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09/06/2025, 09:00
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Carla Bonifazi (ICAS-ICIFI-UNSAM/CONICET), Irina Nasteva (Federal University of Rio de Janeiro (BR))09/06/2025, 09:05
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Matthew Green (NC State University)09/06/2025, 09:20Talk
The COHERENT Collaboration is continuing its efforts to measure CEvNS and inelastic neutrino interactions at Oak Ridge National Laboratory’s Spallation Neutron Source. This presentation will include an overall summary of COHERENT’s efforts as the Collaboration transitions from first-light CEvNS observations to precision measurements with larger-mass detector systems and a power-upgraded SNS....
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Francesc Monrabal-Capilla (Donostia International Physics Center (DIPC) (ES))09/06/2025, 09:45Talk
I will present the current status of the experiment GanESS and the GaP proptotype, an effort to detect Coherent Elastic Neutrino-Nucleus Scattering (CEνNS) at the European Spallation Source (ESS), utilizing high-pressure Time Projection Chambers (TPCs) as the detection technology. The use of high-pressure noble gas TPCs allows for very good energy resolution and sub-keV thresholds,...
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Prof. Xiang Xiao (Sun Yat-sen University (China))09/06/2025, 10:07Talk
The CICENNS (CsI detector for Coherent Elastic Neutrino Nucleus Scattering) experiment aims to construct a CsI(Na) detector array with total mass of 300 kg, located at the China Spallation Neutron Source (CSNS), for the precise measurement of CEvNS signals. I will present the plan, status, and physics goals of CICENNS in this talk.
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Matteo Cappelli (Sapienza Universita e INFN, Roma I (IT))09/06/2025, 11:00Talk
A precise characterization of CEνNS in the fully coherent regime will have important implications both in the search for new physics and in technological applications. To this aim, the NUCLEUS experiment will exploit the two reactor cores of the Chooz-B nuclear power plant in France as neutrino sources, and cryogenic calorimeters made of CaWO$_4$ and Al$_2$O$_3$ crystals read out by TES as...
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Raimund Johann Strauss (Technische Universitaet Muenchen (DE))09/06/2025, 11:22Talk
The CRAB (Calibrated nuclear Recoils for Accurate Bolometry) project is aimed at precise calibration of cryogenic detectors at sub-keV nuclear recoil energies, addressing key challenges in coherent neutrino scattering and low-mass dark matter detection.
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After the successful validation of the method, demonstrated by the detection of recoil peaks in cryogenic detectors exposed to a commercial... -
Leila Haegel09/06/2025, 11:44Talk
The RICOCHET experiment aims to observe coherent elastic neutrino-nucleus scattering (CEνNS) with electron antineutrinos at the Institute Laue-Langevin (ILL) research nuclear reactor based in Grenoble, France. The setup is based on two arrays of cryogenic detectors operated at 10 mK: the CryoCube and the Q-Array. The CryoCube consists of 42-g germanium bolometers and achieves particle...
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Giorgio Del Castello (Istituto Nazionale di Fisica Nucleare (Italy))09/06/2025, 12:06Talk
BULLKID is a novel detector concept based on an array of particle absorbers sensed by multiplexed Kinetic Inductance Detectors (KIDs). The aim of this detector is to control the backgrounds by creating a fully active structure and by applying fiducialization
techniques.Following the encouraging results from a 20 g prototype detector,
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here we present the first operation of 3-wafer... -
Valentina De Romeri (IFIC CSIC/UV (Valencia, Spain))09/06/2025, 14:00Talk
In this talk I will discuss some implications of the first indication of nuclear recoils from solar neutrinos on a xenon target at direct detection experiments. By analyzing data from the XENONnT and PandaX-4T experiments, I will present the first constraints on new interactions and neutrino electromagnetic properties from the first CEνNS data using solar 8B neutrinos.
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Matteo Cadeddu09/06/2025, 14:22Talk
The Standard Model (SM) has consistently provided a robust description of particle interactions, yet intriguing anomalies, particularly within the neutrino sector, suggest potential areas for further exploration. In this talk, we present a comprehensive global fit of coherent elastic neutrino-nucleus scattering (CEνNS) data from COHERENT (CsI, Ar), CONUS+, TEXONO, and neutrino-electron...
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Mattia Atzori Corona (Sapienza Universita e INFN, Roma I (IT))09/06/2025, 14:44Talk
Coherent Elastic Neutrino-Nucleus Scattering (CEνNS) is a powerful tool for probing both Standard Model (SM) and beyond-SM (BSM) physics. The remarkable CEνNS observations from the CONUS+ collaboration at nuclear reactors using a germanium target explore the fully coherent regime at unprecedentedly low energies, where nuclear structure uncertainties play a marginal role.
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This talk presents... -
Matheus Hostert09/06/2025, 15:06Talk
In this talk I will present some novel ideas to constrain new forces coupled to a secluded sector of particles. To access these sectors, neutrinos must first oscillate via (ultra-)long-baseline oscillations to the dark fermions. Then, via a dark photon or similar mediators, these dark fermions induce CEvNS or nu-e scattering events in underground detectors. These scenarios also typically...
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Patrick Huber09/06/2025, 16:00Talk
We present initial results on nuclear recoil detection based on the fluorescence of color centers created by nuclear recoils in lithium fluoride. We use gamma rays, fast and thermal neutrons, and study the difference in responses they induce, showing that this type of detector is rather insensitive to gamma rays. We use light-sheet fluorescence microscopy to image nuclear recoil tracks from...
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Andrei Puiu09/06/2025, 16:22Talk
The capability to perform precision measurements of nuclear form factors or coupling constants with CEνNS relies on a precise knowledge of the incoming neutrino flux and spectrum. Isotopes decaying via electron capture (EC) represent a close-to-ideal neutrino source, thanks to the monoenergetic spectrum and the possibility of precisely measuring the source activity. However, the low energy of...
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Elizabeth Tilly09/06/2025, 16:44Talk
The Migdal In Galactic Dark mAtter expLoration (MIGDAL) detector is a state-of-the-art low energy optical time projection chamber capable of resolving low dE/dx electrons alongside very high dE/dx nuclear recoils. The goal of this experiment is to make the first observation of the Migdal effect, a rare nuclear scattering process invoked to extend the sensitivity of dark matter experiments to...
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Michael Litke (University of Hawaii at Manoa)09/06/2025, 17:06Talk
The directions of low energy nuclear recoils open windows into previously unprobed areas of physics. Specifically, directional detection of coherent elastic neutrino nucleus scattering (CEνNS) would probe for new, beyond-the-standard-model (BSM) gauge bosons involved in that interaction as well as provide a tool for distinguishing between dark matter and neutrino scattering. Currently the only...
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George Savvidis (Queen's University)09/06/2025, 17:28Talk
The NEWS-G3 experiment aims at the detection of reactor neutrinos using a 60cm-diameter Spherical Proportional Counter (SPC) at high pressure. The low energy threshold down to single-electron detection and the electron-counting capabilities, allow for the detection of low energy nuclear recoils, with an estimated event rate of 5 events/bar/day/GW in argon at 20m from the reactor core....
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Cristian Fabian Macias Acevedo (Universidad Nacional Autónoma de México)09/06/2025, 18:00Poster
Coherent CAPTAIN-Mills (CCM) is a 10 ton liquid argon scintillation detector at Los Alamos National Laboratory for the study of neutrino and beyond Standard Model physics. It is located 23 m from the stopped pion source of the Lujan Facility, and will receive $1.5\times 10^{22}$ POT in its ongoing 3-year run cycle. CCM is instrumented with 200 8-inch PMTs, of which $80\%$ are coated with...
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Ana Carolina Oliveira (Centro Brasileiro de Pesquisas Físicas)09/06/2025, 18:00Poster
The Coherent Neutrino Nucleus Interaction Experiment (CONNIE) aims to detect, for the first time, coherent elastic antineutrino-nucleus scattering (CEvNS) in silicon and probe physics beyond the Standard Model. To that end, the experiment has been taking data next to the Angra 2 nuclear power plant since mid-2021 with high-sensitivity detectors known as Skipper-CCDs. These pixelated sensors...
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Mr Lingquan Kong09/06/2025, 18:00Poster
Our research group has developed a novel approach to detect Coherent Elastic Neutrino-Nucleus Scattering (CEvNS) signals using cesium iodide (CsI) crystals operated at liquid nitrogen temperatures. This poster presents the results of comprehensive tests conducted on the CsI crystals, including low-temperature light yield, spatial uniformity of light emission, and background measurements...
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Pedro Zilves Maio Ventura (São Paulo University)09/06/2025, 18:00Poster
The COherent Neutrino-Nucleus Interaction Experiment (CONNIE) investigates coherent elastic neutrino-nucleus scattering (CEvNS) using high-resistivity silicon Skipper-CCDs at the Angra-2 nuclear reactor in Brazil. The introduction of Skipper-CCD technology has enabled an unprecedented low-energy threshold of 15 eV, significantly improving sensitivity to low-energy events and rare interactions....
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Laura Duque Herrera09/06/2025, 18:00Poster
In this work we present a study of Coherent Elastic Neutrino-Nucleus Scattering (CEvNS) with a proposed array of isotopic enriched detectors. These detectors could improve the precision of CEvNS measurements, allowing to test predictions of the Standard Model, nuclear physics and new physics scenarios, due to the correlation of the systematic uncertainties. Based on these results, we explore...
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Camila Martínez09/06/2025, 18:00Poster
The search for dark matter requires extremely sensitive detection techniques. In this context, atmospheric muons, though typically considered background, can be used as a tool for detector spatial calibration. This work is based on data from the CONNIE experiment, which employs a vertical array of CCD sensors to detect ionizing particles at a distance of 30 meters from the core of the Angra 2...
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Sara Mirthis Dantas dos Santos (Universidade Estadual de Campinas - UNICAMP)09/06/2025, 18:00Poster
The Coherent Neutrino-Nucleus Interaction Experiment (CONNIE) operates at the Angra 2 Nuclear Reactor in Brazil. Using silicon Skipper-CCDs, CONNIE aims to identify and investigate coherent elastic neutrino-nucleus scattering (CE$\nu$NS). However, background particles from various sources, combined with the large volume of data, present significant challenges, making manual analysis of...
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Tatiana LE BELLEC (IP2I)09/06/2025, 18:00Poster
The Ricochet experiment is an international collaboration that aims at detecting the CEvNS process using germanium crystal calorimeters at cryogenic temperatures. The detectors can simultaneously readout the ionization and heat energies following particle interactions occurring in the crystal. This dual measurement allows to both perform particle identification, i.e. to discriminate between...
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Lucas Magno Dantas Ramos09/06/2025, 18:00Poster
Future experiments dedicated to the detection of Coherent Elastic Neutrino-Nucleus Scattering may be powerful tools in probing light new physics. In this paper we study the sensitivity on light Z′ mediators of two proposed experiments: a directional low pressure Time Projection Chamber detector, νBDX-DRIFT, that will utilize neutrinos produced at the Long Baseline Neutrino Facility, and...
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Ms Sol Dominique Hartzstein (Departamento de Física. Buenos Aires, Argentina, Universidad de Buenos Aires, Facultad de Ciencias Exactas y Naturales)09/06/2025, 18:00Poster
The quenching factor in silicon is a fundamental parameter for particle physics experiments that detect nuclear recoils. This is particularly critical for experiments employing CCD sensors as target materials—such as CONNIE and Atucha—which rely on it to convert ionization signals into nuclear recoil energies. Its importance extends beyond neutrino detection, playing a central role in dark...
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Seung Mok Lee (Carnegie Mellon University)09/06/2025, 18:00Poster
After the detection of CE$\nu$NS, the COHERENT collaboration is exploring new physics by precisely measuring the process. However, the uncertainty of the neutrino flux normalization is limiting the precision. To reduce the uncertainty, a heavy water (D$_{2}$O) detector has taken data at the Spallation Neutron Source (SNS) at Oak Ridge National Laboratory (ORNL) since 2023. By utilizing the...
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Nicola Cargioli10/06/2025, 09:00Talk
Since its first observation in 2017, Coherent Elastic Neutrino-Nucleus Scattering (CEvNS) has proven to be an effective method for testing the Standard Model of particle physics and searching for potential indications of new physics at low energies. In recent years, substantial progress has been made, including the first detection of CEvNS from reactor antineutrinos, as well as from solar...
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Oleksandr Tomalak10/06/2025, 09:22Talk
To consistently incorporate radiative corrections in coherent elastic neutrino-nucleus scattering (CEvNS), we develop and apply an effective field theory framework to provide precise predictions for CEvNS cross sections and neutrino flavor-dependent cross-section ratios for spin-0 nuclei. Additionally, I analyze (anti)neutrino energy spectra from radiative muon, pion, and kaon decays, which...
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Dr Dimitrios Papoulias (IFIC (CSIC/Valencia U.))10/06/2025, 09:44Talk
We present nuclear structure calculations adopting a novel hybrid nuclear model, combining the nuclear shell model and the microscopic quasiparticle-phonon model [1]. The predictivity of the hybrid model is tested by computing inelastic neutral-current neutrino-nucleus scattering cross sections off the stable thallium isotopes, taking also into account the effect of nuclear recoil energy. The...
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Martin Gonzalez-Alonso (CERN)10/06/2025, 10:06Talk
We demonstrate that CEνNS measurements at spallation sources are valuable probes of muon-decay physics. Using COHERENT data we derive the first constraint on the Michel parameters governing the $\bar\nu_\mu$ energy distribution. We also discuss future sensitivities and assess the implications for the Lorentz structure of the interactions mediating muon decay. Talk based on 2502.18175 and ongoing work.
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Prof. Henry Wong (Institute of Physics, Academia Sinica)10/06/2025, 11:00Talk
We will present a retrospective account of the TEXONO program on coherent neutrino nucleus scattering at the Kuo-Sheng Reactor Neutrino Laboratory in Taiwan with sub-keV germanium ionization detectors [1]. The latest limits [2] and the various spinoff-impacts [3] will be discussed. We would provide updates on quantifying the quantum-mechanical coherency effects of the interactions [4]....
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Dr Litao YANG (Tsinghua University)10/06/2025, 11:18Talk
The RECODE (Reactor neutrino COherent scanning Detection Experiment) uses two sets of high-purity germanium arrays to accurately measure the CEvNS process of reactor neutrinos. The high-purity germanium technology used comes from the PPC germanium detector technology developed by CDEX in dark matter experiments. The currently confirmed experimental site is located at Sanmen Nuclear Power Plant...
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Prof. Manfred Lindner (Max-Planck-Institut fuer Kernphysik, Heidelberg, Germany)10/06/2025, 11:30Talk
The talk will cover latest results of the CONUS+ experiment. In addition the current status, an outlook and the physics perspectives will be covered.
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Alexey Lubashevskiy (JINR)10/06/2025, 11:55Talk
The $\nu$GeN experiment is aimed to studying neutrino properties in the close vicinity of the reactor core of the Kalinin Nuclear Power Plant (KNPP) at Udomlya, Russia. The experimental setup is installed under reactor unit #3 of KNPP at the moving platform, which allows changing the distance from the center of the 3.1 GW$_{th}$ core from 11.1 to 12.2 m. In this way, we obtain an enormous...
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Janina Dorin Hakenmueller (Duke University)10/06/2025, 12:17Talk
For a successful CEvNS detection, a detector with a low enough noise threshold is required. HPGe spectrometers are highly suitable for this task due to the large number of charge carriers created in particle interactions, the high level of radiopurity that can be achieved and the possibility to have kg-sized detector masses. The developments in the last decades on noise levels make it feasible...
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Dr Peter Denton (Brookhaven National Laboratory)10/06/2025, 14:00Talk
In neutrino oscillation physics numerous exact degeneracies exist under the name LMA-Dark. These degeneracies make it impossible to determine the sign of $\Delta m^2_{31}$ known as the atmospheric mass ordering with oscillation experiments alone in the presence of new neutrino interactions. The combination of different measurements including multiple oscillation channels and neutrino...
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Eduardo Peinado10/06/2025, 14:22Talk
Searching for dark matter and new light mediators enters a precision era driven by rapid advances in coherent elastic neutrino-nucleus scattering (CEνNS) experiments and direct detection of dark matter. This talk will focus on U(1)′ extensions of the Standard Model. We will explore how CEνNS experiments constrain this sector and how this complements the direct detection results when the light...
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Mr Anirban Majumdar (Indian Institute of Science, Education & Research - Bhopal)10/06/2025, 14:44Talk
With the rapid advancement of low-energy neutrino experiments, coherent elastic neutrino-nucleus scattering (CE$\nu$NS) has become a powerful tool for precision studies in both Standard Model (SM) and beyond-the-Standard-Model physics. I will present our recent works based on recent and projected phenomenological studies of CE$\nu$NS at two key facilities: the CONUS+ reactor experiment |1| and...
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Thomas Rink (Karlsruhe Institute of Technology (KIT))10/06/2025, 15:05Talk
In the last years, the long predicted Standard Model reaction channel of coherent elastic neutrino-nucleus scattering (CEvNS) has been confirmed by measurements of (anti-)neutrinos emitted from pion decay at rest sources and nuclear reactors, also with multiple target materials. As we slowly transition with the next generation of experiments from first observations to precision measurements,...
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Mr Dacheng Xu (Columbia University)10/06/2025, 16:00Talk
Solar neutrinos interacting with nuclei in dark matter detectors through coherent elastic neutrino-nucleus scattering (CEvNS), often referred to as the 'neutrino fog,' presents a significant challenge to direct DM detection efforts. The XENONnT detector, known for its large exposure and low background, offers an exceptional opportunity to investigate this interaction. Utilizing data from...
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Ibles Olcina Samblas10/06/2025, 16:22Talk
The detection of solar neutrinos via coherent elastic neutrino-nucleus scattering (CEvNS) in liquid xenon time projection chambers (TPCs) represents a major milestone in neutrino physics, offering a new lens into the cosmos. Over the past two decades, liquid xenon TPCs have driven dramatic progress in rare-event detection. In particular, the LUX-ZEPLIN (LZ) experiment, operating a two-phase...
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Morgan McCarthy10/06/2025, 16:44Talk
The LUX-ZEPLIN (LZ) experiment is a low-threshold, low-background dark matter detector deployed 4850 feet underground at the Sanford Underground Research Facility in Lead, South Dakota, USA. The primary detector volume is a time projection chamber (TPC) containing 7 tonnes of liquid xenon. CEvNS interactions in this volume deposit O(1) keV of energy, a regime to which LZ is sensitive. Via...
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Luca Pattavina (UNIMIB & INFN)10/06/2025, 17:06Talk
Core-collapse Supernovae (SN) release nearly all their binding energy as neutrinos. RES-NOVA tackles a major challenge in astroparticle physics by introducing a novel detection approach using cryogenic detectors made from ultra-pure archaeological lead (Pb). The innovation lies in exploiting Coherent Elastic Neutrino-Nucleus Scattering (CEvNS), which offers a cross-section ~10⁴ times larger...
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Jeremy Lu10/06/2025, 17:28Talk
As part of the COHERENT collaboration’s efforts toward precision CEvNS measurements since the first observation in 2017, COH-Ar-750 is the upcoming ton-scale liquid argon detector at Neutrino Alley, located at the Oak Ridge National Laboratory’s Spallation Neutron Source (ORNL SNS). It will replace its smaller predecessor, the CENNS-10 detector, which first observed CEvNS on argon in 2019 and...
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Carla Bonifazi (ICAS-ICIFI-UNSAM/CONICET)11/06/2025, 09:00Talk
The CONNIE experiment began operating with Skipper-CCDs in 2021, marking the first use of Skipper technology in a reactor neutrino experiment. This technology enables charge measurements with sub-electron resolution, enhancing the ability to detect and characterize low-energy signals. As a result, the experiment achieved a detection threshold as low as 15 eV. Data collected with exposures of...
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Eliana Depaoli11/06/2025, 09:22Talk
Atucha-II is a short baseline neutrino experiment that employs 2.2 g of Skipper-CCD. The detector, installed inside the containment sphere of the 2 GWth Atucha II nuclear reactor at a distance of 12 m from the core, has been operating since December 2021. It currently achieves a readout noise of ~ 0.20 e− by averaging 300 samples of the collected charge in each pixel, with a reactor-OFF...
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Dmitry Akimov11/06/2025, 09:44Talk
The RED-100 is a two-phase noble gas emission detector build for observation of a coherent elastic neutrino-nucleus scattering (CEvNS) in reactor antineutrino interactions with matter. The fist data taking run with LXe target was carried out at the Kalinin nuclear power plant in 2022, and the final results are given. The RED-100 experiment is currently in preparation to the Phase II, with LAr....
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Shengchao Li (Westlake University)11/06/2025, 10:06Talk
The neutrino-nucleus coherent scattering (CEνNS), known as CEνNS, has the largest cross-section among all interaction channels for MeV neutrinos, making it the most promising way to remotely monitor nuclear reactors. A precise determination of the CEvNS cross section has a significant impact on understanding the properties of neutrinos and constraining new physics beyond the standard model....
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Chenguang Su (University of Chinese Academy of Sciences)11/06/2025, 10:28Talk
This presentation will detail the latest advancements in the development and characterization of a 6.6 kg proto-type CryoCsI detector, comprising two 3.3 kg cesium iodide (CsI) crystals operated at around 90K. Key performance metrics of the detector, including light yield optimization, spatial uniformity of signal response, and long-term stability under sustained cryogenic conditions, will be...
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Gonzalo Sanchez Garcia (Instituto de Física Corpuscular CSIC/UV (Valencia, Spain))11/06/2025, 11:15Talk
The detection of CEvNS from reactor sources represents a unique opportunity to test beyond the Standard Model physics in the neutrino sector. In this talk, we present the phenomenological implications of the first CONUS+ observation of CEvNS for different new physics scenarios, including non-standard interactions, electromagnetic properties of neutrinos and light mediators. The results...
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Yuber F Perez-Gonzalez11/06/2025, 11:37Talk
As direct detection experiments approach sensitivities where neutrinos become an irreducible background due to their interactions via coherent elastic neutrino-nucleus scattering (CEvNS), they pose a fundamental limitation in the search for Dark Matter. Given that CEvNS has only recently been observed, there remains significant room for new physics beyond the Standard Model (BSM) to alter the...
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Youssef Sarkis Mobarak (ICN-UNAM)11/06/2025, 11:59Talk
Understanding ionization efficiency at energies below 1 keV, both in pure crystals and in noble liquid detectors, provides an essential analytical tool for accurate measurements of Coherent Elastic Neutrino-Nucleus Scattering (CEvNS) and the processes involved in the search for dark matter. This presentation will address theoretical concepts related to the Lindhard integral equation and the...
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sergey pereverzev (LLNL)11/06/2025, 12:21Talk
The detection of nuclear recoils caused by elastic coherent scattering of solar and reactor neutrinos is of significant scientific and practical importance, representing a key milestone in the direct search for dark matter particles. While modern detectors are sensitive to registering these small energy depositions, a challenge lies in discriminating particle interactions from energy...
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Eli Mygatt Ward11/06/2025, 14:00Talk
At Oak Ridge National Laboratory (ORNL), the COHERENT collaboration has built a heavy water Cherenkov detector to measure the neutrino flux coming from the Spallation Neutron Source (SNS) via the scattering of neutrinos on deuterium nuclei, with the primary aim of improving the precision of past and future CEvNS measurements. Detector construction was completed and measurements began in the...
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Ana Zaalishvili (Duke University, Triangle Universities Nuclear Laboratory)11/06/2025, 14:22Talk
In 2015, the COHERENT collaboration attempted to measure the electron-neutrino charged current (CC) cross-section on lead. The Eljen cell and the Neutrino Cubes detectors hunted for the Neutrino Induced Neutrons (NINs) produced by this process. The results indicated a surprisingly small cross-section — less than one third of the predicted signals were observed. Understanding the NINs...
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Marisol Chávez Estrada (Instituto de Ciencias Nucleares UNAM)11/06/2025, 14:44Talk
The Coherent CAPTAIN-Mills (CCM) experiment, located at Los Alamos National Laboratory, employs a 10-ton liquid argon detector to study neutrino interactions, search for dark matter candidates, and explore physics beyond the Standard Model.
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In this work, we present ongoing efforts towards enabling the first measurement of low-energy charged-current (CC) scattering of electron neutrinos on... -
Leire Larizgoitia (DIPC)11/06/2025, 15:06Talk
For the CE$\nu$NS experiments that we are developing at the Donostia International Physics Center (DIPC), it is essential to characterize the neutrons produced at the facility. The European Spallation Source (ESS) being one of the promising experimental facilities for the observation of CE$\nu$NS, detailed simulations of the neutron background at the ESS have been performed. However, as in...
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Francesca Dordei (INFN, Cagliari (IT))11/06/2025, 16:00
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Matthew Green (NC State University)11/06/2025, 16:30
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Diego Aristizabal (Universidad Tecnica Federico Santa Maria (USM))Talk
I will discuss a few aspects of electroweak theory relevant for neutrino scattering on different targets. The presentation will follow historical developments starting with the discovery of the neutron, the establishment of Fermi beta theory and finishing with the SM electroweak sector. A few aspects of effective theories will be covered. And an explicit calculation of the CEvNS cross section,...
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Dario Rodrigues (Departamento de Física. Buenos Aires, Argentina, Universidad de Buenos Aires, Facultad de Ciencias Exactas y Naturales y CONICET - Universidad de Buenos Aires, Instituto de Física de Buenos Aires (IFIBA). Buenos Aires, Argentina)Talk
This three-lecture series will explore the construction and interpretation of confidence intervals within the context of particle physics. We will begin by defining the likelihood function and highlighting its central role in statistical inference. Through a concrete example, we will examine how the likelihood depends on the number of observed events, with special attention to the challenges...
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Yuber F Perez-GonzalezTalk
In this project, we will explore recent results from the CONUS+ experiment and examine how they can be used to constrain physics beyond the Standard Model. In particular, we will focus on scenarios involving non-standard neutrino interactions, neutrino magnetic moments, and light mediators. Our analysis will be guided by the framework and methodology presented in...
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Raimund Johann Strauss (Technische Universitaet Muenchen (DE))Talk
In these lectures, I will discuss key milestones in neutrino physics, from the first detections to current large-scale experiments like DUNE. I will then present the main detector technologies used in neutrino research and the background challenges they face. Finally, I will review a decade of CEvNS experiments, from COHERENT to recent developments in CONUS.
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Prof. Yufeng Li (Institute of High Energy Physics, Beijing)Talk
Sterile neutrinos that couple to the Standard Model via the neutrino magnetic dipole portals have been extensively studied at various experiments. In this work, we scrutinize these interactions for sterile neutrinos in the mass range of 0.1--50 MeV through the nuclear and electron recoils at various neutrino scattering experiments. For the e-flavor specific dipole portal, we demonstrate that...
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Diego Aristizabal (Universidad Tecnica Federico Santa Maria (USM))Talk
In the first part of this project nuclear form factor parametrizations will be discussed. That discussion will then be followed by the determination of neutrino fluxes from pion decay-at-rest and from nuclear reactors. The final part of the project will involve a full numerical implementation of the CEvNS cross section and the calculation of the event rate in both, fixed target and reactor facilities.
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Dr Tulasi Subedi (Concord University)Talk
The COHERENT experiment at the Spallation Neutron Source (SNS) at Oak Ridge National Laboratory consists of several detectors designed to measure coherent elastic neutrino nucleus scattering from a pion-decay-at-rest neutrino source. A significant source of uncertainty in these results is the 10% estimated uncertainty in the neutrino flux from the SNS target. To reduce this uncertainty to...
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Dario Rodrigues (Departamento de Física. Buenos Aires, Argentina, Universidad de Buenos Aires, Facultad de Ciencias Exactas y Naturales y CONICET - Universidad de Buenos Aires, Instituto de Física de Buenos Aires (IFIBA). Buenos Aires, Argentina)Talk
This two-session course will provide an in-depth exploration of Skipper-CCD detector performance and the techniques used to analyze their data. We will begin by reviewing the concept of noise in CCD detectors and how the Skipper architecture enables significant improvements in readout noise. Participants will learn how to quantify this noise using real images. We will then survey the various...
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