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Takaaki Kajita10/08/2026, 09:00
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Beate Heinemann (DESY and University of Freiburg (Germany))10/08/2026, 10:00
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Belen Gavela Legazpi (Universidad Autonoma de Madrid (ES))10/08/2026, 10:30
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Belen Gavela Legazpi (Universidad Autonoma de Madrid (ES))10/08/2026, 10:35
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Alexei Smirnov10/08/2026, 11:30
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Matteo Galli (APC - CNRS)10/08/2026, 12:00Young Scientist Forum talk + poster
The Deep Underground Neutrino Experiment (DUNE) is a next-generation long-baseline experiment designed to resolve key questions in neutrino physics, including the neutrino mass ordering, by studying neutrinos produced by an accelerator beam and from natural sources (atmospheric, supernovas and solar). The sensitivity to the neutrino mass ordering from atmospheric neutrinos at DUNE can be...
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Shreya Pandit (University of Southampton)10/08/2026, 12:06Young Scientist Forum talk + poster
We discuss how non-adiabatic mixing in quantum mechanics can be conveniently described within a density matrix formalism. We derive a general formula for the transition probability that generalises well known Landau-Zener formula and can be applied to different problems. In particular, we consider active-sterile neutrino mixing in the early universe and reproduce numerical results existing in...
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Guilherme A. Nogueira (State University at Campinas)10/08/2026, 12:12Young Scientist Forum talk + poster
We constrain charged-current scalar non-standard interaction with reactor antineutrinos within a quantum field theory framework of neutrino oscillations. We derive an analytical expression up to $\mathcal{O}(\varepsilon^{4})$ for the electron antineutrino survival probability including scalar NSI contributions, and show that these effects induce spectral distortions that admit a large mixing...
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Katarina Bleau10/08/2026, 12:18Young Scientist Forum talk + poster
Neutrino flavour conversion, usually described by vacuum oscillations and neutrino-matter forward scattering, is a a well-established phenomenon that has been observed experimentally. However, in very dense environments such as supernovae, neutrino-neutrino interactions are not negligible and the dominant flavour conversion process is coherent forward scattering. Understanding collective...
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Jan Plößner (Max-Planck-Institut für Kernphysik)10/08/2026, 12:24Young Scientist Forum talk + poster
The KArlsruhe TRItium Neutrino (KATRIN) experiment probes the effective electron anti-neutrino mass by a precision measurement of the tritium beta-decay spectrum near the endpoint. A world-leading upper limit of $0.45\,$eV$\,$c$^{-2}$ (90$\,$% C.L.) has been set, including the data of the first five measurement campaigns. With data collection now complete after a total of 19 measurement...
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Bonnie Fleming (Yale University)10/08/2026, 12:30
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Thomas Schwetz10/08/2026, 14:45
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Kierthika Chathirathas10/08/2026, 15:15Young Scientist Forum talk + poster
We investigate scenarios in which all or part of the neutrino masses arise from a coupling to an ultra-light scalar dark matter field. The oscillating dark matter background induces time-dependent neutrino masses, leading to observable modifications of neutrino oscillation probabilities. Depending on the dark matter mass, different oscillation averaging regimes arise, which we study in a...
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George Parker10/08/2026, 15:21Young Scientist Forum talk + poster
With the JUNO experiment currently operating, and DUNE and Hyper-Kamiokande under construction, if a core-collapse supernova occurs in our galaxy we will have a wealth of fascinating data. In this work, we scrutinize the possibility of neutrinos being accelerated by repeatedly crossing the supernova shockwave (similar to first order Fermi acceleration). In this case, supernova neutrinos could...
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Alex Wen10/08/2026, 15:27Young Scientist Forum talk + poster
We present a method at IceCube to measure the astrophysical tau neutrino component and include preliminary results. BSM context of the measurement will be discussed.
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Pablo Blanco Mas (IFT UAM/CSIC)10/08/2026, 15:33Young Scientist Forum talk + poster
We present a detailed statistical reassessment of the apparent tension between the T2K and NOvA long-baseline neutrino oscillation experiments, focusing on the robustness of its significance under non-asymptotic conditions.
Our analysis reveals that the naive interpretation of the T2K–NOvA discrepancy in terms of the Gaussian approximation can lead to misestimated confidence levels, with...
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Tanvi Krishnan (Harvard University)10/08/2026, 15:39Young Scientist Forum talk + poster
In order to develop a consistent quantum theory of gravity, we must understand whether spacetime exhibits fluctuations at the Planck scale. If these Planck-scale fluctuations exist, they may cause propagating particles to evolve in an apparently non-unitary manner. Neutrinos, which interact only via the weak force and gravity, maintain quantum coherence while propagating over large distances....
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Francis Halzen (University of Wisconsin Madison (US))10/08/2026, 15:45
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Miguel Escudero Abenza (CERN)10/08/2026, 17:00
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Pilar Coloma (Instituto de Fisica Teorica UAM-CSIC)10/08/2026, 17:30
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Laura Baudis (University of Zurich (CH))11/08/2026, 09:00
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Tracy Slatyer11/08/2026, 09:30
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Axel Lindner (Deutsches Elektronen-Synchrotron (DE))11/08/2026, 10:00
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Belen Gavela Legazpi (Universidad Autonoma de Madrid (ES))11/08/2026, 10:30
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Nataliya Porayko (University of Milano Bicocca)11/08/2026, 11:30
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Jorge Alda Gallo (Università di Padova/INFN)11/08/2026, 12:00Poster session only
In this poster I review several recent results regarding the interactions between ALPs with $m_a \sim \mathcal{O}(\mathrm{GeV})$ and hadrons: chirally-consistent extensions of $\chi$PT up to several GeV, implementation in the ALP-aca public library, baryon phenomenology, ALP solutions to the $B^+ \to K^+ \mathrm{inv}$ excess at Belle II...
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Junseok Lee (Tohoku University)11/08/2026, 12:06Young Scientist Forum talk + poster
We show that heavy axion domain walls induce domain walls of the QCD axion through a mixing between the heavy axion and the QCD axion, even when the pre-inflationary initial condition is assumed for the QCD axion. The induced domain walls arise because the effective θ parameter changes across the heavy axion domain walls, shifting the potential minimum of the QCD axion. When the heavy axion...
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Nicolas Martinez (IFT-UAM CSIC)11/08/2026, 12:12Young Scientist Forum talk + poster
The established $d=5$ ALP effective Lagrangian describes scalars with approximate shift-symmetry, which carry no Standard Model charges. It implicitly assumes that ALPs are not charged under any symmetries of the dark sector. In this talk, we remove this assumption. In this case, no $d=5$ ALP effective interaction with SM particles is possible. We build the effective Lagrangian for these...
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José Ricardo Correia (University of Oslo)11/08/2026, 12:18Young Scientist Forum talk + poster
A promising dark matter candidate, which arises from a proposed solution to the strong CP problem is the pseudo scalar axion. If the PQ symmetry is broken after inflation, a network of cosmic strings forms and emits axions until the QCD phase transition, where a hybrid string-wall system forms and collapses. Characterizing both the evolution of the network and the emission of axions by the...
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Jacob Lindahl11/08/2026, 12:24Young Scientist Forum talk + poster
Cosmological simulations in the post-inflation scenario have shifted the favored axion mass toward higher values, necessitating new ways to probe this region. The plasma haloscope presents a promising approach for high-mass axion dark matter searches, addressing the loss of interaction volume that limits traditional cavity haloscopes at high frequencies. It employs wire metamaterials, in which...
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Eva Villaver11/08/2026, 12:30
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Keir Rogers11/08/2026, 14:45
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Stefan Nellen Mondragón (HEPHY - ÖAW)11/08/2026, 15:15Poster session only
The Migdal effect—the prompt ionization induced by a sudden nuclear recoil—is widely used in direct dark matter searches. Recently, the first detection of the Migdal effect was announced in a gaseous target. All previous theoretical calculations relied on the so-called impulse approximation: the assumption that the projectile scatters of the nucleus instantaneously. Nevertheless, one would...
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Nora Hoch11/08/2026, 15:21Young Scientist Forum talk + poster
The search for sub-GeV dark matter requires novel experimental design due to the small expected energy signal and large backgrounds, many of which still need to be modeled or calibrated. One way forward is to explore different detector volumes with unique material properties and combine them with cutting-edge photodetectors. I will present on two materials that would make good detector...
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Torben Flehmke11/08/2026, 15:27Young Scientist Forum talk + poster
Liquid xenon detectors such as XENONnT or LZ are amongst the leading experiments to provide limits on the WIMP-nucleon cross section for WIMPs heavier than 10 GeV/$c^2$. In order to achieve these results, photosensors with outstanding sensitivity and a low intrinsic radioactivity are required. The traditionally used photomultiplier tube (PMT) is a well established technology, that provides the...
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Rinchen Sherpa (Indian Institute of Science (IISc), Bengaluru)11/08/2026, 15:33Young Scientist Forum talk + poster
A variety of detection techniques employing different materials has been suggested
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for the direct detection of low-mass galactic dark matter particles, which fall below the
sensitivity of traditional direct detection experiments. Bilayer graphene is one such material
that has been proposed for the detection of sub-MeV mass dark matter particles through
electronic excitations. In this work,... -
Pamela Stark11/08/2026, 15:39Young Scientist Forum talk + poster
The QCD axion is a well-motivated dark matter candidate that could simultaneously resolve two major open questions in physics: the strong-CP and dark matter problems. Experimental searches for the axion often target its coupling to the photon, where axion-to-photon conversion in a strong magnetic field produces a faint alternating current whose frequency depends on the unknown axion mass....
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Ryan Plestid (CERN)11/08/2026, 15:45
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Maria Ramos11/08/2026, 17:00
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Prof. Mariangela Lisanti (Princeton University)11/08/2026, 17:30
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Dr Eva Villaver11/08/2026, 19:00
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Prof. Eiichiro Komatsu (Max Planck Institute for Astrophysics)12/08/2026, 09:00
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Dr Vivian Poulin (LUPM, CNRS & U. de Montpellier, France)12/08/2026, 09:30
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Yvonne Wong12/08/2026, 10:00
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Belen Gavela Legazpi (Universidad Autonoma de Madrid (ES))12/08/2026, 10:30
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Mikko Sakari Laine (Universitaet Bern (CH))12/08/2026, 11:30
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Vinicius Oliveira12/08/2026, 12:00Young Scientist Forum talk + poster
We present an updated study of the strong-coupling freeze-in mechanism for dark matter (DM) production, extending the analysis of Invisible Higgs decay from dark matter freeze-in at stronger coupling (Published in: JHEP 04 (2025) 136). This framework enables the production of light non-thermal DM with sizeable interactions to the Higgs field, even for order-one portal couplings, leading to...
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Daniel Naredo Tuero12/08/2026, 12:06Poster session only
The majoron is the Nambu-Goldstone boson associated with the spontaneous breaking of a global $B-L$ symmetry. Remarkably, the minimal majoron framework can simultaneously address three key empirical indications of physics beyond the Standard Model: neutrino masses, the matter-antimatter asymmetry, and dark matter. In this work, we identify the cosmologically viable region in which majoron dark...
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Giorgio Laverda12/08/2026, 12:12Young Scientist Forum talk + poster
Stochastic backgrounds of gravitational waves (GWs) represent a unique source of information on very high-energy processes taking place in the early Universe: they offer us a gravitational window into the otherwise hidden physics between inflation and the onset of the hot Big Bang. In this context, it is interesting to consider how minimal scenarios of reheating via a beyond-the-Standard-Model...
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Charalampos Nikolis12/08/2026, 12:18Young Scientist Forum talk + poster
Axion relic pockets are phase-transition remnants consisting of regions of false vacuum stabilised from collapse by a hot axion gas. Axion relic pockets can comprise dark matter, but little is known about their phenomenology. We consider trapped axions coupled to electromagnetism and show that axion-photon conversion occurs in atomic electric fields, leading to high-energy electromagnetic...
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Paolo Bilisco (IPhT - Université Paris-Saclay)12/08/2026, 12:24Young Scientist Forum talk + poster
LIGO, VIRGO and Kagra (just to name a few) represent outstanding feats of engineering that have launched us in a new era of gravitational-wave (GW) detection. Even so, we may wonder whether their sensitivity is enough to detect very high-frequency signals of beyond-Standard-Model origin, such as those sourced by primordial stochastic GW backgrounds, primordial black holes, or black hole...
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Joachim Kopp (Johannes Gutenberg Universitaet Mainz (DE))12/08/2026, 12:30
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Raman Sundrum13/08/2026, 09:00
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Xubin Hu (University of Southampton)13/08/2026, 09:30Young Scientist Forum talk + poster
I will discuss SO(10)-inspired leptogenesis, a well known scenario of leptogenesis relying on conditions realised within SO(10) models and also beyond. I will first review results within current approximations and then I will show new results including flavour coupling effects that have not yet been considered so far. I will also confront predictions and constraints from SO(10)-inspired...
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Anna Llauradó Filella (IJCLab, Université Paris-Saclay)13/08/2026, 09:36Young Scientist Forum talk + poster
The rare decay $B\to K\nu\nu$ provides a theoretically clean observable to probe New Physics effects, as the problematic charm-loop contributions that affect processes involving muons are negligible in this case. Recent measurements from the Belle II experiment have shown a deviation from the Standard Model predictions at the $3\sigma$ level, which can be accommodated by an Effective Field...
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Lucas Puetter13/08/2026, 09:42Young Scientist Forum talk + poster
We investigate how scalar-mediated potentials with Lorentz-violating couplings to Standard Model fermions affect spectroscopic observables in atoms and highly charged ions. Using high-precision hydrogen spectroscopy, we constrain the parameter space for both ordinary scalar couplings and couplings to the time-like component of a background Lorentz-violating vector. By considering hydrogen and...
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Jonathan Steiner (University of Heidelberg)13/08/2026, 09:48Young Scientist Forum talk + poster
String theory compactifications come with numerous U(1) factors, implying the presence of many hidden photons in the low-energy EFT. One may call this the string photoverse. We argue that, generically, these hidden photons are massless and do not couple to any light dark current such that, naively, kinetic mixing with the Standard Model is unobservable. On symmetry grounds, one thus expects...
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Elina Merkel (University of Bologna & INFN Bologna)13/08/2026, 09:54Young Scientist Forum talk + poster
Rich dark sectors represent a compelling class of non-minimal SM extension models with potential to address one or several puzzles in astroparticle physics and cosmology such as dark matter, neutrino masses, and baryogenesis. Such models feature multiportal connection to the SM and non-negligible couplings between numerous dark particles which results in phenomenological signatures...
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Seth Koren (University of Notre Dame)13/08/2026, 10:00
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Aneesh Vasant Manohar (Univ. of California San Diego (US))13/08/2026, 11:30
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Prof. Tom Melia (Kavli IPMU)13/08/2026, 12:00
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Rachel Houtz13/08/2026, 12:30
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Jorinde van de Vis (CERN)13/08/2026, 14:45
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Andrea Giovanni De Marchi13/08/2026, 15:15Young Scientist Forum talk + poster
Blazars are a subclass of active galactic nuclei (AGN), the brightest continuously emitting sources in the Universe, powered by accreting supermassive black holes (SMBH). Their defining characteristic is the presence of powerful, back-to-back relativistic jets of protons and electrons, with one jet closely aligned in the direction of Earth. This offers a unique opportunity to probe physics...
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Maya Hager (Max-Planck-Institut für Kernphysik)13/08/2026, 15:21Young Scientist Forum talk + poster
Dirac leptogenesis offers an alternative mechanism
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to generate the matter-antimatter asymmetry that avoids the typical requirements of lepton number violation, as in Majorana leptogenesis, or of a first order phase transition, as in electroweak baryogenesis. Instead, the asymmetry can be generated through
chiral asymmetries that remain out of equilibrium in the early Universe.... -
Pedro Zilves Maio Ventura (São Paulo University)13/08/2026, 15:27Young Scientist Forum talk + poster
In this work, we study the Migdal effect in the direct detection of dark matter using different atomic targets, focusing on how this phenomenon can modify current exclusion limits, particularly in the low-mass region. The Migdal effect, which describes electronic ionization or excitation induced by a nuclear recoil, has recently become a key topic in dark matter searches, as it enables...
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Maximilian Detering13/08/2026, 15:33Young Scientist Forum talk + poster
We proposes a novel link between the hierarchy problem and Weakly Interacting Massive Particles (WIMPs), suggesting that the small mass of the Higgs boson arises from the universe’s WIMP-induced proximity to the critical boundary of a phase transition. Intriguingly, such a requirement aligns with the so-called “WIMP miracle”: a WIMP with mass around the weak scale and Standard Model couplings...
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Mrs Garance Lankester--Broche (Particle Physics Group, Faculty of Physics, University of Vienna; Marietta Blau Institute for Particle Physics, Austrian Academy of Sciences)13/08/2026, 15:39Young Scientist Forum talk + poster
Small-scale tensions in the internal structure and evolution of dark matter halos motivate the exploration of dark matter dynamics beyond the collisionless $\Lambda$CDM paradigm. In particular, dark matter self-interactions can modify halo thermodynamics through heat transport and effective viscosity. If light dark-sector states can be radiated, these self-scatterings also open dissipative...
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Dr Venus Keus (Dublin Institute for Advanced Studies (DIAS))13/08/2026, 15:45
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Kimmo Juhani Kainulainen (University of Jyvaskyla (FI))13/08/2026, 17:00
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Prof. Jose Juan Blanco-Pillado (IKERBASQUE & UPV/EHU)13/08/2026, 17:30
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Hitoshi Murayama (University of California Berkeley (US))14/08/2026, 09:00
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Jose Daniel Domenech Moya (IFT - UAM)14/08/2026, 09:30Young Scientist Forum talk + poster
Mainly the content of our two most recent papers:
https://arxiv.org/pdf/2506.21716
https://arxiv.org/pdf/2507.20988Possibly also another work conducted this year. Everything is about multiple Higgs production within the Higgs Effective Field Theory.
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Esteban Ricardo Chalbaud Mogollon (Laboratory of Instrumentation and Experimental Particle Physics (PT))14/08/2026, 09:36Young Scientist Forum talk + poster
We investigate the CP structure of an invisible $Y_0$ mediator using a new set of NLO angular observables ($b_2$, $\tilde{b}_{2}^{\hat{y}}$, $n4$) optimized for $t\bar{t}$ dileptonic final states. Our analysis reveals that simple Forward-Backward Asymmetries ($A{FB}$) are exceptionally robust, matching the exclusion power of full shape-based methods, providing strong sensitivity for mediators...
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Marta Fuentes Zamoro14/08/2026, 09:42Young Scientist Forum talk + poster
Perturbative partial-wave amplitudes diverge in cases with a massless exchanged particle in the $t$-channel. We argue that the divergence is an artifact of perturbation theory and give a prescription for the all-orders correction factor that renders the partial waves finite. As an example, we apply this to longitudinal $W^+W^-$ elastic scattering, for which there is a photon exchange...
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Cristofer Caballeros14/08/2026, 09:48Young Scientist Forum talk + poster
Effective Field Theories (EFTs) are a framework to probe physics beyond the Standard Model (BSM) in a model independent way. The Standard Model Effective Theory (SMEFT) provides an expansion of higher-dimensional operators that encode the effects of heavy new physics; however, in the operator basis there exists a redundancy in the space of field redefinitions which leaves on-shell amplitudes...
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ALVARO LOZANO ONRUBIA (IFT UAM-CSIC)14/08/2026, 09:54Young Scientist Forum talk + poster
Many well-motivated extensions of the Standard Model predict new, entirely bosonic sources of CP violation (CPV). In these scenarios, the simultaneous observation of carefully selected bosonic processes emerges as a simple yet powerful method to unambiguously reveal the presence of CPV. The present study, which establishes a promising framework of CPV searches for the upcoming HL-LHC era,...
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David Kaplan14/08/2026, 10:00
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Thomas Steingasser (IFT Madrid)14/08/2026, 11:30
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Dr Olcyr Sumensari (IJCLab)14/08/2026, 12:00
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Xabier Cid Vidal (Instituto Galego de Física de Altas Enerxías)14/08/2026, 12:30
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Sophie Alice Renner (University of Glasgow (GB))14/08/2026, 14:45
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Rebeca Gonzalez Suarez (Uppsala University (SE))14/08/2026, 15:15
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Karl Jakobs (University of Freiburg (DE))14/08/2026, 15:45
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Poster session only
First of all, we will reiterate a mechanism for relic early universe gravitons. This is the precursor of the main result of this paper and involves the decay of micro black holes, with relic graviton production. . For the 2nd part of graviton physics, we invoke re acceleration of the universe The case for a four-dimensional graviton mass (non-zero) influencing reacceleration of the universe...
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DHRUV PASARI (Durham University)Poster session only
Domain walls beyond the textbook Z₂ kink have been studied analytically and through effective models, but seldom simulated directly on the lattice. We close that gap, evolving Z₃ and Z₄ wall networks with CosmoLattice. These networks are qualitatively richer than Z₂: walls come in distinct species, meet along junctions, and can transmute into one another rather than simply annihilating. To...
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David Cabo Almeida (University of Göttingen)Poster session only
In theories with extended scalar sectors, the lightest new scalar could be accessible at colliders. Instead of relying on simplified models, we describe such scenarios in a general and gauge-invariant way using an extended HEFT framework with a nonlinearly realized electroweak symmetry. The structure of the effective operators depends on the $SU(2)$nature of the scalar in the UV, leading to...
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Patrick FitzpatrickPoster session only
The apparent fine-tunings of the Standard Model Higgs potential may be a consequence of its near-criticality. If its parameters are selected by an underlying mechanism that places the theory near criticality, then the scale of vacuum instability sets an upper bound on the Higgs mass. This reframes the hierarchy problem as a consequence of vacuum metastability and predicts new physics that...
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Poster session only
Neutrinos can experience more than the MSW effect when they travel through an elliptically polarized oscillating background: ultralight vector dark matter. This is analogous to the Landau–Zener–Stückelberg–Majorana effect. We show that Majorana neutrinos convert into antineutrinos in such a background coupled to lepton number, e.g., the gauge boson of $U(1)_{B-L}$. The conversion is suppressed...
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Poster session only
Neutrinos are electrically neutral within the Standard Model, but this property need not hold in theories beyond it. If neutrinos possess a tiny electric charge (“millicharge”), they would experience Lorentz deflection while propagating through magnetic fields. For supernova neutrinos, such deflection in Galactic and extragalactic magnetic fields would increase their path length and,...
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Poster session only
I will present unique features in the growth of structure in wave dark matter models with warm white noise, where the power spectrum is peaked at sub-horizon wavenumbers. The post-inflationary production of bosonic particles, such as axions or axion-like particles, leads to an enhanced isocurvature density power spectrum on small scales. Moreover, when dark matter is extremely light, these...
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Poster session only
I will present $\texttt{BARYONET}$, an open-source framework for computing the baryon asymmetry of the Universe within electroweak baryogenesis (EWBG). Starting from the semiclassical WKB approach—where spatially varying complex masses across expanding bubble walls generate CP-violating forces—we derive and solve the transport equations governing chemical potentials and velocity perturbations,...
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Giovani Dalla Valle Garcia (The University of Melbourne)Poster session only
We investigate minimal dark matter models based on a confining ($\mathrm{SU}(N)$) dark sector, motivated by the central role of non-Abelian gauge forces in the Standard Model. After arguing that dark gluons alone cannot provide viable self-interacting dark matter capable of addressing small-scale structure tensions, we consider theories with dark quarks. Although light dark quarks can generate...
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Poster session only
We propose two medium-baseline, kiloton-scale neutrino experiments to study neutrinos from LHC proton-proton collisions: SINE, a surface-based scintillator panel detector observing muon neutrinos from the CMS interaction point, and UNDINE, a water Cherenkov detector submerged in Lake Geneva (or Lac Léman) observing all-flavor neutrinos from LHCb. Using a Monte Carlo simulation, we estimate...
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Poster session only
Ultralight dark matter may couple quadratically to Standard Model particles. Such quadratic interactions give rise to both coherent and stochastic signals in pulsar timing array (PTA) observations. In this work, we characterize these signals, including the effects of dark matter propagation in a finite-density medium, and assess the sensitivity of current and upcoming PTA observations to their...
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Poster session only
DUNE is a next-generation neutrino physics experiment that is currently under construction in the United States. The experiment will feature a high-intensity neutrino beam and a Near and Far Detector complexes located at a distance of 574 m and 1300 km from the neutrino source, respectively. While the primary goal of DUNE will be the discovery of CP violation in the lepton sector and the...
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Antonio Zoccoli (Universita e INFN, Bologna (IT))
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