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Prof. David Caratelli (UC Santa Barbara)29/06/2026, 10:00
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Dr Peter Denton (Brookhaven National Laboratory)29/06/2026, 10:30
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Laura Johanna Fields (University of Notre Dame (US))29/06/2026, 13:30
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Brooke Russell (Massachusetts Institute of Technology)29/06/2026, 15:30
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29/06/2026, 17:00
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Prof. Phillip Barbeau30/06/2026, 09:001
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Brooke Russell (Massachusetts Institute of Technology)30/06/2026, 10:45
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Laura Johanna Fields (University of Notre Dame (US))30/06/2026, 13:30
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Dr Peter Denton (Brookhaven National Laboratory)30/06/2026, 14:45
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Dr Teppei Katori (King's College London), Teppei Katori (King's College London)30/06/2026, 16:30
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Teppei Katori (King's College London), Dr Teppei Katori (King's College London)01/07/2026, 09:00
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Prof. Phillip Barbeau01/07/2026, 11:00
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Lauren Yates (University of Notre Dame), Dr Lauren Yates (Fermilab)01/07/2026, 14:00
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Matheus Hostert (University of Iowa)01/07/2026, 16:00
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01/07/2026, 17:30
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Lauren Yates (University of Notre Dame), Dr Lauren Yates (Fermilab)02/07/2026, 09:00
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Matheus Hostert (University of Iowa)02/07/2026, 11:00
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Graciela Beatriz Gelmini (University of California Los Angeles (US))02/07/2026, 14:00
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02/07/2026, 16:00
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Graciela Beatriz Gelmini (University of California Los Angeles (US))03/07/2026, 09:00
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03/07/2026, 11:00
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Chami Amarasinghe03/07/2026, 14:00
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06/07/2026, 09:00
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06/07/2026, 11:00
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06/07/2026, 14:00
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08/07/2026, 11:00
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08/07/2026, 16:00
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09/07/2026, 09:00
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09/07/2026, 10:45
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09/07/2026, 13:30
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09/07/2026, 15:15
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10/07/2026, 09:00
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Adam Wong (University of Sussex)
The AntiMatter-OTech (AM-OTech) project, funded by the European Innovation Council (EIC) and UK Research and Innovation (UKRI), is a pioneering initiative in nuclear security and reactor diagnostics. Led by a collaboration of European academic institutions and EDF, AM-OTech explores the use of antineutrinos from nuclear fission as a non-intrusive, real-time probe for monitoring industrial...
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Anthony Kelly (Indiana University Bloomington)
Previous neutrino experiments have observed a significant excess or deficit in electron neutrinos suggesting a deviation from three flavor oscillations. One of these experiments is MiniBooNE which was based at Fermilab and saw an excess of electron-neutrino-like events from the Booster Neutrino Beam (BNB). Other anomalies include the gallium and reactor anomalies which saw a disappearance of...
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Jason Chapman (University of North Carolina at Chapel Hill)
The MAJORANA DEMONSTRATOR (MJD) is a low-background experiment that searched for neutrinoless double-beta decay ($0\nu\beta\beta$) in high-purity germanium (HPGe) detectors enriched to $>$90% in $^{76}$Ge. In addition to the search for $0\nu\beta\beta$, MJD's low-background configuration makes it sensitive to several other beyond standard model (BSM) phenomena, including quantum mechanical...
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Justin Mitchell
J. M. Mitchell, A. R. Fazely — Southern University and A&M College, IceCube Collaboration
The IceCube Neutrino Observatory detects high-energy astrophysical neutrinos through Cherenkov radiation produced when secondary charged particles travel through Antarctic ice. The IceCube Upgrade has recently deployed new optical modules along additional strings in the DeepCore region, extending the...
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Ali Kurmus (University of Washington), Ms Yao Yin (University of Washington)
The Project 8 neutrino mass experiment envisions a multi-phase approach to reach 40meV neutrino mass sensitivity using Cyclotron Radiation Emission Spectroscopy (CRES). The first two phases demonstrated the principle of CRES and produced the first CRES spectrum of the tritium beta-decay endpoint. One of the primary goals of the third phase is to demonstrate sub-eV energy resolution near the...
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Sayan Kr Das (University of Sussex)
LiquidO is an opaque scintillator-based radiation detection technology which aims to
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overcome some of the drawbacks of the transparent detectors. Instead of letting the
scintillation photons propagate freely through the detector, it uses an opaque medium
with low scattering length to confine the light stochastically near its creation point.
The scattered photons are then collected by an... -
Erwan LE BLEVEC
The Hyper-Kamiokande detector represents the next generation of neutrino observatories, following in the lineage of the Kamiokande and Super-Kamiokande experiments. With significantly enhanced sensitivity, Hyper-Kamiokande will support a diverse and ambitious physics program, including searches for proton decay, studies of solar neutrinos under non-standard interactions, and the...
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Juan David Villamil (UV - IFIC - CSIC)
The NEXT collaboration searches for neutrinoless double beta decay (0νββ) using high-pressure xenon gas Time Projection Chambers (TPCs). A key advantage of this technology is the topological reconstruction of 0νββ events—a track with two highly ionizing "blobs" at its ends—which provides exceptional background rejection. However, high transverse electron diffusion in pure xenon blurs this...
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Seung Mok Lee (Carnegie Mellon university)
Coherent elastic neutrino–nucleus scattering (CEνNS) has opened a new avenue for new-physics searches. The COHERENT collaboration leads precision measurements of CEνNS at Oak Ridge National Laboratory (ORNL); however, these measurements are currently limited by the 10% uncertainty in the neutrino flux. To better constrain the neutrino flux, we have deployed a pair of water Cherenkov detectors...
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Nicholas Craft (Drexel University)
The PRecision Oscillation and SPECTrum (PROSPECT) experiment is a short-baseline reactor experiment that was located at the High Flux Isotope Reactor (HFIR), an 85MW highly-enriched uranium reactor at Oak Ridge National Laboratory (ORNL). A goal of PROSPECT is to measure the absolute neutrino flux, a measurement that is dependent on several detector characteristics and variables that all must...
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Paige Trevarrow (University of Kansas)
The Deep Underground Neutrino Experiment (DUNE) is a long baseline oscillation experiment that will test the three-flavor neutrino paradigm and measure all of its parameters, including mass ordering and the CP-violating phase, as part of a broad physics program. DUNE will utilize a powerful wideband spectrum neutrino beam, four 10 kt Liquid Argon Time Projection Chamber (LArTPC) Far Detector...
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Xingyun Yang
The ongoing Jiangmen Underground Neutrino Observatory (JUNO) and the upcoming Hyper-Kamiokande (HK) and Deep Underground Neutrino Experiment (DUNE) are expected to detect the neutrinos in the Diffuse Supernova Background (DSNB). However, the DSNB signal is similar to neutrinos from the annihilation of dark matter at the MeV scale. We study the neutrino flux from dark matter annihilation and...
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AJ Nielsen (University of California Irvine (US))
The 2x2 Demonstrator and the Full Scale Demonstrator (FSD) are prototypes of the Liquid Argon Time Projection Chamber (ND-LAr) that will be used in the Near Detector complex of the Deep Underground Neutrino Experiment (DUNE). These detectors incorporate several innovations to cope with the high level of pile-up expected at ND-LAr, such as the adoption of a modular design and the use of a...
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Yao Yin (University of Washington)
The Project 8 experiment is pioneering cyclotron radiation emission spectroscopy (CRES) to measure the energy spectrum of beta electrons emitted in the decay of tritium, with the goal of improving sensitivity to the neutrino mass to 0.04 eV. The current prototype, the Cavity CRES Apparatus (CCA), will be the first CRES detector with resonant cavity geometry, enabling scalability, improved...
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Radovan Beno (Institute of Physics of the Czech Academy of Sciences)
In the electroweak theory of particle physics, the neutrinos are electromagnetically (EM) neutral and lack direct tree-level EM interactions, they are, however predicted to possess small charge radii generated by radiative corrections. What is more in theories beyond Standard Model (BSM) massive neutrinos could exhibit anomalous EM properties such as magnetic and electric moments. A primary...
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Dario Pullia (CERN, APC)
The Deep Underground Neutrino Experiment (DUNE) is a next-generation long-baseline oscillation experiment, aiming to address fundamental questions about neutrino oscillations, CP violation, and the origin of matter–antimatter asymmetry. At CERN, the ProtoDUNE detectors play a crucial role in preparing for the DUNE far detector construction and operation through extensive testing of detector...
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Camilo Cortes Parra (IFIC (CSIC - UV))
The NEXT experiment aims to conduct a sensitive search of the neutrinoless
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double beta decay (ββ0ν) in $^{136}$Xe, using high-pressure gas electroluminescent
time projection chambers (HP-ELTPCs). The NEXT-White detector, a first
radiopure demonstrator, was operated between 2016 and 2021 in the Canfranc
Underground Laboratory (LSC). This detector demonstrated the capabilities
of the... -
Diego Martinez-Montiel (University of Tennessee)
Galactic cosmic rays (GCRs) are continuously modulated in the heliosphere by solar wind structures and transient disturbances, producing measurable variations in secondary cosmic ray (SCR) fluxes at Earth. We present a multi-year analysis of SCR in Mexico City, based on observations from a scintillator-based muon detector, which measured an average flux of (97.5 $\pm$ 3.0) m$^{-2}$ s$^{-1}$...
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Rumman Neshat (University Of Utah)
The IceCube Neutrino Observatory is a cubic-kilometer detector located at the South Pole that utilizes the deep Antarctic ice as a medium for neutrino interactions. The baseline array consists of 5,160 Digital Optical Modules (DOMs) designed to detect Cherenkov radiation. The IceCube Upgrade has integrated six additional, densely instrumented strings featuring over 500 next-generation optical...
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Nayan Babu (Louisiana State University)
The Tokai-to-Kamioka (T2K) experiment is a state-of-the-art long-baseline neutrino experiment with the primary objective of measuring neutrino oscillation parameters. The latest oscillation measurements have shown that the dominant systematic uncertainty arises from the modeling of neutrino interactions. The dominant interaction channel at the T2K beam energy is the charged-current interaction...
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Maël Martin (Centre National de la Recherche Scientifique (FR))
The Deep Underground Neutrino Experiment (DUNE) is a next-generation long baseline neutrino experiment. By using Liquid Argon Time Projection Chamber (LArTPC) detectors to detect accelerator GeV-scale neutrinos, DUNE's main physics goals are to measure the CP-violating phase, determine the neutrino mass ordering and resolve the $\theta_{23}$ octant. Besides these observations at high energy,...
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Yoshita Dabburi (Queen Mary University of London)
The Short-Baseline Near Detector (SBND) is a 112-ton Liquid Argon Time Projection Chamber (LArTPC) positioned 110 meters from the Booster Neutrino Beam (BNB) target at Fermilab. As the near detector of the Short-Baseline Neutrino (SBN) program, it is capable of recording around 3 million neutrino interactions per year. This enables precise measurements of unoscillated neutrino event rate and...
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Dylan Brown-Simms (Drexel University)
Precision and control of neutrino flux predictions is necessary to optimize the sensitivity of accelerator-based neutrino measurements. The EMPHATIC collaboration’s goal is to reduce uncertainties in neutrino flux predictions. EMPHATIC achieves this goal by measuring hadron scattering and production cross-sections with a compact high precision spectrometer at the Fermilab Test Beam Facility....
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Andrea Roche Fernández (IFIC (CSIC-UV))
The Deep Underground Neutrino Experiment (DUNE) is a next-generation international experiment that aims to advance our understanding of neutrinos. By combining a powerful wide-band neutrino beam and a high-performance Near Detector complex at Fermilab with a massive Far Detector (FD) located 1300 km away at the Sanford Underground Research Facility (SURF), DUNE will be able to determine the...
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Saandeep Unnikrishnan (University of Kansas)
The Short Baseline Near Detector (SBND) is a 112 ton of liquid argon time projection chamber (LArTPC), and it is the near detector of the Short-Baseline Neutrino (SBN) program located at Fermilab, USA. The primary goal of the program is to perform high-precision searches for neutrino oscillations in the short-baseline regime and address the sterile neutrino hypothesis. This work focuses on the...
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Clara Saia
The ICARUS detector, a key component of the Short Baseline Neutrino (SBN) Program at Fermilab, consists of two identical T300 modules filled with liquid argon. It is equipped with a Light Detection System (LDS) based on 360 8-inch Hamamatsu R5912-MOD photomultiplier tubes (PMTs) arranged behind the wire planes to collect Vacuum Ultraviolet (VUV, ~128 nm) scintillation light. Operating under...
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River Govin (Indiana University)
We investigate the phenomenological signatures of Lorentz and CPT symmetry violation within two-neutrino (2νββ) and neutrinoless (0νββ) double beta decay. Using the Standard-Model Extension (SME) framework, we analyze how Lorentz-violating operators distort standard decay rates. For 2νββ decay, these violations manifest as precise spectral distortions in the continuous electron energy...
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Salvador Aguilar (Laboratorio Internacional de Partículas Elementales, Departamento de Física, DCeI, CL. UGTO)
The detection of cosmic radiation is a fundamental tool for studying phenomena associated with particle physics, astrophysics, and instrumental applications. This work presents the design, construction, characterization, and simulation of a modular Cherenkov detector based on a cylindrical polymethyl methacrylate (PMMA) rod for recording atmospheric muons produced by cosmic radiation. The...
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Brandon Weiss (Columbia University)
We present PROfit, a new open-source C++ framework designed for efficient and robust estimation of neutrino oscillation parameters, systematic uncertainties, and beyond-the-Standard-Model (BSM) physics, with particular emphasis on reliable global optimization in high-dimensional parameter spaces and rigorous treatment of systematics. Initially developed for the Short-Baseline Neutrino (SBN)...
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Laksha Das (University of Iowa)
In this work, we present a new evaluation of the prompt atmospheric lepton flux, which includes an intrinsic charm component in cosmic ray–air interactions. The intrinsic charm enhances the forward production of $\bar{D}^0$, $D^-$, and $\Lambda_c$, and subsequently the atmospheric lepton fluxes. An intrinsic charm-induced enhancement of the prompt muon flux leads to a corresponding enhancement...
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Emerson Bannister (University of Sussex)
The NOvA (NuMI Off-Axis electron neutrino Appearance) Experiment is a long-baseline neutrino oscillation experiment composed of two functionally identical detectors, a 300 ton Near Detector, and a 14 kton Far Detector separated by 809 km and placed 14 mrad off the axis of the NuMI neutrino beam created at Fermilab. This configuration enables NOvA's rich neutrino physics program, which includes...
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Vojtech Vasicek (Czech Technical University in Prague, FNSPE, Institute of Physics of the Czech Academy of Sciences)
This work focuses on the reconstruction and identification of Michel electron signals produced in the decay of stopped cosmic muons in a prototype detector of the DUNE experiment. It exploits a combination of data from the Time Projection Chamber (TPC) and the Photon Detection System (PDS), which together provide information on the ionization charge and scintillation light generated by...
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Martina La Rosa (Università degli studi di Padova, INFN Padova)
The explosion of the type II supernova SN1987A provides a unique laboratory to constrain novel energy-loss mechanisms and possible extensions of the standard properties of neutrinos. Here we revisit, in light of modern 1D supernova simulations and advancements in the understanding of the Milky Way magnetic field, a detailed analisys on the production and emission of right-handed neutrinos νR...
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Ryan Chaudoin (UCSB)
MicroBooNE is a Liquid Argon Time Projection Chamber used at Fermilab to detect neutrinos as part of the Short Baseline Neutrino program. MicroBooNE uses 32 photomultiplier tubes to detect scintillation light created by neutrino interactions. In this study, we investigate the distinction between protons and muons using scintillation light signals: both the total light yield of the events and...
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Alejandra Maria Granados Hernandez (Michigan State University)
The IceCube Neutrino Observatory, located at the South Pole, covers a cubic kilometer of Antarctic ice to detect astrophysical neutrinos in the TeV-PeV energy range. While IceCube has recently identified the existence of a diffuse flux of neutrinos originating from the Galactic Plane, the identification of individual sources within the Milky Way remains elusive. Both neutrinos and gamma rays...
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Kyra Mossel (JGU Mainz)
Double beta plus decay is a rare nuclear process whose neutrinoless mode would provide evidence for lepton number violation and the Majorana nature of neutrinos. Experimental searches are particularly challenging due to the low decay rates, limited isotope abundances, and complex event signatures involving positrons and annihilation photons.
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NuDoubt$^{++}$ is a hybrid opaque scintillation... -
Philipp Anton Schwarz (Johannes Gutenberg Universitaet Mainz (DE))
The reconstruction of neutrino energy from final state particles produced in neutrino-nucleus interaction is a crucial input for the precision measurement of neutrino oscillations in present (T2K, NOVA) and future (HyperKamiokande, DUNE) experiments.
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While the neutrino energy reconstruction for Quasi-Elastic reactions has been historically made by detecting the outgoing charged lepton only,... -
Jinyoung Kim (Chung-Ang University (CAU) / CUP, IBS)
The COSINE-100 experiment uses NaI(Tl) detectors to search for WIMP dark matter and to test the DAMA/LIBRA annual modulation claim.
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A model-independent analysis of six years of data shows no evidence of annual modulation, excluding the DAMA/LIBRA signal at a significance greater than 3σ.
A model-dependent WIMP analysis based on three years of data further excludes the DAMA/LIBRA allowed... -
Aedan Cataldo (University of Notre Dame)
The Short-Baseline Near Detector (SBND) is a Liquid Argon Time Projection Chamber (LArTPC) located at Fermilab. It utilizes electrons ionized by passing particles inside the detector to create 3D reconstructions of interactions. This is achieved by drifting ionized electrons towards the instrumented wire planes.
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Structurally, the cathode can be mapped using cosmic ray muons by using... -
Henry Truelson (Colorado State University)
The flavor puzzle remains one of the biggest open questions in particle theory to date and the upcoming results from precision neutrino experiments like DUNE, HK, JUNO, KATRIN, and cosmology will have a large impact on its potential solution in the future. We show how five popular classes of flavor model predictions relate to these expected measurements. We discuss correlations,...
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Fatima Houria
The Jiangmen Underground Neutrino Observatory (JUNO) is a multipurpose neutrino experiment located in Kaiping (south China), ∼53 km distant from Yangjiang and Taishan Nuclear Power Plants, with the main goal of determining the Neutrino Mass Ordering (NMO). The experiment is located 650 m underground and the main detector consists of a central transparent acrylic sphere, with a ∼ 35 m diameter,...
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Mariya Mollova (APC-Paris)
The Deep Underground Neutrino Experiment (DUNE) is a next-generation long-baseline neutrino experiment designed to address the fundamental open questions in neutrino physics. Its Far Detector, located 1300 km from the neutrino source and 1.5 km underground, will comprise four massive liquid argon time projection chamber (LArTPC) modules, one of which will be equipped with the Vertical Drift...
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Youwei Liu (The Ohio state University)
The Radio Neutrino Observatory in Greenland (RNO-G) is an in-ice antenna array with 35 planned stations, designed to detect ultra-high-energy (UHE) neutrinos interacting in the ice in Greenland. RNO-G is designed to detect the radio signal from Askaryan radiation produced by UHE neutrinos (either astrophysical or cosmogenic in origin) when they interact in the ice sheet. Neutrinos are...
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Yufan Qie (Columbia University)
A nearby core-collapse supernova would produce a burst of neutrinos spanning a timescale of O(seconds), carrying information about both stellar collapse dynamics and fundamental neutrino properties. The Short-Baseline Near Detector (SBND) is a 112-ton liquid argon time projection chamber (TPC) operating on the Earth’s surface, 110 meters from the Booster Neutrino Beam (BNB) target at Fermilab....
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Dr Sang Yong KIM (Chonnam National University)
The Reactor Experiment for Neutrinos and Exotics (RENE) aims to search for sterile neutrinos in the Δm²≈2 eV² region, motivated by the Reactor Antineutrino Anomaly. The detector consists of a cylindrical target volume filled with 270 liters of Gd-loaded liquid scintillator (Gd-LS), and a surrounding box-shaped gamma catcher with approximately 3,000 liters of liquid scintillator (LS). The...
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Lea Schlickmann
The Wavelength-shifting Optical Module (WOM) is a novel optical sensor developed to enhance the sensitivity of neutrino detectors to ultraviolet (UV) Cherenkov light. It employs wavelength-shifting and light-guiding technology to efficiently detect UV photons that are otherwise difficult to capture with conventional sensors. Each WOM consists of a quartz tube coated with a wavelength-shifting...
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Annalea Corallo (Universita e INFN, Ferrara (IT))
The Short-Baseline Near Detector (SBND) is the near detector of the Short-Baseline Neutrino Program, located only 110 m away from the Booster Neutrino Beam (BNB) target at Fermilab (Illinois, USA). SBND employs key detection technologies: a 112-ton Liquid Argon Time Projection Chamber for ionization electrons, an advanced Photon Detection System (PDS) made up of photomultiplier tubes and...
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Daniel Chris Xing (University of Colorado Boulder (US))
The Deep Underground Neutrino Experiment (DUNE) is an international particle physics experiment looking to answer some of the largest unanswered questions in neutrino physics. DUNE uses a high-power neutrino beam produced at Fermi National Accelerator Laboratory (Fermilab) and consists of a near detector (ND), also located at Fermilab, and a far detector (FD) 1300 km away at the Sanford...
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Haowei Zheng (Stony Brook University)
This poster summarises ongoing work on the 2nd iteration combined analysis of T2K beam and SK atmospheric neutrinos. The analysis aims to constrain parameters of the PNMS matrix, in particular the leptonic CP violation phase, via complementarity between beam and atmospheric neutrino data. T2K Near Detector will reduce cross-section systematics for SK atmospheric data while neutron-tagged SK...
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Gloria Piemonti (Universita & INFN, Milano-Bicocca (IT))
The Deep Underground Neutrino Experiment (DUNE) is a next-generation neutrino oscillation experiment based on Liquid Argon Time Projection Chamber (LArTPC) technology. The DUNE Far Detectors will be equipped with a Photon Detection System (PDS) consisting of X-ARAPUCA modules to improve neutrino event reconstruction and enable astroparticle studies through triggering of non-beam...
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