogenously incorporated infra-red (IR) dye such as IR-783 and IR-806 can be added to the LiPCDA formulation for calibration. This enables an accurate thickness correction using the Beer-Lambert law. For use as a calibrant, however, these dyes must be both stable in ambient environmental conditions over time and resistant to radiolysis. To investigate the stability of these IR dyes, LiPCDA gelatin-based coatings from the two proposed IR dyes were prepared. The coatings were left in ambient conditions in a dark space, and their absorbance spectra was measured frequently for >100 days. We performed control experiments with IR-783 and IR-806 dyes to investigate degradation in time without the active LiPCDA material, which showed average decay lifetimes of τ = 73 ± 7 days and τ = 7 ± 3 days, respectively for IR-783 and IR-806. When incorporated with LiPCDA, IR-806 showed a significant shift in the main absorbance peak, overlapping with the dosimeter active component. Comparatively, IR-783 combined with LiPCDA did not show significant overlapping peaks in the spectrum and exhibited single exponential decay behaviour with a faster decay rate (τ = 4 ± 1 days) relative to the control. IR-783 was further observed to be insensitive to ionizing radiation dose. Therefore, IR-783 may be a suitable dye for calibrating radiochromic dosimeters given its predictable and reproducible exponential decay behaviour.
We are well aware that every human can be identified by their unique fingerprint. Taking inspiration from natures’ this wonder, there is an exclusive feature to identify different molecules/chemicals in materials science. We can find this attribute in the way molecules vibrate. Different molecules have different vibrational modes depending on their chemical constituents, bonding strength, structure, interaction and so on. Hence, we need sensitive instrumentation that can detect these vibrations, that is, Vibrational Spectroscopy (VS). VS is a powerful technique, which identifies the chemical-specific fingerprint of a molecule in its natural state without the need for labelling or sample preparation. This is a considerable advantage to chemists and biologists for the recognition and characterization of synthesized drugs, and chemicals, and assessing the purity of compounds compared to other techniques which are either invasive or/and require tagging of a molecule with a fluorophore to visualize them. VS encompasses two complementary techniques i.e. Raman and Infra-red (IR) spectroscopy forming a comprehensive system. They only differ in the selection rules for the different vibrational modes. That is, Raman detects those vibrational modes resulting from change in polarizability whereas, in IR, vibrations due to change in dipole moment are registered.
Although powerful as a technique, there are limitations to the concentrations of molecules that Raman can detect since it is a weak process. In order to alleviate this issue, tailored nanostructured particles are employed to create local enhancement effects known as hot spots. These nanostructures enhance the Raman signals even for ultra-low concentrations of molecules. In my talk, I will discuss the nanostructured devices used for surface enhanced Raman scattering with biological applications related to sensing.
Constraining the properties of nuclear media at extreme densities has been a long-time goal of relativistic heavy-ion collision experiments. Mounting evidence gathered from these experiments suggests that a strongly interacting plasma of quarks and gluons – the Quark Gluon Plasma (QGP) – is being created within these collisions. The QGP can be well described using multi-stage simulations where relativistic dissipative hydrodynamics plays a key role. Recently, hydrodynamics has been systematically derived from the relativistic Boltzmann equation by isolating its long-distance moments in an irreducible moment expansion. This formulation of hydrodynamics is the basis of modern fluid simulations of the QGP. To compare hydrodynamical calculations against data, fluid dynamical simulations are followed by molecular dynamics of hadronic (quarks and gluon) bound states. The latter is responsible for simulating hadronic chemical and kinetic evolution far outside thermal equilibrium. A systematic extraction of QGP properties thus requires a combination of multi-stage simulations running on supercomputers, along with Bayesian model-to-data comparisons. As most of the particles produced in a heavy-ion collision are soft (with $p_T < 3$ GeV/$c$), Bayesian analyses of the QGP have focused on describing soft particle emissions. I will describe what constraints on the dissipative properties of the QGP, i.e., on its shear and bulk viscosity, were achieved using Bayesian analyses I have led, and outline a path towards an even deeper understanding of the QGP.
We discuss how a condensate of non-abelian gauge fields is impacted with gravitational interactions in the early universe. The aim is to provide for new observational physics in the current cosmological background, as relics of early universe phenomena.
Since the derivation of a well-defined D → 4 limit for 4D Gauss-Bonnet (4DGB) gravity coupled to a scalar field, there has been interest in testing it as an alternative to Einstein’s general theory of relativity. Using the Tolman-Oppenheimer-Volkoff (TOV) equations modified for 4DGB gravity, we model the stellar structure of quark stars (QS) using a novel interacting quark matter equation of state, since it is feasible that some of the stranger gravitational wave observations may have come from QS systems. We find that increasing the Gauss-Bonnet coupling constant α or the interaction parameter λ both tend to increase the mass-radius profiles of QS described by this theory, allowing a given central pressure to support a larger QS in general. Additionally, we analytically identify a critical central pressure, below which no QS solutions exist due to the pressure function having no roots.
We investigate the mutual information harvesting protocol for two uniformly accelerated particle detectors. We numerically show that, while a single detector responds as if it is immersed in a thermal bath, the quantum mutual information between two accelerating detectors behaves differently than that of two inertial detectors in a thermal bath. This is due to the fact that while the Wightman function along the trajectory of a single uniformly accelerating detector is the same as that of as a detector in a thermal bath, a pair of detectors in the same respective cases will have different Wightman functions.
Low-latency detection of Binary Black Hole (BBH) and Binary Neutron Star (BNS) merger Gravitational Wave (GW) signals is essential for enabling multi-messenger observations of such systems. The merger GW signals have changing frequencies and are contaminated by non-stationary noises. Earlier studies of non-templated merger signal detection techniques used traditional Fourier transform-based time-frequency decomposition methods for spectrogram generation, which have had difficulties identifying rapid frequency changes in merger signals with heavy background noise. To address the problem, we introduce the Joint-Chirp-rate-Time-Frequency Transform (JCTFT), in which complex-valued window functions are used to modulate the amplitude, frequency, and phase of the input signal. In addition, we outline the techniques for generating chirp-rate-enhanced time-frequency spectrograms from the results of a JCTFT. We demonstrate an average of 14% improved merger detectability among simulated detector signals with Signal-to-Noise Ratios between 6 and 10 using the InceptionV3 image classification neural network when compared to the same network trained with Q-transform spectrograms. The JCTFT is a general transformation technique that can be applied to existing and third-generation GW detector signals. We aim to analyze the characteristics of the complex window functions through the study of the Wigner distribution and the Fresnel functions.
Post-secondary science courses, including physics, have a role to play in supporting equity and inclusion in STEM. The extent to which our courses have equitable outcomes influences which doors are open or closed, and to whom, and ultimately determines if we can address the need for diverse teams of skilled scientists and citizens to devise and implement effective solutions. The Canadian Consortium of Science Equity Scholars is a cross-discipline, multi-institution group of educators and researchers dedicated to enhancing equity in post-secondary science courses. By examining disaggregated sociodemographic data, we can pinpoint evidence of inequities in achievement and affective outcomes—in disciplinary and social belonging, self-efficacy, and course experience—that may lead to underrepresentation in the field. This research aims to address systemic barriers to student success and uncover ways to foster students’ sense of belonging in physics. In this presentation, I will share preliminary results from the initial year of data collection by the Consortium, highlighting outstanding questions suggested by the results.
The Innovation, Diversity, Exploration, and Advancement in STEM (IDEAS) Initiative is a national EDI-focused outreach program run out of Queen’s University. IDEAS utilizes a multi-generational approach to outreach, aiming to coordinate historically under-represented individuals within STEM in fostering an interest towards the natural sciences in Canadian youths. The IDEAS Initiative has run an extensive collection of outreach programs and events following this mission since 2019.
Volunteer scientists lead experiments, projects, and confidence building activities both in-person and online to encourage development of self-identity and a sense of belonging to STEM within participants. In parallel, the IDEAS Initiative provides opportunities for volunteers to participate in teaching and outreach training workshops as a cornerstone of a network-building objective. This maximizes its impact beyond a local scope as support is offered to projects run by members nationally.
The IDEAS Initiative is a major EDI and outreach arm of both the Arthur B. McDonald Canadian Astroparticle Physics Research Institute and the Queen’s University Department of Physics, Engineering Physics & Astronomy. Teaching philosophy, performance, and prospects of the IDEAS Initiative will be discussed.
While tremendous progress has been made, women and other gender minorities remain largely underrepresented in the Canadian physics community, a problem which first manifests at the high school level. All efforts to narrow the gender gap at the undergraduate level and beyond will continue to be hampered by the lack of gender diversity in students with the necessary prerequisites for a physics degree. Despite this, data characterizing gender representation in high school physics is not widely available. To address this gap we have collected detailed administrative data from all provincial Ministries of Education across Canada. This includes male and female enrolment rates in university-track STEM courses for all publicly funded secondary schools across the country.
In this talk, we will present these data to describe the current gender gap present in high schools across the country. In the past decade, the continuation rate of male and female students from grade 10 science through to grade 12 physics has remained nearly constant, restricting the growth potential of physics departments across Canada. In the same time period, there has been only minimal growth in the median proportion of female students in grade 12 physics. At the current rate of growth, parity in male and female enrolment in high school physics would not happen until ~2100. In contrast, the continuation rates of female students in all other high school STEM courses have increased dramatically, greatly increasing female representation. Efforts to address the gender gap in STEM appear to have been successful – just not in physics.
Because physics is one of few STEM fields that has yet to successfully address its gender and diversity gaps, there is work to be done to encourage different types of people to pursue physics as a degree. Part of the responsibility for this work rests with undergraduate physics professors and teaching staff, whose influence on students is profound. One question that has not been adequately answered in the literature is exactly how physics departments should attempt to increase participation and belonging in physics. I will present a part of my Ph.D. dissertation research that focused on working with undergraduate physics instructors to make changes in their department that we hoped would encourage students to feel welcome, to feel they belonged, to build their physics identities, and ultimately, to increase and broaden participation in the undergraduate program. This in-depth, qualitative case study produced some expected results and some surprising ones. I will make recommendations for you to consider applying in your own contexts, and I hope to hear what has worked for others.
Experiments currently searching for dark matter, studying properties of neutrinos require very low levels of radioactive backgrounds both in their own construction materials and in the surrounding environment. These low background levels are required so that the current and next generation experiments can achieve the required sensitivities for their searches. SNOLAB has several facilities which are used to directly measure these radioactive backgrounds. This presentation will describe the low background measurement facilities currently used to measure these backgrounds, describe the data analysis techniques used and present results from these detectors. In addition, plans and options to expand these facilities to allow for the increased sensitivity required by the next generation of experiments will be described.
Many particle and rare-event search detectors use liquid scintillators as the active detector material. Candidate scintillating fluids include liquid noble elements such as Liquid Argon (LAr) and Liquid Xenon (LXe). Detectors that make use of scintillators hold the fluid inside an acrylic vessel, which can be coated with various films. One common coating is 1,1,4,-tetraphenyl-1,3-butadiene (TPB) which is a wavelength shifter that converts ultraviolet (UV) lighted emitted by the scintillator into visible wavelength wavelengths that are detectable by photodetectors, such as photomultiplier tubes. Another coating of interest is Clevios, an optically transparent conductive organic polymer. One application of this material is to generate a voltage gradient between two electrodes for functionality in a time projection chamber.
The acrylic vessel, coatings, and other detector components can emit undesirable fluorescent and scintillation light that contribute to background signals in the experiment. It is critical that the optical properties of these materials be investigated to support the efforts of such rare-event search detectors. In addition, optical properties of a material change with temperatures, providing a motivation to study such materials at the cryogenic operating temperature of liquid scintillator detectors.
The optical cryostat lab at Queen’s University is well suited to study photoluminescent properties of inorganic scintillators, coatings, and their substrates at temperatures ranging from 300K to 4K. An overview of lab activities to be presented include previously studied samples, data acquisition/analysis, and preliminary results from recent measurements.
nEXO is a next-generation neutrinoless double-beta decay experiment that is searching for this decay in 5-tonnes of liquid xenon (LXe) enriched in the isotope 136Xe. Silicon-photomultipliers have been selected to measure the vacuum ultraviolet (VUV) scintillation light from interactions within the LXe. Although candidate SiPMs from Hamamatsu (HPK) and FBK have been characterised within the collaboration and shown to meet nEXOs performance requirements, the long-term stability of their detection efficiency, gain, and correlated noise under VUV exposure has not been thoroughly reported. To investigate long term effects under VUV exposure, a sample of HPK VUV4 SiPMs were irradiated with a flash lamp. The performance of the SiPMs were then reevaluated following repeated VUV exposure. This process was repeated with increasing dose until exceeding the expected exposure from 10 years of nEXO run time. I will report on the stability of the PDE, gain, and correlated noise for a sample of HPK VUV4 SiPMs following a large dose of VUV radiation.
Liquid xenon (LXe) is frequently employed to build detectors for rare event searches due to many of its advantageous properties including high stopping power, high ionization and scintillation yields, and relatively high cryogenic operating temperature. Time projection chambers (TPC) with LXe allow for 3D event reconstruction and identification which is important for reducing backgrounds. Due to the high drift fields TPCs are operated at, it is crucial to model breakdown properties in LXe. Often, a high voltage (HV) discharge is able to damage the detector instrumentation, e.g., the photo-sensors array. The context for this research is the appearance of HV instabilities on the EXO-200 (0νββ search experiment from the Enriched Xenon Observatory (EXO) collaboration) TPC HV line, accompanied by scintillation VUV light. In our investigation we use a cryogenic setup called EXO-100 capable of purifying and liquifying Xenon, with a TPC modelled after the EXO-200 TPC but specifically designed to study HV instabilities and breakdowns in LXe. In this follow-up presentation, results (based on data collected in EXO-100) are presented displaying the analysis of HV instability pulse waveforms, and some possible origins of these instabilities in LXe.
Ionization chambers are widely used for detecting radiation emitted as a result of nuclear decay, and offer potential for high-resolution energy measurement, particle track reconstruction, and for long-lived isotope lifetime measurements. Presently, they are commonly used for measuring the energy of alpha particles emitted during radioactive decay processes and are also used for fission fragment experiments. When built with a conventional Frisch grid design and waveform digitizing data acquisition system (DAQ), these detectors can recover one of the two spherical angles of emission of a particle via the relationship between signal rise time and the polar angle of emission.
In order to fully characterize the particle track however, the azimuthal angle must also be known. To recover this, it is necessary to build a chamber with a segmented electrode where each segment is connected to an independent amplification system and DAQ channel. When this is done, complete reconstruction in 3D space of the particle track is possible in addition to high-resolution measurement of its energy.
The SCI-CASTER project being developed at the Simon Fraser University Nuclear Science Laboratory aims to achieve full 3D track reconstruction and high-resolution energy measurement of low-rate alpha decay experiments by segmentation of the chamber anode. In principle, this design will also allow for the rejection of events originating from outside the detector volume by analysis of segment signal timing, thereby improving background rejection.
Preliminary experiments using a non-segmented design have been carried out to evaluate the performance of the DAQ and accompanying amplification circuitry. Further, data from a simulated segmented detector has been analyzed to characterize the signals induced on the anode electrodes.
This presentation will outline the design process of the current SCI-CASTER prototype detector system and will discuss results from the non-segmented design, ongoing simulations, and the prototype segmented detector currently under construction.
Lanczos-based algorithms have been demonstrated to play a pivotal role in quantum computing and classical methods. I review the development of these methods for a variety of physical systems and new implementations. I also review new use cases of these algorithms.
London dispersion is a weak, attractive, intermolecular force that occurs due to interactions between instantaneous dipole moments. While individual dispersion contributions are small, they are the dominating attractive force between non-polar species and determine many properties of interest. Standard methods in density-functional theory do not account for dispersion contributions, so a correction such as the exchange-hole dipole moment (XDM) or many-body dispersion (MBD) models must be added. Recent literature has discussed the importance of many-body effects on dispersion, and attention has turned to which methods accurately capture them. By studying systems of interacting quantum harmonic oscillators from first principles, we directly compare computed dispersion coefficients and energies from XDM and MBD. While the results are similar at large separations, MBD is found to be susceptible to a polarization catastrophe at short range. Additionally, the self-consistent screening formalism used in MBD is shown to be surprisingly sensitive to the choice of input polarizabilities. Connection is made to interactions between noble gas atoms, as well as to the methane and benzene dimers, and to two layered materials, graphite and MoS2, for which similar results to the oscillator models were obtained.
We consider a one-dimensional flowing Bose-Einstein condensate (BEC). We numerically model the mean-field wave function of this system, and compare our results to an analytical solution derived using the hydrodynamic approximation. We find that a sonic event horizon forms in the BEC, where in one region the flow of the condensate exceeds the speed of sound in the BEC, while across a boundary the opposite holds. We further introduce wave packets into the BEC to investigate their time evolution.
The discovery of non-thermal behaviour in a thermalizing quantum many-body system [Nature 551, 579-584 (2017)] led to the introduction of quantum many-body scars (QMBS). They are atypical eigenstates of chaotic systems and generally exhibit sub-volume or area law entanglement as opposed to the volume law present in the bulk of the eigenstates. The term, QMBS, was given using heuristic correlations with quantum scars (eigenstates with high probability density around unstable classical periodic orbits) in quantum systems with a semiclassical description. Through the study of entanglement in a multi-qubit system with a semiclassical description, we show that the properties of QMBS states strongly correlate with those of the eigenstates corresponding to the very few stable periodic orbits in a chaotic system rather than unstable periodic orbits in such systems.
We study the model, quantum kicked top (QKT), an experimentally realized, paradigmatic model for quantum chaos. It has a multi-qubit representation in the permutation symmetric subspace that carves a way to calculate entanglement. The QKT exhibits Wigner distribution level statistics, typical of quantum chaotic models, in most of the parameter regime. In permutation-symmetric multi-qubit systems, random states exhibit logarithmic scaling in entanglement. When the system is quantum chaotic, we see that the bulk of the eigenstates exhibits logarithmic scaling in entanglement as expected. Nonetheless, we find a few atypical eigenstates with sub-logarithmic entanglement scaling. Further investigation reveals that these eigenstates have high probability density around stable periodic orbits present in the system despite the system being chaotic. We use the term, QMBS-like state, for such atypical eigenstates with sub-logarithmic entanglement scaling and which have support on stable periodic orbits. Moreover, we find variational quantum states that have close to 99.9 percent fidelity with the QMBS-like states. On the other hand, we find that the quantum scar eigenstates in the system exhibit logarithmic entanglement. Thus, we show that QMBS-like states with support on stable periodic orbits are better analogs of QMBS states in quantum many-body systems. This study would be helpful in understanding the mechanism of non-thermal behaviour (whenever present) in quantum chaotic systems.
This analysis will make a measurement of the inclusive charged current anti-neutrino cross section on hydrocarbon as a function of muon kinematics. This measurement is being made with an unprecedented 1.8 million data events which have been recorded in the MINERvA detector [1]. The goal of the MINERvA experiment is to make high precision cross section measurements on various nuclei. There were 10.7 × 10^20 protons on target in the NuMI beamline [2] yielding a beam of anti-neutrinos with an energy peaking at 6 GeV. A very well constrained flux prediction developed using neutrino-electron elastic scattering and inverse muon decay has been employed to constrain the uncertainty on the anti-neutrino flux. Both single and double differential cross sections in muon transverse and longitudinal momentum are reported. Motivation for making a measurement in these variables stems from great detector resolution for muon kinematics. The cross-section measurements made by the MINERvA experiment will constrain the models that feed into the next generation of experiments which are neutrino oscillation experiments.
[1] Design, calibration, and performance of the MINERvA detector MINERvA Collaboration • L. Aliaga (William-Mary Coll.) et al. DOI: https://doi.org/10.1016/j.nima.2013.12.053 Published in: Nucl.Instrum.Meth.A 743 (2014), 130-159
[2] The NuMI Neutrino Beam P. Adamson (Fermilab), K. Anderson (Fermilab), M. Andrews (Fermilab), R. Andrews (Fermilab), I. Anghel (Iowa State U. and Argonne) et al. e-Print: 1507.06690 [physics.acc-ph] DOI: 10.1016/j.nima.2015.08.063 Published in: Nucl.Instrum.Meth.A 806 (2016), 279-306
Abstract: Water Cherenkov detectors such as Super-Kamiokande are an important detector technology for Neutrino experiments. They consist of large volumes of water surrounded by phototubes that collect Cherenkov radiation created by charged particles. The characteristic Cherenkov ring reveals the particle’s information, like the energy and direction of travel. However, the Cherenkov ring is not a sharp ring, and it is disturbed by scattering, which may lead to getting improper information about the particles. Rayleigh, Mie and Raman scattering, as well as absorption, are microscopic processes which are considered to influence light propagation. The Raman scattering effect is a sub-leading effect relative to the Rayleigh scattering and has not yet been implemented in the GEANT4 optical photon model. It is an inelastic scattering of light by molecules which shifts the wavelength of light. In this work, the wavelength shift of Raman scattered light is investigated using the Monte Carlo method. Also, the total number of photoelectrons detected by PMTs is calculated, which shows the relative scale of the Raman scattered photon compared with Rayleigh scattering for two different pathlengths of light, the Hyper-K and the Super-K water tank diameters. The Results predict the probabilities of different outgoing wavelengths for an incident photon wavelength as well as the size effect of the Raman scattering compared with the Rayleigh scattering in large detectors, which is not negligible. All in all, this work indicates that the Raman scattering effect needs to be implemented in the GEANT4 simulation as the calculations show considerable values for that.
The DEAP-3600 experiment is a single-phase liquid argon dark matter experiment that uses scintillation light to look for weakly interacting massive particles (WIMPs). In addition to the dark matter search, the detector’s properties including low background and argon medium make it a good candidate for a first observation of 8B solar neutrino charged-current interactions on 40Ar. Solar neutrinos with sufficient energy, like 8B neutrinos, interacting with 40Ar may produce an excited state of 40K that will deexcite in a series of gamma rays. We present an overview of the ongoing solar neutrino absorption study in DEAP-3600 with a discussion of the analysis strategy.
The NEWS-G experiment searches for low-mass dark matter candidates at SNOLAB in Sudbury, Ontario. The direct dark matter search is performed using a spherical proportional counter (SPC) filled with light atomic mass gases. NEWS-G3 is a proposed experiment that employs the same technology as the NEWS-G experiment to search for coherent elastic neutrino-nucleus scattering (CEνNS) at a nuclear reactor. NEWS-G3 will consist of a 60-cm high purity copper SPC implemented in a compact shield consisting of many different layers of material. One layer of shielding is an active muon veto system consisting of plastic scintillators coupled with a photomultiplier tube (PMT). In this presentation, I will present the current status of the NEWS-G3 experiment at Queen’s University and the commissioning of the muon veto system. I will also discuss the results of my undergraduate thesis of the background decomposition of the NEWS-G3 experiment.
PICO-500 is a large scale bubble chamber WIMP dark matter detector in its early stages of construction underground at SNOLAB. The detector will contain ~250 litres of superheated C$_3$F$_8$ (freon) contained between two quartz jars. The quartz jars will sit inside a pressure vessel filled with mineral oil that will control the pressure of the active freon volume. The entire detector will be housed inside a tank of ultrapure water. PICO-500’s detection method is based on the Seitz model, in which nuclear recoiling of freon from an incoming particle results in localized boiling if the energy deposition, within a critical radius, is in excess of the Seitz threshold energy. The operating Seitz threshold of PICO-500 will be optimized for dark matter sensitivity and gamma and electron insensitivity. Muons will be vetoed using strings of photomultiplier tubes around the edges of the water tank to detect their Cherenkov light. Alphas will be discriminated from dark matter signals by the acoustic parameter (AP), which describes the acoustic power of the bubble formation, and is larger in alpha events than neutron or WIMP events. Calibration of the Seitz threshold will be done by lowering a $^{60}$Co gamma source into the detector through 3 separate source tubes, 2 of which feed into the water tank, and 1 of which feeds into the pressure vessel. AP calibrations will be done using runs with AmBe and/or $^{252}$Cf neutron sources. This talk will give an overview of PICO-500 and the methods of calibration.
Laser applications at TRIUMF's isotope separator and accelerator facility for (i) laser ion source use and (ii) nuclear spin polarization and (iii) measurement of nuclear moments and chang3s in nuclear mean square charge radii will be presented and discussed.
Microchip single mode lasers capable of high output powers are paramount for use in photonic integrated circuits, light detection and ranging (LIDAR) for the automotive industry and remote sensing in general. Of the many developments done to miniaturize single mode lasers, we take interest in parity-time (PT) symmetric lasers. These types of lasers rely on the interplay between the gain and loss of micro resonators to obtain single mode emission. Our proposed laser architecture exhibits PT-symmetric behavior in the polarization space. To control the polarization eigenstates of our laser, we use a pair of nanostructured mirrors consisting of an inscribed diffraction grating on the top layer of a Bragg mirror to obtain a phase shift of π and a difference in reflectance between transverse electric and magnetic polarization states. The addition of a phase shift on the mirrors provides control of the amplitude of the standing wave inside the resonator by changing the relative angle (α) of the two mirrors' principal axes. Thus, suppressing multiple longitudinal modes emission arising from spatial hole burning. Moreover, with the addition of a difference in attenuation between the mirrors' two principal axes, the polarization eigenstates of this laser are no longer orthogonal and for a specific angle of (α), they merge into one eigenstate called an exceptional point. Experimental results reveal enhanced purity of the emission spectrum compared to a resonator with conventional mirrors.
Producing neutral-atom Bose-Einstein condensation, despite being a routine procedure, remains susceptible to experimental imperfections. In order to reach the condensation of widely used atomic species such as rubidium, researchers require ultrahigh vacuum, high current sources, and stable, precision lasers. The BECs are sensitive to residual magnetic fields, low-power scattered resonant light, and even to the humidity of a room. Despite best efforts, we observed a significant atom number drift in our system with different timescales. Due to the process being divided into many temporal steps and multiple independent parameters associated with different cooling mechanisms, we were unable to identify some causes of the drift.
To address the problem of atom number drift in our system over varying time frames, we installed several sensors to track changes in the environment. The high dimensionality of the parameter space prompted us to use a multilayer neural network to identify all the underlying relationships. The trained neural network was successful in predicting atom number drifts.
With a neural network that predicts the atom number, we extend the work to correct for the instabilities.We created a second list of parameters, which could be controlled externally, and we started exploring it with Gaussian processes [1]. We concluded that it was crucial to combine two learning models: one of them has access to control parameters but does not account for drift (gaussian optimizer), while the second one was slower and thus not suited for real-time use, but could account for external parameter drift (neural network). We optimized this dual learning algorithm for our system and explored the parameter space to achieve optimal BEC production under a wide range of parameter settings, allowing our experiments to collect high-quality data continuously.
We describe a low cost, simplified setup for creating a large-gain four wave mixing system in atomic Rubidium. By utilizing recent low cost, high power laser diodes and in-house construction, we have developed a system for producing narrowband, states of light in a high optical gain system.
Such systems have previously demonstrated intensity squeezing, EPR entanglement, and high purity Fock states, albeit at much higher cost.
This work can help open the door to smaller budget experimental groups as well as undergraduate teaching labs.
Inelastic light scattering allows one to transfer energy from light to a system. Tracking the absorption provides clues about the allowed energy states in the system. The strongest signatures in such a spectrum usually come from the collective modes excited in the system. In this talk I will present new collective modes in spin-orbit coupled (SOC) systems, called the chiral-spin waves, and how they can be studied using resonant electronic Raman scattering, a form of inelastic light scattering. This discussion is relevant to a wide variety of quantum materials such as quantum wells, topological insulators, 2D Vanderwaal’s structures and even giant-Rashba SOC materials. The presence of spin-momentum locking in SOC systems also provides an enhanced coupling of light to certain charge excitations such as plasmons. I will present the unifying theory behind all these effects and provide the corresponding experimental evidence.
An exact analytical expression for the probability of photon reabsorption and recycling in an idealized solar cell with Lambertian surfaces is derived. The existing approximations are found to agree with the exact formula to within a few per cent. The most accurate approximation turned out to be the simplest one that sets the reabsorption probability to the weak-absorption limit of the cell absorbance. The maximal photoconversion efficiency of a silicon solar cell is evaluated to be 29.5 % at the base thickness of 98 $\mu$m in a cell whose front and rear surfaces are Lambertian.
In this project, we explored the fabrication of SiGe quantum dots (QDs) in a silica matrix by ion implantation. Ion implantation is an important fabrication tool in the semiconductor industry, and can be used to make compounds beyond the chemical solubility limit and allows the study of a range of concentrations of Si and Ge. The relative concentration of Ge in SiGe alloys has a direct influence on the bandgap, and by changing the Ge content, different emission wavelengths can be achieved and adjusted according to the requirements of applications. As an initial step, samples were implanted with Si+ at 40 keV into a 1 μm thermally-grown SiO2 film on a Si (001) substrate to achieve a peak concentration of 17.5 at. % with respect to SiO2. The implantation energy placed the implanted Si peak 50 nm below the surface. Samples were subsequently implanted with 55 keV Ge+ with 0.5-7.0 peak at. %, giving the same implantation depth as Si, and thermally annealed to promote cluster growth/crystallization. For the second set of samples, Ge+ implantation was done after 1100oC annealing, necessary for Si QDs growth. Our photoluminescence (PL) results indicate that emission peak positions and intensity depend strongly on the fabrication sequence. Both sets of samples present emission around 780 nm and 1050 nm. We observe that PL intensity decreases in both sets of samples when the Ge amount is increased, and the sample with no annealing between the implants exhibits more intense PL. Time-resolved PL revealed dynamic behaviour with at least two time constants, both in the 100-700 microsecond range, with longer lifetimes for higher Ge concentrations. Raman spectra (Ge-Si peak at 405 cm-1) revealed that Ge incorporation in Si QDs is detected only in the sample with Ge content of 7.5 peak %.
The long-term objective of this project is to develop cost-effective, versatile, and scalable, short-wave infrared detectors directly integrated into silicon. Unlike the direct bandgaps materials such as Si, Si1-xGex, and Si1-x-yGexSny provide a promising path toward Si-compatible devices for SWIR detection. In this project, Si (001) samples were implanted at room temperature with a tilt of 7 degrees, with 65keV Ge and 100 keV Sn at the Tandetron Accelerator lab, Western University, to achieve average Si0.80Ge0.15Sn0.05 concentrations over the top 100nm. After implantation, the samples were furnace-annealed at 400oC, and 600oC, for 30 minutes, in dry nitrogen gas, leaving one as ‘as is’ for comparison. Aluminum metal contacts were deposited at the surface of selected samples using lithography process for IV measurements, with Al round contacts of a diameter of 600 µm, 700 µm apart (Western Nanofab). Spectral response (SR), quantum efficiency (QE), current density, and the current-voltage (IV) characterization were performed on selected samples at Sciencetech Inc. In our IV measurements at room temperature, we found that the IV curves can be divided into three regions, Region 1, where we see the reverse bias current, which is the small leak current. In Region 2, Si1-x-yGexSny materials exhibit Ohmic behavior. And finally, Region 3 where the current does not change with voltage, this region operates like an ideal current source. More so, this IV curve passes through the origin, implying that it does not store energy. We see an interesting observation, in Region 2, the IV characteristic curve showed an increment in the current with respect to the voltage with the increase in the degree of annealing on the sample. All studied samples have maxima in the SR and QE responses at around 1099nm, and a broad plateau at 1600-1980 nm, respectively. Along with this, there is a slight incremental shift in the long wavelength of the spectral response for the annealed samples. Overall, there was a decrease in the maximum SR, QE, and current density of samples annealed at high temperatures, compared to asis sample.
The discovery of the lepton-number-violating neutrinoless double-beta decay process will prove that neutrinos are Majorana fermions. The Large Enriched Germanium Experiment for Neutrinoless double-beta Decay (LEGEND) project will search for this decay in $^{76}\mbox{Ge}$. In its first phase — LEGEND-200 — $200~\mbox{kg}$ of $^{76}\mbox{Ge}$-enriched high-purity germanium detectors will be deployed in a liquid-argon cryostat. It is under construction at the Laboratori Nazionali del Gran Sasso (LNGS) in Italy. The first phase has a background goal of <0.6 counts/(FWHM t y), which yields a 3σ half-life discovery sensitivity beyond $10^{27}$ years. The second phase — LEGEND-1000 — will comprise 1000 kg of enriched germanium detectors. It will be sited deep underground with SNOLAB as the baseline host. LEGEND-1000 will have a discovery sensitivity beyond $10^{28}$ years. In this talk, I will give an overview of the LEGEND project.
The light-only liquid xenon (LoLX) experiment is a small-scale liquid xenon (LXe) detector with cutting-edge photo-detection technology. LoLX is designed to characterize the performance of silicon photomultipliers (SiPMs), and to study light emission, transport, and detection in LXe to inform future LXe rare-decay detectors. LoLX consists of 96 Hamamatsu VUV4 SiPMs arranged in a cylindrical geometry and submerged in LXe. This R&D detector is used to investigate the timing structure of light production processes like scintillation and Cherenkov radiation in LXe, and to provide better understanding of SiPM external crosstalk between neighboring SiPMs and its effect on the overall detector performance.
When photons are detected by a SiPM, photodiodes undergo an avalanche process, from which secondary photons can be produced. In a process called SiPM external crosstalk, these photons can reach other SiPMs and produce correlated hits on nearby devices. Characterizing the SiPM pulse shape and correlated noise contributions allows for accurate and reliable reconstruction of photons, which is needed to improve the energy and timing resolution of our response model for photon detection. To reconstruct photon signals, we have developed an improved pulse-fitting algorithm that constructs a functional form of the pulse shape. I will present on the functioning of the fitter, its performance, and compare it to other photon-counting algorithms, in particular, to a traditional pulse-finding algorithm with respect to improving energy resolution.
Neutrinoless double beta decay is a proposed nuclear transition involving the emission of two electrons with no neutrinos. In $^{136}$Xe, observing the $^{136}$Ba daughter directly is a positive detection of double beta decay. This is barium tagging, and it would significantly enhance the signal to background ratio in experiments using a liquid xenon time projection chamber. However, extracting a single ion inside of a large cryogenic environment requires rapid and accurate motion of an ion collection probe. For this reason, we have developed a fine motion control apparatus to reliably position a thin capillary probe which enables the extraction and transport of single ions. I will present my work on the design and construction of the displacement apparatus along with studies on its ion extraction efficiency.
Studies of short-lived radioactive isotopes, at the limits of nuclear binding (the “drip lines”), are crucial for understanding how the nuclear force evolves toward the extremes. In neutron-deficient nuclei, measurements of β-delayed proton emission can be used to constrain proton-capture reaction pathways in nucleosynthesis and test isospin symmetry. In this talk, I will present my analysis of the proton drip-line nucleus, $^{22}$Si, from a β-delayed proton decay spectroscopy experiment performed at the National Superconducting Cyclotron Laboratory (NSCL). My analysis involved determining proton energies, proton intensities, and calculating β-decay branching ratios. I will discuss the results of several newly discovered energy states in the daughter nucleus, $^{22}$Al. To develop a similar experimental program here in Canada, our group at the University of Regina is building a novel silicon strip detector array that will be coupled with the Gamma-Ray Infrastructure For Fundamental Investigations of Nuclei (GRIFFIN) facility at TRIUMF. An overview of the detector design, construction, and future plans will be presented.
I'll discuss the motivations for sub-GeV dark matter scenarios, and review progress over the past decade in accelerator-based searches.
Investigating neutrinos’ helicity flip that could be caused by the curvature of spacetime becomes more involved when the neutrinos are, in addition, allowed to couple to a scalar field. It is, nevertheless, of great importance to investigate such a possibility if one wishes to keep up with multi-messenger astronomy and explore novel ways of bringing into evidence any eventual existence of cosmological scalar fields in Nature. I will discuss neutrinos’ helicity flip within well-known screening models from the literature, such as the chameleon and the symmetron models. Technical subtleties will be pointed out, and the main difficulties one encounters when dealing with rotating gravitational sources will be exposed.
Muons are elementary particles with a finite lifetime, and their self-energy describes the interaction between a muon and the surrounding electromagnetic field. Accurate determination of the muon self-energy is essential for precision tests of the electroweak sector of the Standard Model and for probing new physics beyond the current model. In this study, we utilized the Marty program to calculate the muon self-energy at a one-loop level within the Standard Model. Our study contributes to the understanding of the muon self-energy and highlights the usefulness of Marty as a computational tool for particle physics calculations.
Microvascular stalling, the process occurring when a capillary temporarily loses perfusion, has gained increasing interest
in recent years through its demonstrated presence in various neuropathologies. Despite efforts trying to
study the stalling events, investigations are hampered by their elusiveness and scarcity. In an attempt to alleviate these
hurdles, we present here a novel methodology enabling transient occlusions of targeted microvascular segments through
multiphoton excitation of Rose Bengal, an established photothrombotic agent.
The increasing availability of high-intensity radiation via synchrotron light source facilities has revolutionized paleontology research in the last couple decades. Synchrotron techniques are often non-destructive, allowing thorough imaging and chemical analysis of fossils without damaging precious specimens. Hard tissue skeletal remains such as bones and teeth have long been the only source of information about ancient creatures that lived over 66 million years ago. However, while much more rare, soft tissue structures and remains of original organic material can be preserved in deep time, and they can provide a more lifelike reconstruction of ancient ecosystems.
Here, using a suite of high-resolution imaging and chemical analysis techniques performed at the Canadian Light Source (CLS), a vast network of blood vessels has been characterized inside a rib bone from a specimen of Tyrannosaurs rex. The techniques used include micro–Computed Tomography (μ-CT), X-Ray Fluorescence (XRF), X-Ray Absorption Near Edge Structure (XANES), as well as Scanning Electron Microscopy (SEM). The vessels were found to be composed predominantly of goethite, an iron (III) molecule that has been associated with exceptional preservation in previous studies. This specimen, nicknamed Scotty, famous for being the largest T. rex ever uncovered, was found in a Late Cretaceous (67-66 Ma) deposit of southwestern Saskatchewan, Canada. Scotty is known to have sustained many injuries, including a fracture on the rib bone of interest. We suggest that healed injuries may provide a target for future studies of soft tissue preservation in dinosaurs. This research can also help us construct the pathway of physical, chemical, and biological processes that led to the exceptional preservation of Scotty.
Elastography is a growing area of research in which certain imaging modalities, such as magnetic resonance imaging (MRI), are employed to measure the response of materials to external stress allowing for quantitative estimation of viscoelastic properties. This has tremendous potential in a clinical setting, as changes in tissue viscoelasticity can be indicative of myriad health conditions. Although informative, the long-term clinical viability of conventional magnetic resonance elastography (MRE) techniques may be limited by the requirement of large and expensive MRI scanners and complex acquisition/processing schemes.
Growing trends toward the use of portable, low-field magnetic resonance (MR) instruments in specific, targeted applications motivate the development of portable MRE techniques. For motion encoding, the configuration of several small permanent magnets can be optimized to provide a region with a constant gradient. This “sensitive volume” serves as an integrator, encoding information on the spatial distribution of velocities within the region of interest through modulation of signal due to phase interference.
In past work, we have demonstrated that a constant gradient portable magnet array can be employed to detect longitudinal waves, allowing for relative measurements of viscoelastic properties. Current research is focused on extending this research to detect shear waves, where changes in viscoelastic properties influence the velocity distribution and amount of phase interference within the sensitive volume. Various experimental parameters can be adjusted to regulate phase interference and extract information on the wavelength present in the sensitive volume. Several approximations and limiting cases used in the signal analysis will be discussed, and experimental results depicting the dependence of MR signal on shear wavelength will be presented. Relatively fast measurement times, combined with the portability (a shoebox size) of the setup, and other advantages associated with portable MR, make for promising practical applications of the methodology.
Dielectric Wall Accelerators (DWAs), which coordinate high-gradient, nanosecond electric field pulses with particle bunch trajectory, may be suitable as compact accelerators for proton therapy. Parallel plate waveguides (PPWGs) have been proposed as a means of generating the electric field pulses. This work is a study of annular PPWGs, where electrical impulses applied at the outer radius propagate radially and produce electric fields at the inner radius (i.e. the beampipe). Radial propagation of the signal introduces distortions which must be quantified to 1) design upstream circuits that produce a suitable electrical impulse and 2) select the geometric and material properties of the PPWG. The design choices are made to produce a time-varying electric field at the beampipe that maintains longitudinal beam stability.
The electromagnetic fields of a PPWG were derived in cylindrical coordinates assuming radial propagation and axial symmetry. For TEM modes, the electric field is:
\begin{align}
\mathbf{E} &= \frac{\beta_s }{i\omega \varepsilon} \left[\kappa_1 J_0(\beta_s s) + \kappa_2 Y_0(\beta_s s)\right] \hat{z}; & \beta_s = \omega\sqrt{\varepsilon\mu},
\end{align}
where $\omega$ is frequency, $\varepsilon$ is permittivity, $\mu$ is permeability, $\kappa_1$ and $\kappa_2$ are constants, $J_0$ and $Y_0$ are Bessel functions, and $s$ is radial distance. By comparing field magnitude at the inner and outer radii, one obtains an expression for frequency-dependent amplification.
Various PPWG configurations were modelled in COMSOL Multiphysics and excited at the outer radius with a Gaussian pulse. The frequency response was measured by comparing the spectra of the input and output pulses. Numerical PPWG simulations with impedance-matched inner boundary conditions were compared to results obtained from the field equation.
Agreement between theory and simulation indicates that at lower frequencies (<10GHz), $\omega$, $\varepsilon$, $\mu$, and radii all affect amplification, while at higher frequencies, amplification increases to a plateau determined exclusively by the two radii of the annulus. Plate separation has no effect on amplification for the studied TEM mode, but affects higher order mode activation. A mismatched impedance at the beampipe leads to deviation from theory. Future work will study physically realistic, time-dependent (due to particle transit) beampipe impedance. Additionally, experimental validation and collaboration with colleagues in beam physics and circuitry design will help to identify suitable PPWGs for use in DWAs.
Decide Competitors for Thurs. PM.
Join us for a short summary of the latest NSERC news and a brief overview of the 2023 Discovery Grant competition results. NSERC staff and the physics evaluation group Chair will be on-hand to answer questions. The CAP-NSERC Liaison Committee Chair will also provide an overview of committee activities in the last year and can answer questions.
Veuillez vous joindre à nous pour un résumé des dernières nouvelles du CRSNG et un aperçu des résultats du concours 2023 des subventions à la découverte. Le personnel du CRSNG et la présidente du groupe d’évaluation de physique sera sur place pour répondre aux questions. Le président du comité de liaison CAP-CRSNG donnera aussi un aperçu des activités du comité pendant la dernière année et pourra répondre aux questions. À noter que la présentation sera en anglais mais vous pouvez poser des questions dans la langue officielle de votre choix.
The concept of vibrational modes of excitation of the nuclear surface, known as phonons, was developed in the early 1950s by A. Bohr and B. Mottelson within their collective model. The observed pattern of level excitation energies and spins for nuclei believed to have a spherical shape appeared consistent with the picture of multiphonon excitations. With the confirmation of the collective natures of these states, this picture of spherical nuclei possessing nearly harmonic multiphonon states become standard textbook material – a practice which continues to this day. Over the past couple of decades, we have performed very detailed spectroscopic studies of the cadmium isotopes that revealed serious discrepancies with the multiphonon picture, ultimately developing an alternative interpretation that the excited states were based on multiple deformed shapes that could rotate, rather than a spherical shape that vibrates. This has inspired investigations by many groups around the world to test our interpretation, and a realization that the simple picture presented in textbooks needs to be modified.
CINP Board meeting
The Super Cryogenic Dark Matter Search (SuperCDMS) experiment uses silicon and germanium calorimeters operating at cryogenic temperatures to search for dark matter interactions. In recent years, SuperCDMS HVeV (high voltage with eV resolution) detectors have enabled searches for sub-GeV dark matter candidates coupling to either nuclei or electrons such as low mass Weakly Interacting Massive Particles, dark photons, and axion-like particles. HVeV detectors are equipped with transition-edge sensors (TESs) connected to superconducting aluminum fins to achieve high-resolution athermal phonon sensing. The excellent phonon resolution enables single-charge sensitivity by applying an electric field across the crystal to achieve phonon-based charge amplification via the Neganov-Trofimov-Luke (NTL) effect. In this talk, I will present the performance of a newly commissioned 1-gram silicon HVeV detector operated at the NEXUS (Northwestern EXperimental Underground Site) facility hosted at Fermilab (Batavia, IL).
Radon is the limiting background in many leading dark matter and low energy neutrino experiments. One way to mitigate radon background is to fill external experimental components with a clean cover gas such as N2. At SNOLAB, the radon concentration in the experiments cover gas system is monitored using a radon assay board. To improve the sensitivity of gas assays a new trapping mechanism is developed. This talk will present the current status of this mechanism and the sensitivity of the radon board after its installation.
We present new Big Bang Nucleosynthesis (BBN) limits on the cosmic expansion rate or relativistic energy density, quantified via the number $N_\nu$ of equivalent neutrino species. We use the latest light element observations, neutron mean lifetime, and update our evaluation for the nuclear rates d + d → $^3$He + n and d + d → $^3$H + p. Combining this result with the independent constraints from the cosmic microwave background (CMB) yields tight limits on new physics that perturbs $N_\nu$ and the baryon-to-photon ratio $\eta$ prior to cosmic nucleosynthesis: a joint BBN+CMB analysis gives $N_\nu$ = 2.898 ± 0.141, resulting in $N_\nu$ < 3.180 at 2$\sigma$. The strength of the independent BBN and CMB constraints now opens a new window: we can search for limits on potential changes in $N_\nu$ and/or $\eta$ between the two epochs. The present data place strong constraints on the allowed changes in $N_\nu$ between BBN and CMB decoupling; for example, we find -0.708 $
The MINERvA experiment was designed to measure neutrino-nucleus interactions using the NuMI beam at Fermilab. Between 2013 and 2017, 12x10^20 protons on target were delivered both in neutrino and antineutrino modes with an average neutrino energy of 6 GeV, providing a high statistics neutrino interaction data sample. Among neutrino interactions, a significant primary charged current process is pion production. While charged pions can be detected by ionisation-induced scintillation, as neutral particles, π0 can only be detected from their decay into two photons producing two separate gamma showers. The reconstructed gammas are then used to reconstruct the π0 kinematics. This talk will present the different neutral pion analyses in the MINERvA scintillator tracker, as well as passive iron and lead targets with <Eν> at 6 GeV. This talk will also present a machine learning based semantic segmentation gamma selection, relying on the high statistics of the plastic scintillator.
Various forms of astrophysical evidence indicate the existence of Dark Matter (DM) which is predicted to account for about 85% of the matter in the universe. Our solar system moves through the hypothesized DM halo in our galaxy and many experiments pursuing different detection approaches are trying to observe the resulting DM particle flux.
Among them, SuperCDMS is a direct detection DM experiment presently being constructed at the SNOLAB underground facility in Sudbury, Canada. It will make use of cryogenically cooled Germanium and Silicon crystals equipped with sensors in different designs, which are interleaved Z-dependent Ionization and Phonon (iZIP) detectors and High Voltage (HV) detectors. The iZIP detectors can measure both ionization and phonon signals, allowing the distinction between electron recoils and nuclear recoils. While the former is typically induced by background events, the latter can be caused by DM particles, in particular so called WIMPs. With that recoil discrimination ability, a separation between background and signal is possible which helps to improve sensitivity for WIMPs. HV detectors operate with a larger voltage bias in order to accelerate charge carriers created by ionization, and only measure the resulting amplified phonon signal. Despite not having recoil discrimination ability, it empowers a much better resolution and a comparatively low energy threshold that opens the DM search to lower mass regions.
Ultimately, the complementary approach of the different crystal materials and detector designs enables a broadband DM search for particles with masses $\le 10$ GeV/c$^2$, scanning the parameter space down to unprecedented cross sections.
This talk will cover the current status of the SuperCDMS experiment, explain the detector designs and their working principles, and present discovery prospects at SuperCDMS SNOLAB.
Leading cosmological surveys and models provide strong indications for cold Dark Matter (DM) being one of the major constituents of our Universe. There are many experimental efforts utilizing highly sensitive, low-background detectors with the goal of observing the hypothesized flux of DM halo particles streaming through the Earth.
The SuperCDMS experiment will employ two types of state-of-the-art cryogenic Ge and Si detectors capable of detecting sub-keV energy depositions from potential DM interactions. In order to extend the sensitivity to lower experimental thresholds and DM masses below 10 GeV/$c^2$, a precise understanding of the detector response down to the semiconductor bandgap energy of $\mathcal{O}$(eV) is required.
One of the key techniques to interpret data from test facilities operating SuperCDMS prototype detectors and guiding the development of new devices is to perform comprehensive Monte-Carlo simulations of the involved detector physics. The SuperCDMS Detector Monte-Carlo (DMC) framework is based on the GEANT4 Condensed Matter Physics (G4CMP) package. This package adds phonon and charge modeling in solid-state crystals -- including electron and hole propagation, phonon and charge carrier scattering, as well as phonon emission by accelerated charge carriers -- on top of GEANT4's particle physics and solid-state detector response. Moreover, our DMC framework facilitates modeling of the sensor physics and readout electronics of our cryogenic detectors.
This talk will present an overview of our phonon and charge sensor based detector technology, the key aspects of G4CMP and recent achievements in modeling SuperCDMS prototype detectors with our DMC framework.
Quantum resource theories are a powerful framework for the quantification of resourcefulness in the quantum world. They arise naturally whenever one has a restriction on what one can do on a quantum system. However, the idea behind them is very general, and can be successfully exported to non-quantum scenarios. After introducing quantum resource theories and their mathematical framework, I will present some situations in which we can learn something new from their application to a non-quantum setting, e.g. to statistical mechanics in arbitrary physical theories and to discrete dynamical systems.
I show, within the Group Field Theory (GFT) approach to quantum gravity, how cosmological physics emerges from the collective behavior of spacetime quanta, in what can be understood as the hydrodynamic limit of the underlying quantum gravity theory. In particular, I discuss explicitly how two of the most important challenges in quantum gravity (the problem of the continuum limit and the problem of time) are explicitly addressed in this framework. I finally review and summarize the main properties of the emerging quantum cosmological physics, emphasizing in particular: the initial singularity resolution into a quantum bounce; the presence of an alternative, purely quantum geometrical, inflationary mechanism; and the impact of quantum gravity effects on the dynamics of cosmological perturbations.
The field equations of scalsr-tensor and viable'' Horndeski gravity can be written as effective Einstein equations with an effective dissipative fluid as a source. It is miraculous that this effective fluid obeys the constitutive relations postulated in Eckart's first-order thermodynamics, allowing one to introduce atemperature of gravity'' that describes how alternative gravity approaches, or departs from, Einstein gravity. Recent progress on this first-order thermodynamics will be reviewed.
We present the utility of chains defined on causal sets in estimating continuum properties like the curvature, the proper time and the space-time dimension through a numerical analysis. In particular, we show how right continuum properties emerge in deSitter and FLRW spacetimes.
We also discuss a possible test of manifoldlikeness by considering two models of non-manifoldlike causal sets. This is a part of a broader idea of the geometrical reconstruction of continuum properties given a discrete sub structure, in this case the causal set.
In an infinite-dimensional Hilbert space it is possible to implement the Conjugate Gradient (CG) method to find the ground state eigenvectors and eigenvalues of a Hermitian operator H with sufficiently sparse matrix elements in a particular basis. Several different functions on the state vector can be minimized to achieve this goal.
To find excited eigenvectors and eigenvalues of operator H is non-trivial due to its infinite-dimensional representation. In this talk several approaches to determining excited state eigenvectors and eigenvalues of H using the CG method will be illustrated. The first approach will be based on the method's preservation of symmetry of the initial state chosen. The second approach will involve an iterative application of the CG method to operators of H that have been successively reduced using previous eigenvalue/vector determinations. Inspired by the properties of a multi-particle quantum state of identical fermions, the final approach will apply the CG method to a function acting on states in an antisymmetrized tensor power (n) of the original Hilbert space to simultaneously find the n lowest eigenvalues and eigenvectors of H with a single application of the CG method.
The approaches will be illustrated with one-dimensional quantum mechanical examples where H is a time-independent Hamiltonian of a single-particle system. Mitigation of the effects of numerical approximation in the CG method will be considered.
High precision measurements of the ft values for superallowed Fermi β decays are crucial for providing stringent tests of electroweak theory and constraining possible new physics beyond the Standard Model. To achieve this goal, ft values for these decays must be determined experimentally to ± 0.10% or better. In this work, a high-precision half-life measurement, one of the key ingredients for determining the ft value, was performed for the superallowed Fermi β+ emitter 14O at TRIUMF’s Isotope Separator and Accelerator (ISAC) facility. This work represents the first high-precision experiment using the Gamma-Ray Infrastructure for Fundamental Investigations of Nuclei (GRIFFIN) spectrometer. In this talk, I will discuss new results for the half-life of 14O that were obtained by gating on 2.3-MeV γ-ray photopeaks and including corrections for detector pulse pile-up effects and dead-time losses. The results obtained will be compared to a previous high-precision half-life measurement that employed direct β counting techniques.
As one moves away from stable isotopes and deeper into the neutron-rich region, the likelihood of β-delayed neutron (βn) emission decay increases. The ability to understand the neutron emission probabilities and the neutron energy spectrum can reveal details of the nuclear structure that a conventional β-decay study using only γ-ray detection cannot. We propose to build the Detector Array for Energy Measurements of Neutrons (DAEMON) that will employ the time-of-flight technique to enable high-resolution energy measurements of the neutrons emitted following βn emission. The initial trials, performed at the University of Guelph, testing the rudimentary geometries of EJ200 plastic scintillators and various electronic parameters of silicon photomultiplier (SiPM) arrays for the foundation of DAEMON will be presented. Upon successful comparison of data taken with γ sources with GEANT4 simulations, the DAEMON prototype will be tested with monoenergetic neutron beams at the University of Kentucky Accelerator Laboratory. Used in conjunction with the GRIFFIN Decay Station at TRIUMF in Vancouver, BC, DAEMON will enable βn studies not currently feasible at the facility, initiating a road to strong international collaborations. From shaping the abundance curve of the astrophysical rapid neutron capture process, as well as controlling the neutron induced fission in nuclear reactors, a broad range of applications will be addressed through improved knowledge of the neutron emission spectrum that this new detector will bring.
One of the challenges faced while studying the nuclear many-body problem is the nature of the nucleon-nucleon interaction. In recent decades, models for the nucleon-nucleon interaction were produced from a power counting expansion in Chiral Effective Field theory (EFT). As a result, these modern nuclear interactions have an advantage over previously used phenomenological potentials, since they have a connection to the symmetries of the underlying theory of QCD [1]. To investigate the nuclear many-body problem, we employ an ab initio approach. Quantum Monte Carlo (QMC) consists of a family of powerful stochastic methods for solving the many-body Schrodinger equation [2]. QMC methods provide very accurate results, at the cost of being computationally expensive. In addition to their accuracy, QMC methods have the benefit that we can build the appropriate physics, such as pairing, directly into them. Combining these two tools, non-perturbative QMC methods and the perturbative Chiral-EFT derived nucleon-nucleon interaction, leads to an obvious contradiction. Historically it has been very difficult to calculate perturbative corrections higher than first order in most ab initio methods. However, our recent work [3] has made significant progress in calculating the second-order perturbative correction in a QMC context. To show this, we explore a variety of low-density neutron matter systems that have a direct application to neutron-rich systems such as the inner crust of neutron stars. In addition, we also apply this new method to probe the perturbativeness of modern chiral EFT potentials and discuss the implications for nuclear many-body physics.
[1] R. Machleidt and D.R. Entem, Chiral Effective Field Theory and Nuclear Forces, Phys. Rep. 503, 1 (2011).
[2] J. Carlson et al., Quantum Monte Carlo Methods for Nuclear Physics, Rev. Mod. Phys. 87, 1067 (2015).
[3] R. Curry et al., Second-Order Perturbation Theory in Continuum Quantum Monte Carlo Calculations, arXiv:2302.07285, (2023).
Nuclear theories often operate under the assumption that the strong nuclear force is charge independent. As a result, it is expected that mirror nuclei, which are identical under the exchange of total number of protons and neutrons, will have similar nuclear structures when Coulombic contributions are considered. Under the assumption of charge independence, protons and neutrons are grouped together as nucleons which differ only by their isospin quantum number. However, the charge dependence of the strong nuclear force creates isospin non-conserving interactions which give rise to quantities like Mirror Energy Differences in analogous excited states for mirror nuclei which cannot be accounted for by Coulombic forces. Building a deeper understanding of isospin non-conserving interactions and how they affect nuclear structure will allow for more robust predictive powers in nuclear theories.
In order to explore the charge dependence of the strong force, a stable $^{20}$Ne beam experiment to produce $^{55}$Co was conducted at TRIUMF, Canada’s national particle accelerator centre, with an approved complimentary radioactive $^{21}$Na beam experiment for production of $^{55}$Ni, which is $^{55}$Co's mirror nucleus. These experiments are conducted using TRIUMF’s TIGRESS detector array for gamma-ray detection, SFU’s TIGRESS Integrated Plunger for charged particle detection, and $^{40}$Ca targetry. The $^{55}$Co experiment used a thick target to employ the Doppler-Shift Attenuation Method, while the approved $^{55}$Ni experiment will use a thin target to take advantage of TRIUMF’s ElectroMagnetic Mass Analyzer for measurement of the A, Z, and energy of residual nuclei which enhances the selectivity of reaction channels.
This presentation will discuss how the $^{55}$Co experiment was conducted, the preliminary analysis of the resulting data set, as well as the lessons that will be carried forward for the approved $^{55}$Ni experiment. In addition to investigating the charge dependence of the strong interaction, this data will be utilized to explore the f$_{7/2}$ hole configurations in $^{56}$Ni and electromagnetic transition rates for excited states of $^{55}$Ni and $^{55}$Co.
An understanding of the properties and behaviour of neutron-rich nuclei is essential in the study of phenomena such as neutron stars and supernovae. Successive addition of neutrons to an atomic nucleus yields isotopes that may or may not be stable: past a certain point, a nucleus experiences a decay process in which it leaks out neutrons, known as a neutron drip line. For nearly 20 years, the largest nucleus for which this was observed experimentally is Oxygen; its heaviest bound isotope is ${}^{24}$O, and it is confirmed that ${}^{26}$O and ${}^{28}$O are unbound. A breakthrough in 2019 resulted in experimental confirmation of drip lines for isotopes of Fluorine and Neon. However, results for elements higher in the nuclear chart remain unknown and unverified in either experiment, or even theory, due to the computationally complex nature of the problem.
Quantum computing has the potential to solve problems in the physical sciences more efficiently. While it has been widely applied to quantum chemistry, there are relatively fewer applications in nuclear physics. In this work, we extend the study of Oxygen to heavier isotopes than have been explored previously in order to demonstrate the neutron drip line using quantum computing. We begin using a basic 12-qubit variational eigensolver on a quantum simulator, and develop highly-optimized quantum circuits for this purpose. We evaluate the ground state energies using both phenomenological interactions and recently-developed microscopic interactions for which the drip line has been observed to closely match experimental results. Then, we leverage symmetries to reduce the problem to a 5-qubit one which is suitable for execution on real quantum hardware, and discuss the prospects of doing so. Such a demonstration shows how, with suitable resource management and leveraging key properties of the system, quantum computing may soon enable us to explore systems beyond the reach of both contemporary nuclear theory and experiment.
Heavy-ion storage rings connected to radioactive beam facilities offer a unique environment for nuclear physics experiments. So far, storage rings have been only coupled to in-flight fragmentation facilities, for example the ESR and the CRYRING at GSI Darmstadt, Germany, the CSRe at HIRF in Lanzhou, China, and the Rare RI Ring at RIKEN Nishina Center in Japan.
Neutron capture reactions play a crucial role for the understanding of the synthesis of elements heavier than iron in stars and stellar explosions via the slow (s), intermediate (i), and rapid (r) neutron capture processes. While the majority of the s-process neutron captures occur on stable or long-lived nuclei and have already been experimentally constrained, measuring the direct neutron capture cross section of short-lived nuclides (half-life << 1 year) has so far been out of reach and led to large uncertainties in Hauser-Feshbach predictions of very neutron-rich nuclei. To partially circumvent this problem, indirect measurements via (d,p) reactions in inverse kinematics are carried out, and the neutron capture cross section extracted with the help of theoretical models.
Recently, a new method to couple a neutron-producing "facility" to a RIB storage ring was proposed [1]. While their initial proposal involved a storage ring running through a high flux reactor, later ideas involved the use of a spallation neutron source. This direction is presently investigated at Los Alamos National Laboratory.
The TRIUMF storage ring project proposes to instead use a compact neutron generator. The whole facility would fit into the existing ISAC experimental hall and could be operational within a decade. Here, the TRISR project is introduced and some measurements are outlined that would become possible, especially with the upcoming availability of clean, intense radioisotope beams from the new ARIEL facility.
[1] R. Reifarth and Yu. A. Litvinov, Phys. Rev. ST Accel. Beams 17, 014701 (2014)
Despite tremendous progress, key questions remain in the field of neutrino physics. Are neutrinos Dirac or Majorana fermions? What is their absolute mass scale and mass ordering? Neutrinoless double beta decay ($0\nu\beta\beta$) searches are sensitive probes aiming to answer these questions. $0\nu\beta\beta$ experiments are continuously striving to further reduce background levels in order to observe these exceedingly rare decays. Where possible, observing the daughter ion, e.g. a $^{136}$Ba from a $^{136}$Xe double beta decay, would eliminate all non-$\beta\beta$ background signals, therefore increasing the detector sensitivity by large factors and offering an unambiguous identification of a positive $0\nu\beta\beta$ signal. We are developing a system to extract and identify Ba ions from liquid xenon. The system consists of a capillary probe to transport the ion from the liquid Xe volume to a Xe gas environment, followed by an RF-only ion funnel to extract the ion to vacuum. Then, the ion is loaded into a linear Paul trap for identification by laser spectroscopy. A multi-reflection time of flight mass spectrometer is under development to verify the ion's mass A=136. Ion sources are also being investigated, in particular an accelerator-based in-liquid Xe Ba-ion source. I will discuss the various aspects of this system and present the status of their development at Canadian institutions. Once an efficient system is demonstrated, we plan to deploy a demonstrator ion extraction apparatus with the intent of testing the Ba-ion tagging scheme for $0\nu\beta\beta$ searches.
nEXO is a proposed experiment that aims to detect neutrinoless double beta decay (0vbb), a Standard Model (SM) forbidden, rare nuclear process that, if observed, would have profound implications for fundamental physics. Such decay would be the first experimental evidence of the Majorana nature of neutrinos (i.e., neutrinos would be their own antiparticles), provide insights into the neutrino mass hierarchy, and also potentially explain the matter-antimatter asymmetry observed in the universe. nEXO will search for 0vbb in 5 tonnes of liquid xenon enriched in the double-beta decaying isotope Xe-136.
A technique called Ba-tagging has been proposed as a potential future upgrade path to nEXO, identifying the Xe-136 bb-decay daughter nucleus, Ba-136. Detection of a Ba-136 ion at the site of a possible 0vbb event will effectively exclude all non-double-beta decay background events and facilitate the unambiguous verification of a Xe bb-decay event. This talk will discuss the potential benefits of Ba-tagging for the upgraded nEXO experiment and focus on the latest results for the Ba-tagging subsystems, a linear Paul trap, and a time-of-flight mass spectrometer currently being commissioned at McGill University.
Silicon photomultipliers (SiPMs) are the photo-detection technology of choice for future noble-liquid scintillator rare-event search experiments, both in neutrino-less double beta decay and dark matter. The high radio-purity and exceptional gain of SiPMs along with a high VUV detection efficiency make them ideal for these applications. The Light only Liquid Xenon (LoLX) experiment is a small-scale R&D liquid xenon (LXe) detector located at McGill University. LoLX operates 96 Hamamatsu VUV4 SiPMs in a cylindrical geometry submerged in LXe. LoLX aims to perform detailed characterization of SiPM performance in LXe, and to characterize the light emission and transport from LXe to inform future LXe detectors. When photons are detected by a SiPM, individual photodiodes undergo an avalanche process. During this avalanche, near infra-red photons are emitted and can transport across the detector to other SiPMs which may produce correlated hits on other devices, a process referred to as SiPM external crosstalk (eXT). Using the LoLX detector we performed measurements of SiPM external crosstalk in LXe with similar geometric acceptance as future planned experiments. In this presentation, we will present the measurement of SiPM eXT detection within LoLX, with comparisons to GEANT4 eXT simulations informed by ex-situ measurements of SiPM photon emission characteristics.
Using the EMPIRE 3.2 code, an optimal model has been adapted to describe the proton interaction on 232Th for accelerator-based production of 225Ra and 225Ac which are important alpha emitting medical radioisotopes with viable production in accelerators. A hybrid nuclear level density which combines the nuclear level densities in Empire for the production of 225Ra, and 225Ac has been determined. The optimal model shows the important roles of the nuclear level densities and pre-equilibrium contribution to the good description of these interactions from 0 – 200 MeV. The reaction descriptions are found to be sensitive to the Nuclear Level Density description at different energies. It is noted that while no single description of the Nuclear Level Density provides an overall generally good description of the reaction throughout the energy range from threshold to 200 MeV, the energy and spin dependent level density parameter affects the Nuclear Level Density contribution significantly. The excitation functions obtained from this optimal description have been shown to have good agreement up to about 12% standard deviation with available measurements in EXFOR. The result of this work gives an insight into the necessary parameters for the production of 223Ra and 225Ac through 232Th.
Keywords: 225Ra, 225Ac, Alpha emitter, Proton interaction, Radioisotopes.
Graduate studies in physics (and other fields) is going through an existential crisis. The belief that the PhD was a solid pathway to an academic career was never grounded in reality (e.g., in the US in 18-19, 1903 PhD PhDs were conferred while only 369 new tenure-track positions advertised[1]). In recent times, the sharp increase in the cost of living without corresponding funding improvements forces us to question the value of the MSc and PhD, especially if it now requires students to take on outside part-time employment or pile on tuition debt. The traditional graduate degree is based on the student-supervisor relationship with the potential of a wonderful mentorship experience but with considerable risk of disfunction exacerbated by the intrinsic power imbalance. With no meaningful feedback channels, graduate training practices and student deliverables have tended to remain static, with little thought to what a student needs now in 2023 (or in the future). The NSERC Collaborative Research and Training Experience program provides a sandbox to experiment with graduate training, with its focus on student mobilization (national and international), professional skill development, interdisciplinary research, and collaboration between academia and industry. Results from our CREATE-Materials for Advanced Photonics and Sensing will be discussed, included interventions that proved transformative for some students and other efforts that fell flat.
[1] AIP reports “Faculty Job Market in Physics and Astronomy Departments“ “Trends in Physics PhDs”
I cover an introductory article I wrote with a group of students in the French language on the concepts of quantum information in tensor network algorithm. The resulting entanglement renormalization algorithms are known to be highly efficient for both classical and quantum lattice problems in a variety of use cases. I review best practices for creating such an introductory article, when they are necessary, as well as the physics. I then trace how this article has been used by future students.
[1] T.E. Baker, S. Desrosiers, M. Tremblay, M.P. Thompson, Méthodes de calcul avec réseaux de tenseurs en physique, Can. J. Phys. 99, 4 (2021) [ibid. Basic tensor network computations in physics, arxiv: 1911.11566]
Many measurements in physics lab experiments are affected by random errors. The usual approach in such cases is to take multiple measurements and use the mean value of the measurements as the experimental value for the physical quantity. The best estimate of the uncertainty in this experimental value is the error of the mean. Students are very familiar with the concept of the mean value due to its common use in determining their grades. The error of the mean, however, is not something that they encounter in everyday life and it has been my experience that the vast majority of students in first year physics labs do not come away with a clear understanding of this important quantity. At best they treat it as a black-box formula they are expected to use without really understanding it and, at worst, they fail to understand the difference between the standard deviation and the error of the mean. In this talk I will discuss a laboratory exercise which gives students a practical introduction to the normal distribution, standard deviation and the error of the mean. This exercise helps undergraduate physics students to gain a practical understanding of this important concept in experimental physics.
Degrees of freedom are one of the first concepts that an undergraduate student in physics learns. They are used in classical mechanics, statistical physics, and QFT, among others. However, its definition is not always carefully explained. In this talk, I will present a pedagogical approach to this concept through simple (but not trivial!) mechanical systems. I will underlie the role played by topology and geometry. Moreover, this approach provides as well a physical introduction to topology.
The CAP welcomes all Congress attendees for a discussion about funding for discovery research including student support. Dr. Marc Fortin, Vice-President, Research Grants and Scholarships Directorate at NSERC, will present a summary of NSERC’s funding for discovery research and scholarship programs. The presentation will be followed by a general discussion about ways to build funding for discovery research.
Support Our Science (SOS) is a grassroots organization that has been advocating for increased funding to graduate students and postdoctoral scholars in Canada. This past year they have organized a national walkout across 46 institutions coast to coast, launched multiple petitions and letter writing campaigns which have grabbed the federal government. Sarah Laframboise is this Executive Director of SOS and joins us to discuss the organization’s key asks: to increase funding to graduate students and postdocs thought scholarships, fellowships and grants.
In person at UNB Kinesiology, Rm. 215 with Teams connection
Axions and axion-like particles (ALPs) are a prominent dark matter candidate, drawing motivation in part from the axiverse of string theory. However, the string axiverse is not the only game in town: In this talk I will discuss axion-like particles that emerge as pions of a QCD-like dark sector. In a dark Standard Model (SM) wherein all 6 quark flavours are light while the photon is massive — one finds a rich low-energy spectrum of stable ultralight particles, in the form of neutral and charged dark pions, and complex neutral scalars analogous to the SM kaon, with mass splittings determined by the mass and charge of the dark quarks. Dark matter can be a mixture of all these ultralight bosonic degrees of freedom, and exhibit both parity-even and parity-odd interactions, making the theory testable at a wide variety of experiments. In context of dark QCD with $N_f$ flavours of light quarks, this scenario predicts $N_f^2-1$ ultralight axion-like particles — effectively an axiverse from dark QCD. This axiverse is consistent with but makes no recourse to string theory. Accounting for the full spectrum of the theory, it can also include a superheavy (“WIMPzilla") dark matter component, whose mass is connected to the axiverse by the confinement scale of the dark QCD.
The Penrose inequality places a lower bound on the mass of a black hole spacetime in terms of the area of a cross-section of the event horizon. The heuristic argument for the inequality is based upon the standard picture of gravitational collapse and it has been rigorously proved in the setting of time-symmetric initial data. We will discuss the derivation of a Penrose-type inequality with angular momenta for four dimensional, biaxially symmetric, maximal, asymptotically flat initial data sets $(M,g,k)$ for the Einstein equations with fixed angular momenta and horizon inner boundary.
Using an exact solution for a two-dimensional scalar field propagating in a variation of the Alcubierre metric, we analyze how apparent horizons affect localized quantized wavepackets. We analyze the loss of fringe visibility in a single-photon interferometer, and the reduction of entanglement between two 2D photons, if one photon travels through a region with spacetime curvature. We also derive an expansion of the field operator in terms of localized modes by means of an over-completeness relation.
The direct observation of gravitational waves was one of the most exciting events in physics in the last decade. It opened a whole new window for studying the universe and prompted a lot of interest in the observable effects of gravitational waves. One example of this is studying the effect of gravitational waves on quantum fields. In this talk I will discuss the series solution of the massless Klein-Gordon equation in a region of spacetime with curvature described by a spatially dependent gravitational wave that falls off with distance from the source. This will allow us to study how a quantum plane wave will be affected by a gravitational wave. This seemingly straightforward problem actually requires careful analysis in order to get the correct result in the limit where the gravitational wave and the quantum wave are collinear. One of the interesting results of this analysis is an enhancement of the probability current of the quantum wave along the direction of propagation of the gravitational wave.
The Lambert W function has been used in solving a variety of diverse problems in a variety of topics in physics, chemistry, engineering and mathematics. In physics, it has been useful in the study of statistical distributions such as the Planck black body, Fermi-Dirac and Bose-Einstein distributions and the fringe fields associated with a parallel plate capacitor, the study of thermoelectric as well as metamaterials and solar cells. For metamaterials, a geometric analytic solution is employed in 2 complex planes, where one plane is the inverse Lambert W mapping of the other and the solutions are the intersection of the associated radial equation and the Lambert lines.
In this work, we have analyzed the Graded Index Metamaterial (GIM) Waveguide problem discussed by Xu et al (2013) and given a Lambert W interpretation for the model. The solution set is a subset of the solutions of the radial equation and the corresponding Lambert lines. Some key differences that exist between previously discussed models and the GIM models are analyzed. The solution of the GIM Model is represented as the intersection of the radial equation and family of the solution obtained from the intersection of two perpendicular Lambert Sheets.
Many would agree that the best way to learn physics is to do physics, such as in a research lab setting. This can be difficult in practice, as principal investigators are often working at a frenetic pace to obtain and distribute results of their work.
I will describe our efforts in setting up a funded research laboratory experience for undergraduates: The Quantum Teaching Lab (QTL). In the QTL short term research projects in Atomic and Quantum Optics are performed that are chosen to be suitable for dedicated undergraduates.
Introducing students to quantum science at an earlier age is essential to developing the quantum workforce and fostering widespread appreciation of quantum technologies. Hands-on active learning can help make the abstract ideas of quantum information tangible to students, but lab experiments in quantum information are traditionally too expensive, too complex, or too indirect to be useful in classrooms. In this session, we'll outline efforts by the Institute for Quantum Computing (IQC) to develop lab activities for the Quantum School for Young Students (QSYS) and other student groups primarily at the upper high-school level. In particular, we'll highlight a low-cost 3D-printed quantum key distribution demonstration that gives students hands-on experience with the fundamental principles of quantum information.
Hands-on experience in a science lab is crucial for science majors, especially for those pursuing a degree in physics as it forces the engagement of different levels of knowledge in decision-making (Millar, 1994). The switch to online learning due to the pandemic placed an Everest-sized challenge at our feet; how to satisfy the experiential learning outcomes of the program when students do not have access to the physical space and equipment while knowing that the type of laboratory experience affects gains and depth of learning (Bernhard, 2018).
The task brought together a collaboration between research and teaching faculty and technical staff, in order to create meaningful experiential learning opportunities for over a thousand stakeholders. The implemented solutions included the development of hardware and software, the creation of documentation and training procedures for teaching assistants, and designing of the support system for the students.
While at-home labs of various kinds have been successfully implemented at various institutions across North America the remote labs were a creative alternative developed by the physics teaching team at the University of Calgary. Students could log into a website and view a livestream of physical equipment located at the University, connect to the devices, and send commands that allowed them to make measurements in real-time. We used Arduinos and high-resolution cameras to actuate motors, read sensor data, and collect photographs of various digital and analog meters.
During this session we will briefly discuss all solutions we implemented, spending the most time on the remote laboratories, together with some data showing students’ self-assessment of their learning. We will also share ideas of how, moving forward, the resources we have developed can be used to increase the accessibility to our courses for life-long learners of various backgrounds and to enhance outreach and recruitment efforts.
This presentation describes different ways a smartphone’s onboard magnetometer can be combined with a simple student-constructed coil of wire and used to explore relationships between electricity and magnetism. The measurement of electrical phenomena such as DC current and voltage will be discussed.
For several years students and teachers have had access to software that enables the use of smartphones as experimental tools, or SETs, by providing access to the output of sensors common to most smartphones such as accelerometers, light sensors and microphones. A significant amount of attention has been paid by the academic community to the effectiveness of this approach and many different student activities have been developed that allow more traditional (and expensive) teaching equipment to be supplemented by and perhaps even replaced by student smartphones equipped with free software.
A smartphone’s ability to measure electrical signals directly is usually limited to the use of an earphone jack, and the risk of damage to the smartphone posed by this approach makes it unattractive to teachers. As a result, the area of secondary- and undergraduate-level physics education least addressed by existing SETs-related resources is electricity.
Almost all smartphones include a magnetometer based on multiple Hall Effect sensors, and this presents a relatively risk-free way to infer electrical current from the magnetic field created by a simple coil, for example. This presentation will review the small number of publications that examine this idea, describe experimental results obtained using different smartphones and different coil designs, and provide example activities a teacher may attempt using this approach.
Physical examples are a great way to get students engaged with course content but it is not always easy to find classroom examples for senior course material. One such concept that I have been struggling with is wave modes. This concept arises naturally in mathematical physics courses and it is critical in my research area of acoustical oceanography. In searching for a classroom demonstration for dispersive waves, I happened across the idea of using the various acoustic modes that can propagate through a cylindrical pipe. In this paper, I review the background theory of sound wave propagation in a cylinder and demonstrate that you can hear the effect of the modal propagation in a classroom scale demonstration. Spectral analysis of sound recordings clearly shows the frequency cutoffs of distinct modes.
Au mois de juin 2022, dans le cadre du programme de soutien à la mobilité enseignante géré par la Direction des affaires internationales de la Fédération des cégeps, un séjour scientifique de 18 jours a été réalisé dans la région du Val di Noto, au sud-est de la Sicile, en Italie, dans le but notamment de valider les informations descriptives à caractère géologique contenues dans le récit intitulé Mémoire sur les volcans éteints du Val di Noto, rédigé par le minéralogiste français Déodat de Dolomieu (1750-1801), publié en 1784. À l’aide de cartes géologiques modernes fournies par le Département de géologie de l’Université de Catane ainsi qu’avec l’utilisation d’un drone, les environs des villages de Vizzini et de Militello in Val di Catania (Valle del Loddiero) ont été examinés du point de vue de la pétrographie et de la stratigraphie. Les résultats de ces observations de terrain confirment les descriptions détaillées faites par Dolomieu dans son mémoire et corroborent partiellement ses interprétations, qui sont à l’origine de la spectaculaire alternance de vulcanites et de calcarénites présentes dans les régions examinées. Dans cette présentation, les résultats principaux de cette recherche seront exposés en accordant une importance particulière au rôle historique fondamental joué par Dolomieu dans l’étude du volcanisme des monts Hybléens.
Discussion of the topics that the CAP should be including in their brief to the Federal Finance Committee this fall for the 2024 Budget. This will be a follow-on from the morning presentation (R1-6), expanded to cover other topics of importance/ interest.
I will give an overview of gravitational-wave discoveries to date, and the advances in technology and data science that have enabled these early detections. I will summarize new physics that will be unlocked by future gravitational-wave detectors on Earth and in space.
In this talk, Dr. Grant Williams will leverage playful ideas and metaphorical thoughts to draw connections between fundamental physics concepts and such aspects of the human experience as birth, childhood, puberty, friendship, love, relationships, conflict, family, diversity, equity, inclusion, spirituality, aging, death and the beyond.
Results of Council Elections
Strategic Planning Committee Draft Report
Virtual viewing: https://teams.microsoft.com/l/meetup-join/19%3axvWhM82L7XsnMYJaAwZJP4eDOJBo4VLs95gO7aQmP6E1%40thread.tacv2/1686742652109?context=%7b%22Tid%22%3a%22244e6ed2-339a-47f3-b95c-e45351c198b7%22%2c%22Oid%22%3a%222541dfad-f78d-4bb3-a827-4062f4553e13%22%7d
Virtual viewing: https://teams.microsoft.com/l/meetup-join/19%3axvWhM82L7XsnMYJaAwZJP4eDOJBo4VLs95gO7aQmP6E1%40thread.tacv2/1686742652109?context=%7b%22Tid%22%3a%22244e6ed2-339a-47f3-b95c-e45351c198b7%22%2c%22Oid%22%3a%222541dfad-f78d-4bb3-a827-4062f4553e13%22%7d