20–26 Aug 2023
Natural Science Lecture Center (building-28), Seoul National University, Korea
Asia/Seoul timezone

Contribution List

243 out of 243 displayed
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  1. Tamer Tolba
    20/08/2023, 14:00
  2. Dr Marcos Dracos (Centre National de la Recherche Scientifique (FR))
    20/08/2023, 14:05
  3. Natalie Yvonne Jachowicz (Ghent University (BE))
    20/08/2023, 14:35
  4. Tamer Tolba
    20/08/2023, 15:05
  5. Natalia Milas (European Spallation Source)
    20/08/2023, 15:40
  6. Andrea Longhin (CEA Saclay), Andrea Longhin (Universita e INFN, Padova (IT)), andrea longhin (INFN)
    20/08/2023, 16:00
  7. Georgios Fanourakis (Nat. Cent. for Sci. Res. Demokritos (GR)), Kaare Endrup Iversen (Lund University (SE))
    20/08/2023, 16:20
  8. Jaejun Yu
    21/08/2023, 09:00
  9. Kyung Kwang Joo (Department of Physics-Chonnam National University-Unknown)
    21/08/2023, 09:05
  10. Chang Kee Jung (Stony Brook University (US))
    21/08/2023, 09:10
  11. Eung Jin Chun
    21/08/2023, 09:40
  12. Prof. Jian Tang (Sun Yat-Sen University(CN))
    21/08/2023, 10:40
  13. Dr Elena Gramellini (University of Manchester)
    21/08/2023, 10:50
  14. Megan Friend (High Energy Accelerator Research Organization (JP)), Megan Friend (KEK)
    21/08/2023, 11:00
  15. Yuki Fujii, Yuki Fujii (Monash University (AU))
    21/08/2023, 11:10
  16. Julia Harz
    21/08/2023, 11:20
  17. Yasuhiro NISHIMURA (Keio University)
    21/08/2023, 11:30
  18. Nagisa Hiroshima (University of Toyama)
    21/08/2023, 11:40
  19. Un Ki Yang (Seoul National University (KR))
    21/08/2023, 11:50
  20. Dr Rebekah PESTES (APC/IPGP)
    21/08/2023, 13:30
    Oral
  21. Laura Munteanu (CERN)
    21/08/2023, 13:55
    Oral
  22. Juan Pedro Ochoa Ricoux
    21/08/2023, 14:20
    Oral
  23. Natalie Yvonne Jachowicz (Ghent University (BE))
    21/08/2023, 15:10
    Oral
  24. Anthony Onillon (Technical University of Munich, 85747 Garching, Germany)
    21/08/2023, 16:00
    Oral
  25. Michael Schmidt (UNSW Sydney)
    21/08/2023, 16:25
    Oral
  26. Tomoko Ariga (Kyushu University (JP))
    21/08/2023, 16:50
    Oral
  27. John Leslie Almond (Seoul National University (KR))
    21/08/2023, 17:15
    Oral
  28. Prof. Yeongduk Kim (Institute for Basic Science (IBS), South Korea)
    21/08/2023, 17:40
    Oral
  29. Matteo Agostini
    22/08/2023, 08:30
    Oral
  30. Juraj Klaric (Universite Catholique de Louvain (UCLouvain))
    22/08/2023, 08:55
    Oral
  31. Sophie Berkman (University of British Columbia), Sophie Berkman
    22/08/2023, 09:20
    Oral
  32. Raquel Castillo Fernandez (University of Texas at Arlington)
    22/08/2023, 09:45
    Oral
  33. Prof. Omar Benhar (INFN and Sapienza University)
    22/08/2023, 10:10
    WG2: Neutrino Scattering Physics
    Oral

    I will outline the conceptual framework supporting the interpretation of the 40Ar(e,e'p) cross sections--recently measured at Jefferson Lab by the E12-14-012 Collaboration---in terms of the spectral functions describing the energy and momentum distribution of protons in the target nucleus. The key underlying assumptions and their validity in the kinematical setup of the Jefferson Lab...

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  34. Takeshi Nakadaira (High Energy Accelerator Research Organization (JP))
    22/08/2023, 11:00
    Oral
  35. Dr Jeffrey Eldred (Fermilab)
    22/08/2023, 11:25
    Oral
  36. Andreas Jansson (Unknown)
    22/08/2023, 11:50
    Oral
  37. Nikolaos Vassilopoulos
    22/08/2023, 12:15
    Oral
  38. Yukine Sato (Tokyo University of Science)
    22/08/2023, 14:00
    WG3: Accelerator Physics
    Oral

    The J-PARC accelerator, serving the long-baseline neutrino oscillation program in Japan, is engaged in a long-term effort to increase the proton beam power from 500kW to 750kW during T2K data-taking, and ultimately more than 1.3 MW for Hyper-Kamiokande.

    The T2K beamline underwent major upgrades in view of the increased beam power, and a successful first run was performed in April...

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  39. Dr Minoo Kabirnezhad (Imperial College London)
    22/08/2023, 14:00
    WG2: Neutrino Scattering Physics
    Oral

    I would like to present my recent work at the NuFact workshop in Seoul. https://journals.aps.org/prc/abstract/10.1103/PhysRevC.107.025502

    I have developed a single pion production model in neutrino-nucleon interaction:
    https://inspirehep.net/literature/1634864 .
    Then I used electron scattering data to extract the nucleon form factors:
    https://inspirehep.net/literature/1802724 ,
    In the...

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  40. MARIA PRADO RODRIGUEZ (University of Wisconsin-Madison)
    22/08/2023, 14:00
    WG1: Neutrino Oscillation Physics
    Oral

    Neutrino Mass Ordering (NMO) studies explore the unresolved fundamental question of whether the neutrino masses follow a normal ordering (m3>m2>m1) or an inverted ordering (m2>m1>m3). IceCube is an ice-Cherenkov neutrino detector deployed about 1.5 kilometers below the surface of the South Pole. Using DeepCore, a more densely instrumented volume of ice near the bottom of the detector, we study...

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  41. Alessandro Massimo Baldini (Universita & INFN Pisa (IT))
    22/08/2023, 14:00
    WG4: Muon Physics
    Oral

    The MEG experiment at Paul Scherrer Institut (Zurich – Switzerland) established in 2016 the best current upper limit of $4.2 \times 10^{-13}$ on the branching ratio of the $\mu->e \gamma$ decay. The search for this decay represents an extremely powerful tool to look for possible extensions of the Standard Model since its existence would unambiguously represent a sign of new physics.

    To...

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  42. Diana Patricia Mendez Mendez (Brookhaven National Laboratory)
    22/08/2023, 14:00
    WG5: Neutrinos Beyond PMNS
    Oral

    The Short-Baseline Near Detector (SBND) will be one of three Liquid Argon Time Projection Chamber (LArTPC) neutrino detectors positioned along the axis of the Booster Neutrino Beam (BNB) at Fermilab, as part of the Short-Baseline Neutrino (SBN) Program. The detector is anticipated to begin operation later this year. SBND is characterized by superb imaging capabilities and will record over a...

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  43. Andrew Furmanski (University of Minnesota (US))
    22/08/2023, 14:00
    WG1: Neutrino Oscillation Physics
    Oral

    DUNE will be a next-generation experiment aiming to provide precision measurements of the neutrino oscillation parameters. It will detect neutrinos generated in the LBNF beamline at Fermilab, using a Near Detector (ND) situated near the beam target where the neutrinos originate and a Far Detector (FD) located 1300 km away in South Dakota. A comparison of the spectra of neutrinos measured at...

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  44. Kajetan Niewczas
    22/08/2023, 14:15
    WG2: Neutrino Scattering Physics
    Oral

    The precise measurement of neutrino properties is among the highest priorities in fundamental particle physics. Accelerator-based neutrino experiments provide a unique framework for such studies, providing oscillation measurements and hints of the CP violation in the leptonic sector. However, since these experiments rely on the interaction of neutrinos with bound nucleons inside atomic nuclei,...

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  45. Hongyue Duyang (Shandong University)
    22/08/2023, 14:20
    WG1: Neutrino Oscillation Physics
    Oral

    The Jiangmen Underground Neutrino Observatory (JUNO) is a multi-purpose experiment currently under construction in southern China. It consists of a 20 kton liquid scintillator detector, whose main physics goal is to determine the neutrino mass ordering (NMO). While its main sensitivity is from reactor neutrino oscillations in vacuum, atmospheric neutrino oscillations in JUNO, via matter...

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  46. Sungbin Oh (Fermilab (US))
    22/08/2023, 14:20
    WG6: Detector Physics
    Oral

    The ProtoDUNE-SP detector is a single-phase liquid argon time projection chamber measuring 7.2 × 6.1 × 7.0 $m^3$ in active volume. It is designed as a test bed and full-scale prototype for the elements of the first far detector module of the Deep Underground Neutrino Experiment (DUNE). Located at the CERN Neutrino Platform, the detector was exposed to a tagged and momentum-analyzed particle...

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  47. Charlie Naseby
    22/08/2023, 14:20
    WG3: Accelerator Physics
    Oral

    For fixed-target experiments, final proton beam monitoring is key to controlling the properties of the particle flux exiting the target. The T2K experiment makes use of an Optical Transition Radiation (OTR) monitor for this purpose. In support of the J-PARC 750kW beam power upgrade, this monitor has undergone a series of changes targeted at increasing its tolerance to the higher beam intensity...

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  48. Meghna Bhattacharya (Fermilab)
    22/08/2023, 14:24
    WG5: Neutrinos Beyond PMNS
    Oral

    The MicroBooNE experiment employs an 85-ton active volume liquid argon time projection chamber to detect neutrinos from both the on-axis Booster Neutrino Beam (BNB) and off-axis Neutrinos at the Main Injector (NuMI) beam. This work investigates short baseline neutrino oscillations in a 3+1 sterile neutrino model and compares our results to previous anomalies found in experiments such as LSND,...

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  49. Dr Raul Gonzalez Jimenez (Complutense University of Madrid)
    22/08/2023, 14:30

    I will discuss some nuclear effects affecting neutrino-nucleus cross sections at energies of interest for neutrino-oscillation experiments. Pauli blocking, binding energies, effects beyond the impulse approximation, and final state interactions are investigated, with focus on the differences between a quantum mechanical approach and the models and methodology found within Monte Carlo neutrino...

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  50. Martin Müller (JGU Mainz)
    22/08/2023, 14:30
    WG4: Muon Physics
    Oral

    The Mu3e experiment will search for the charged lepton flavour violating decay $\mu \rightarrow e^+ e^- e^+$ and is based at the Paul Scherrer Institute (PSI). It aims to achieve a sensitivity of one in $\mathcal{O}(10^{15})$ moun decays in phase 1 and one in $10^{16}$ muon decays in phase 2, which is four orders of magnitude more sensitive than the previous measurement conducted by the...

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  51. Laura Amelie Zambelli (Centre National de la Recherche Scientifique (FR))
    22/08/2023, 14:40
    WG6: Detector Physics
    Oral

    The Deep Underground Neutrino Experiment (DUNE) is a long-baseline neutrino-oscillation experiment aiming at measuring CP-violating phase and neutrino mass ordering. The far detector consists of four 17-kt modules based on Liquid Argon Time Projection Chamber (LArTPC) technology.

    The recently proposed Vertical Drift (VD) concept has been selected as the design of the second module. This...

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  52. Johannes Schumann
    22/08/2023, 14:40
    WG1: Neutrino Oscillation Physics
    Oral

    The KM3NeT collaboration is building two neutrino detectors in the Mediterranean Sea. The KM3NeT/ORCA detector has been optimized for the detection of atmospheric neutrinos with energies between few GeV and 100 GeV. Among the primary goals are the measurement of the neutrino oscillation parameters and the determination of the neturno mass ordering. A correct interpretation of the measurements...

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  53. Katsuya Yonehara
    22/08/2023, 14:40
    WG3: Accelerator Physics
    Oral

    Fermilab's neutrino facilities, including NuMI and the upcoming LBNF, use proton beams to produce positively and negatively charged pions and kaons. Detailed simulations are necessary to study particle interactions and beam propagation. To efficiently analyze beam scan effects, we propose a method for generating multiple simulation samples with high statistics. By simulating a single sample...

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  54. Paloma Rodríguez Casalé
    22/08/2023, 14:45

    Mirar en ficheros adjuntos.

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  55. Lee Hagaman (University of Chicago)
    22/08/2023, 14:48
    WG5: Neutrinos Beyond PMNS
    Oral

    The MicroBooNE experiment is an 85-ton active volume liquid argon time projection chamber (LArTPC) neutrino detector situated in the Fermilab Booster Neutrino Beam (BNB). Leveraging the unique capabilities of the LArTPC technology to distinguish photons from electron electromagnetic showers, MicroBooNE has achieved the world's most sensitive search for neutrino-induced single-photon...

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  56. Gaurav Arora (Postdoc Research Associate)
    22/08/2023, 15:00
    WG3: Accelerator Physics
    Oral

    Beam-intercepting devices face challenges of beam-induced thermal shock and radiation damage effects. Efficient cooling systems are needed to remove heat as beam power increases. Development of novel materials capable of sustaining increased beam power and intensity is crucial for future multi-MW target facilities. In this talk, several promising novel materials will be discussed, including...

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  57. Dr Stephen Dolan (CERN)
    22/08/2023, 15:00
    WG2: Neutrino Scattering Physics
    Oral

    Building on Phys. Rev. D 106, 073001 (2022), we present the implementation and validation of the Hartree-Fock continuum random phase approximation (HF-CRPA) model in the GENIE neutrino-nucleus interaction event generator and a comparison of the subsequent predictions to experimental measurements of lepton kinematics from interactions with no mesons in the final state. These predictions are...

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  58. Dr Sanghoon Jeon (Seoul National University)
    22/08/2023, 15:00
    WG1: Neutrino Oscillation Physics
    Oral

    The RENO experiment has precisely measured the amplitude and frequency of reactor antineutrino oscillation at Hanbit Nuclear Power Plant since Aug. 2011. The 2018 publication reported the measured oscillation parameters based on 2200 days of data. After that, additional 1600 days of data has been acquired with one or two operating reactors, which yields relatively lower antineutrino flux. This...

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  59. Steven Boi
    22/08/2023, 15:00
    WG4: Muon Physics
    Oral

    The Muon-to-Electron-Conversion (Mu2e) Experiment is a high-precision, intensity-frontier experiment being developed at Fermilab which will search for coherent, neutrino-less muon to electron conversion in the presence of an atomic nucleus. Such a process would exhibit charged lepton flavor violation (CLFV), which has not yet been observed. Continuing the search for CLFV, Mu2e will improve the...

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  60. Nicholas Kamp
    22/08/2023, 15:12
    WG5: Neutrinos Beyond PMNS
    Oral

    The 4.8$\sigma$ low-energy excess (LEE) of electron-like events observed by MiniBooNE is one of the longest-standing anomalies in particle physics. As the MiniBooNE reconstruction relied on the identification of Cherenkov rings, the excess could come from extra electrons or photons in the detector. This talk covers new developments regarding each hypothesis. The MicroBooNE experiment has...

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  61. Richard Ruiz (Institute of Nuclear Physics (IFJ) PAN)
    22/08/2023, 15:15
    WG2: Neutrino Scattering Physics
    Oral

    In this talk we revisit so-called target mass corrections (TMCs) to nuclear structure functions in lepton-nucleus deeply inelastic scattering (DIS), which account for the fact that the masses of nuclei are not guaranteed to be small compared to momentum transfers in DIS. We present several findings, including: (i) that nuclear parton distribution functions can be expressed directly in terms of...

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  62. Gaurav Arora (Postdoc Research Associate)
    22/08/2023, 15:20
    WG3: Accelerator Physics
    Oral

    As next-generation accelerator target facilities, for Neutrino Program such as the Long-Baseline Neutrino Facility (LBNF) or Muon Program such as Mu2e-II at Fermilab, become increasingly more powerful and intense, high power target systems face key technical challenges. Beam-intercepting devices such as beam windows and secondary particle-production targets are continuously bombarded by...

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  63. MyeongJae Lee
    22/08/2023, 15:30
    WG4: Muon Physics
    Oral

    COMET is an experiment at J-PARC, Japan, which will search for neutrinoless conversion of muons into electrons in the field of a nucleus ($μ^− + N \to e^− + N$); a lepton flavor violating process. Recent progresses in facility and detector development are presented, aiming for the experimental sensitivity of the order of $10^{−15}$ for Phase-I and $10^{−17}$ or beyond for Phase-II experiment....

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  64. Gray Putnam
    22/08/2023, 15:36
    WG5: Neutrinos Beyond PMNS
    Oral

    ICARUS is a liquid argon time projection chamber (LArTPC) neutrino detector situated at the intersection of two neutrino beams at Fermilab. As part of the Short-Baseline Neutrino (SBN) program, it will search for neutrino oscillations in the Booster Neutrino Beam (BNB). The search will test past anomalous results in neutrino physics such as the LSND, MiniBooNE, and reactor anomalies which...

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  65. Dr Vishvas Pandey (Fermi National Accelerator Laboratory)
    22/08/2023, 16:30

    Current and future accelerator-based neutrino facilities utilizing intense neutrino beams and advanced neutrino detectors are focused on precisely determining neutrino oscillation properties and signals of weakly interacting Beyond the Standard Model (BSM) physics. These are subtle effects, such as extracting the CP violation phase and disentangling parameter degeneracies between oscillation...

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  66. Dr Akira Sato (Osaka University)
    22/08/2023, 16:30
    WG3: Accelerator Physics
    Oral

    The search for muon-electron conversion processes that violate the conservation of charged lepton flavors has attracted much attention for its superior sensitivity to the discovery and verification of new physical phenomena beyond the Standard Model. Two experiments, COMET and Mu2e, are currently underway in Japan and the United States to search for muon electron conversion processes with...

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  67. 22/08/2023, 16:30
  68. 22/08/2023, 16:30
  69. Dung Thi Nguyen (Hanoi University of Science)
    22/08/2023, 16:30
    WG6: Detector Physics
    Oral

    The near detector of T2K (ND280) is undergoing a major upgrade. A new scintillator tracker, named superFGD, with fine granularity and 3D-reconstruction capabilities has been assembled at JPARC. The new Time Projection Chambers are under development, based on the innovative resistive Micromegas technology and a field cage made of extremely thin composite walls. New scintillator panels with...

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  70. Beatriz Oregui
    22/08/2023, 16:30
    WG5: Neutrinos Beyond PMNS
    Oral

    Neutrinoless double-beta decay (0νββ) is a key process to address some of the major outstanding issues in particle physics, such as the lepton number conservation and the Majorana nature of the neutrino. Several efforts have taken place in the last decades in order to reach higher and higher sensitivity on its half-life. The next-generation of experiments aims at covering the Inverted-Ordering...

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  71. SunWoo Gwon
    22/08/2023, 16:50
    WG6: Detector Physics
    Oral

    Neutrino oscillation experiments require accurate measurements of the neutrino energy. However, the kinematic detection of final-state neutrons in neutrino interactions is currently absent in these experiments. A revolutionary 3-Diensional projection scintillator tracker (3DST) is capable of detecting both the kinetic energy and direction of neutrons on an event-by-event basis with precision...

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  72. Nikolaos Vassilopoulos
    22/08/2023, 16:50
    WG3: Accelerator Physics
    Oral

    Since the approval of MELODY in early 2023, the collection of surface muons and pions and the relevant beamlines have been revised.
    In this report, we would like to present our latest studies at MELODY: i) For the target station, a) the optimization in terms of yields and material of the rotated target that is currently preferred and combined with the new sideways collection of both muons and...

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  73. Tristan Doyle
    22/08/2023, 16:54
    WG1: Neutrino Oscillation Physics
    Oral

    T2K is a long baseline neutrino experiment which exploits a neutrino and antineutrino beam at J-PARC to perform precision measurements of atmospheric parameters $\Delta m^{2}_{32}$, $\sin^2(\theta_{23})$ and to search for CP-violation. The main systematic uncertainties limiting the precision will be described, as well as, the role of the near detector to constrain such systematic...

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  74. Matteo Cadeddu
    22/08/2023, 16:54
    WG5: Neutrinos Beyond PMNS
    Oral

    Co-authors: M. Atzori Corona, N.Cargioli, F. Dordei, C. Giunti, Y.F. Li, C.A. Ternes, Y.Y. Zhang

    The detection of Coherent Elastic Neutrino-Nucleus Scattering (CEvNS) performed in 2017 and 2021 with cesium iodide and in 2020 with liquid argon by the COHERENT collaboration has paved the way for precision phenomenological measurements of many diverse physical phenomena.
    CEνNS is a neutral...

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  75. Ziliang Chu (The Institute of High Energy Physics of the Chinese Academy of Sciences)
    22/08/2023, 17:10
    WG6: Detector Physics
    Oral

    25600 3-inch PMTs (SPMTs) were designed in the JUNO detector together with 20012 20-inch PMTs (LPMTs). The SPMT system can enhance the detector’s performances such as calibrating charge nonlinearity of LPMTs and thus improving the energy resolution. Signals of SPMTs are read out by the frontend electronics contained in 200 underwater boxes through 1600 customized multichannel connectors. All...

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  76. Giovanni Dal Maso
    22/08/2023, 17:10
    WG4: Muon Physics
    Oral

    Currently PSI delivers the most intense continuous muon beam in the world with up to a few 10^8 μ+/s. The High Intensity Muon Beam (HiMB) project aims at developing a new target station and muon beam lines able to deliver 10^10 μ+/s, with a huge impact for low-energy, high-precision muon experiments.

    While the next generation of proton drivers with beam powers in excess of the current limit...

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  77. Bryan Ramson (Fermilab)
    22/08/2023, 17:18

    Neutrino interaction cross sections are a significant source of uncertainty for many experiments dependent on the determination of neutrino properties from the inference of neutrino flavor or energy. To mitigate the effect of these large uncertainties on results from NOvA Experiment, a long-baseline experiment currently operating at Fermilab, the...

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  78. Richard Ruiz (Institute of Nuclear Physics (IFJ) PAN)
    22/08/2023, 17:18
    WG5: Neutrinos Beyond PMNS
    Oral

    In the context of the Phenomenological Type I Seesaw, we investigate the LHC's sensitivity to exclusive, mesonic decay modes of long-lived, light (Dirac and Majorana) heavy neutrinos $N$ when they are produced in the decays of $W^\pm$ bosons. We present a new framework that combines massless QCD to describe $N$'s production up to NLO in QCD via weak bosons with a low-energy effective field...

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  79. Yang HAN
    22/08/2023, 17:30
    WG6: Detector Physics
    Oral

    Neutrino detectors are amongst the largest ever built photonics systems, where the neutrino detection is inexorably linked to the challenging detection of scarce photons. The tremendous progresses in neutrino physics over past several decades are inseparable from the evolution of the detector photonics interfaces to yield ever higher precision and richer detection information. The measurement...

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  80. Dr Sohtaro Kanda
    22/08/2023, 17:30
    WG4: Muon Physics
    Oral

    The ultra-slow muon (USM) beamline at J-PARC MLF MUSE provides a low-energy muon beam through laser ionization of thermal muonium in a vacuum. When a muon beam irradiates a hot tungsten foil at 2000 K, muonium atoms are emitted with an energy of 0.2 eV. The atoms can be ionized by two synchronized laser beams with wavelengths of 122 nm and 355 nm [1]. Low-energy muons with adjustable energies...

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  81. Kevin McFarland (University of Rochester), Kevin McFarland
    22/08/2023, 17:42

    The transition axial form factor of the nucleon is a probe of nucleon structure and important for accurate prediction of charged current elastic and quasielastic scattering. Using the hydrogen in its hydrocarbon target, the MINERvA experiment has extracted a sample of antineutrino proton elastic scattering events, and directly extracted the form factor in a technique analogous to that used...

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  82. Yu Seon Jeong (Chung-Ang University (KOR))
    22/08/2023, 17:42
    WG5: Neutrinos Beyond PMNS
    Oral

    The Large Hadron Collider (LHC) can produce huge numbers of neutrinos into the large rapidity region. New experiments at the LHC, the ongoing FASER\nu and SND@LHC and the proposed Forward Physics Facility (FPF) experiments aim to detect such neutrinos, in particular prompt neutrinos which mainly come from charm hadron decays. Prompt neutrinos can be also produced by cosmic ray interactions in...

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  83. Achim Stahl (Rheinisch Westfaelische Tech. Hoch. (DE))
    22/08/2023, 17:50
    WG6: Detector Physics
    Oral

    The Jiangmen Underground Neutrino Observatory (JUNO) is a 20 kton liquid scintillator detector scheduled to come online in 2024. The scintillator volume is observed by approximately 17 000 large 20” PMTs and 25 000 small 3” PMTs. The performance of the PMTs is essential to reach the scientific goals, especially for oscillation physics. I will review the system of the large PMTs. Prior to...

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  84. Jaroslaw Pasternak
    22/08/2023, 17:50
    WG4: Muon Physics
    Oral

    Future muon to electron conversion experiments require an improvement in sensitivity by a factor of 100 and novel accelerator concepts are necessary to achieve this goal.
    A Fixed-Field Alternating gradient (FFA) ring has been proposed to create a Phase Rotated Intense Source of Muons (PRISM), which will allow for a significant purification of the muon beam and suppression of a typically large...

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  85. Dr Luke Pickering (Royal Holloway, University of London), Dr Stephen Dolan (CERN)
    22/08/2023, 18:06
    WG2: Neutrino Scattering Physics
    Oral

    A precise modelling of neutrino-nucleus interactions is of fundamental importance to allow current and future accelerator-based neutrino oscillation experiments to achieve their ambitious goals. However, as it stands, no neutrino interaction model currently implemented in event generators has been shown to offer a quantitatively satisfactory agreement with many (and in some cases, any) modern...

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  86. Jiajun Liao
    22/08/2023, 18:06
    WG5: Neutrinos Beyond PMNS
    Oral

    Most antineutrinos produced in a nuclear reactor have energies below the inverse beta decay (IBD) threshold, and have not yet been detected. We show that a coherent elastic neutrino-nucleus scattering (CEvNS) experiment with an ultra-low energy threshold like NUCLEUS can measure the flux of reactor neutrinos below the IBD threshold. Using a regularized unfolding procedure, we find that a...

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  87. Matteo Sorbara (Istituto Nazionale di Fisica Nucleare - Sezione Roma Tor Vergata)
    23/08/2023, 08:30
    Oral
  88. Dr Innes Bigaran (Fermilab and Northwestern University)
    23/08/2023, 08:55
    Oral
  89. Satoshi Mihara
    23/08/2023, 09:20
    Oral
  90. Tristan Doyle
    23/08/2023, 09:45
    Oral
  91. Michael Joseph Wilking, Michael Wilking (TRIUMF), Prof. Michael Wilking (Stony Brook University)
    23/08/2023, 10:10
    Oral
  92. Haein YIM
    23/08/2023, 11:00
    Oral

    The Women Committee (WCiKPS) in Korean Physical Society has been established in April 2002, just after the 1st IUPAP international conference on Women in Physics held in Paris, in March 2002 aiming for spreading women’s science culture to increase employment and promotion of women physicists and to improve research and work environments women friendly. The number of female physicists in KPS...

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  93. Shota Takahashi (KEK), Shota Takahashi (Conseil Europeen Recherche Nucl. (CERN)-Unknown-Unknown)
    23/08/2023, 11:20
    Oral
  94. Eun-Joo Ahn (University of California Santa Barbara)
    23/08/2023, 11:40
    WG7: Inclusion, Diversity, Equity, Education, and Outreach
    Oral

    Why do we remember some scientists while forgetting others who participated in the same scientific work? Moving away from prominent scientists and focusing on the invisible workers can highlight the role of gender, race, and class in scientific knowledge-making. Using Mount Wilson Observatory at the turn of the twentieth century as an example, I point out how scientists in positions of power,...

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  95. MIA,ROBIN,BYRON WEST
    23/08/2023, 12:00
    Oral
  96. Francesca Dordei (INFN, Cagliari (IT))
    23/08/2023, 12:20
  97. Sayeed Akhter (Aligarh Muslim University)
    23/08/2023, 12:30
    WG2: Neutrino Scattering Physics
    Poster

    MINERvA (Main Injector Neutrino ExpeRiment to study $\nu$-A interactions) is a dedicated (anti)neutrino-nucleus experiment in the few GeV energy region which has used the high-intensity NuMI beamline facility at the Fermi National Accelerator Laboratory.
    The experiment was performed using several nuclear targets, Iron, Carbon, Lead, Water and Hydrocarbon to study the nuclear medium effects in...

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  98. Pragyanprasu Swain (Institute of Physics, Bhubaneswar, India), Mr Sudipta Das (Institute of Physics, Bhubaneswar, India & HBNI, Mumbai, India)
    23/08/2023, 12:32
    WG5: Neutrinos Beyond PMNS
    Poster

    Unified theories such as string theory and loop quantum gravity allow the Lorentz Invariance Violation (LIV) at the Planck Scale ($M_P \sim 10^{19}$ GeV). Using an effective field theory, this effect can be observed at low energies in terms of new interactions with a strength of $\sim 1/M_P$. These new interactions contain operators with LIV coefficients which can be CPT-violating or...

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  99. Daniel Cherdack
    23/08/2023, 16:00
    Oral
  100. Andrew Sutton
    23/08/2023, 16:20
    Oral
  101. Avinay Bhat (University of Chicago)
    23/08/2023, 16:40
    Oral
  102. Dr Alfonso Andres Garcia Soto (IFIC)
    23/08/2023, 17:00
    Oral
  103. Rex Tayloe
    23/08/2023, 17:20
    Oral
  104. Dr Marcos Dracos (Centre National de la Recherche Scientifique (FR))
    23/08/2023, 17:45
    Oral
  105. Seongchul Yoon
    23/08/2023, 18:30
  106. Intae Yu (Sungkyunkwan University (KR))
    24/08/2023, 08:30
    Oral
  107. Dr Mark Patrick Hartz (TRIUMF & Kavli IPMU, University of Tokyo)
    24/08/2023, 08:50
    Oral
  108. Yang HAN
    24/08/2023, 09:10
    Oral
  109. Chris Marshall (University of Rochester), Christopher Marshall (University of Rochester (US))
    24/08/2023, 09:35
    Oral
  110. Neil Kevin Mccauley (University of Liverpool (GB)), Neil McCauley, Neil McCauley (The University of Liverpool)
    24/08/2023, 10:00
    Oral
  111. Alain Blondel (Universite de Geneve (CH)), Mary Bishai (Brookhaven National Laboratory (US))
    24/08/2023, 10:50

    Moderator: Alain Blondel
    Panel:
    Mary Bishai (DUNE Spokesperson)
    Masato Shiozawa (Hyper-K Spokesperson)

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  112. 24/08/2023, 11:50
  113. 24/08/2023, 12:00
  114. Bianca De Martino (Centre National de la Recherche Scientifique (FR))
    25/08/2023, 08:30
    WG3: Accelerator Physics
    Oral

    The neutrino tagging technique proposes to instrument a neutrino beam line with silicon trackers to kinematically reconstruct properties of individual beam neutrinos produced in $\pi\to\mu\nu_\mu$, K$\to\mu\nu_\mu$ decays. As a result, the initial neutrino flux is precisely determined and the individual neutrino energy can be reconstructed with a resolution better than 1%. Moreover, based on...

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  115. Mehedi Masud (Instituto de Física Corpuscular (CSIC-Universitat de València))
    25/08/2023, 08:30
    WG5: Neutrinos Beyond PMNS
    Oral

    One of the basic foundations of quantum field theory is Lorentz invariance. The spontaneous breaking of Lorentz symmetry at a high energy scale can be studied at low energy extensions like the Standard model in a model-independent way through effective field theory (EFT). The present and future Long-baseline neutrino experiments can give a scope to observe such a Planck-suppressed physics of...

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  116. 25/08/2023, 08:30
  117. 25/08/2023, 08:30
  118. Prof. Costas Andreopoulos (University of Liverpool)
    25/08/2023, 08:30

    The international GENIE Collaboration maintains and develops an extensive software suite to meet the simulation needs of the broad neutrino community. GENIE develops a universal event generator simulating neutrino interactions from MeV to PeV energy scales, and a global analysis of neutrino scattering data used for model characterization, tuning and uncertainty evaluations. In recent years,...

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  119. Dr Luke Pickering (Royal Holloway, University of London)
    25/08/2023, 08:50
    WG2: Neutrino Scattering Physics
    Oral

    The NEUT generator has a long, storied history. Originally written to predict neutrino induced backgrounds for the Kamioka Nucleon Decay Experiment (Kamiokande), it is now relied upon by T2K to simulate signal and background interactions for their oscillation and neutrino scattering cross section measurements. Looking to the future, the next-generation Hyper-Kamiokande experiment expects to...

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  120. Sumit Ghosh (KIAS)
    25/08/2023, 08:54
    WG5: Neutrinos Beyond PMNS
    Oral

    Neutrino oscillation experiments have provided crucial insights into the nature of neutrinos, including the discovery of neutrino oscillations and the observation of CP violation. Non-Standard Neutrino Interactions (NSIs) have emerged as an important topic of study, as they can potentially modify the neutrino oscillation probabilities and affect the measurement of CP violation parameters. In...

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  121. Megan Friend (High Energy Accelerator Research Organization (JP)), Megan Friend (KEK)
    25/08/2023, 08:54
    WG1: Neutrino Oscillation Physics
    Oral

    T2K is a long baseline neutrino experiment which exploits a neutrino and antineutrino beam at J-PARC, which is produced by a proton beam impinging on a graphite target, a flux of pions and kaons are produced and neutrinos are produced by their disintegration.

    A very detailed simulation of the beamline allows to predict the rate and energy of produced neutrinos, but still large uncertainties...

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  122. Yuta Higashino (Osaka Univ.)
    25/08/2023, 09:00
    WG4: Muon Physics
    Oral

    The DeeMe experiment is planned at J-PARC MLF H-Line.The experiment aims to search for the muon to electron conversion in the nuclear field, which is one of the charged lepton flavor violating processes that are forbidden in the Standard Model and expected to be highly sensitive to search for new physics.The DeeMe experiment will be the first search with using muonic carbon atoms.We aim to...

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  123. Mr Jake McKean (Imperial College (GB))
    25/08/2023, 09:10
    WG2: Neutrino Scattering Physics
    Oral

    Neutrino oscillation experiments, such as the Tokai to Kamioka (T2K) experiment, are limited by their simulation of accurate neutrino-nucleus interactions. More in-depth theoretical knowledge of neutrino-nucleus interactions are paramount; however, implementing such knowledge in existing event generator frameworks is just as imperative. To evaluate neutrino-nucleus interactions a general...

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  124. Priya Mishra
    25/08/2023, 09:18
    WG5: Neutrinos Beyond PMNS
    Oral

    The focus of our study is to investigate neutrino mass models that arise from discrete non-abelian modular symmetry groups. These symmetries offer a promising theoretical approach to understanding neutrino phenomenology and involve multiple free parameters. Specifically, we examine models based on the $A_4$ modular symmetry and explore how the non-trivial transformation of Yukawa couplings...

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  125. Prof. Jianming Bian (University of California Irvine (US))
    25/08/2023, 09:18
    WG1: Neutrino Oscillation Physics
    Oral

    Neutrinos elastically scattering off atomic electrons is a purely leptonic
    process whose cross section can be precisely calculated in the standard
    model. A measurement of this process can provide an in-situ constraint
    to the absolute neutrino flux in an accelerator-based $\nu_\mu$ beam. NOvA is
    a long-baseline neutrino experiment optimized to observe the oscillation
    of $\nu_\mu$ to...

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  126. Chen Wu (RCNP, Osaka University)
    25/08/2023, 09:25
    WG4: Muon Physics
    Oral

    The COMET experiment aims to search for the muon-to-electron conversion process with a sensitivity 10,000 times better than the current best result. The muon-to-electron conversion process violates charged lepton flavor conservation, which is strictly forbidden in the Standard Model. Once discovered, the muon-to-electron conversion process will provide definitive evidence of the existence of...

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  127. Afroditi Papadopoulou
    25/08/2023, 09:30
    WG2: Neutrino Scattering Physics
    Oral

    Simulations of neutrino-nucleus scattering are a critical input to oscillation analyses and various other investigations in high-energy physics. Achieving the physics goals of future experiments will require substantial improvements to the precision of these simulations. In March of this year, a workshop was held at Fermilab that examined several major topics related to future development of...

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  128. Katsuya Yonehara
    25/08/2023, 09:42
    WG3: Accelerator Physics
    Oral

    Neutrinos at the Main Injector (NuMI) is a project at Fermilab that provides an intense beam of neutrinos used by a number of experiments. NuMI creates a beam of pions that decay into neutrinos, muons, and other particles. Muons are registered by the muon monitors. Magnetic horns are the key elements of the NuMI beam line. This work uses the muon beam profile observed at the muon monitors to...

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  129. Mr Sudipta Das (Institute of Physics, Bhubaneswar, India & HBNI, Mumbai, India)
    25/08/2023, 09:42
    WG5: Neutrinos Beyond PMNS
    Oral

    The discovery of new, flavor-dependent neutrino interactions would provide compelling evidence of physics beyond the Standard Model. We focus on interactions generated by the anomaly-free, gauged, abelian lepton-number symmetries, specifically $L_e-L_\mu$, $L_e-L_\tau$, and $L_\mu-L_\tau$, that introduce a new matter potential sourced by electrons and neutrons, potentially impacting neutrino...

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  130. Guan Ming Wong (TDLI (Shanghai Jiao Tong University))
    25/08/2023, 09:50
    WG4: Muon Physics
    Oral

    The muEDM experiment, currently under development at the Paul Scherrer Institute (PSI) in Switzerland, aims to probe the muon electric dipole moment (EDM) using the frozen-spin technique within a solenoidal storage ring. This experiment seeks to achieve a muon EDM sensitivity of 6×10-23 e⋅cm, which is three orders of magnitude more precise than the current limit set by the BNL Muon...

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  131. Anna Ershova (Université Paris-Saclay (FR))
    25/08/2023, 09:50
    WG2: Neutrino Scattering Physics
    Oral

    As neutrino oscillation physics enters the precision era, the modeling of neutrino-nucleus interactions constitutes an increasingly challenging source of systematic uncertainty for new measurements. To confront such uncertainties, a new generation of detectors is being developed to measure the exclusive final state of neutrino interaction. Precise simulations of the nuclear effects on the...

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  132. Daniel Cherdack
    25/08/2023, 10:06
    WG3: Accelerator Physics
    Oral

    ICARUS is a 430 t liquid argon time projection chamber, neutrino detector located at Fermi National Accelerator Laboratory and serves as the far detector for the Short Baseline Neutrino program. The ICARUS detector lies 795 m downstream and 5.7° above the Neutrinos at the Main Injector (NuMI) neutrino beam. At this large off-axis angle, ICARUS has a unique opportunity to measure a variety of...

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  133. Noah Steinberg (Fermi National Accelerator Laboratory)
    25/08/2023, 10:10
    WG2: Neutrino Scattering Physics
    Oral

    The neutrino community is at an exciting time where new data with higher precision than ever is challenging the empirically based models which have been developed over the last several decades. Understanding this new data requires state of the art theory, leveraging collaboration between the nuclear physics, electron scattering, and neutrino community. One such state of the art model, the...

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  134. Prof. Kim Siang Khaw (Tsung-Dao Lee Institute, Shanghai Jiao Tong University), Dr Kim Siang Khaw (Tsung-Dao Lee Institute (CN))
    25/08/2023, 11:00
    WG4: Muon Physics
    Oral

    The Muon g-2 experiment at Fermilab is making progress towards its physics goal of measuring the muon anomalous magnetic moment with the unprecedented precision of 140 parts per billion. In April 2021 the collaboration published the first measurement, based on the first year of data taking. The second result is based on the second and third years of data taking combined. In this talk, we...

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  135. Takaaki Yasui (High Energy Accelerator Research Organization (KEK))
    25/08/2023, 11:00
    WG3: Accelerator Physics
    Oral

    The main ring synchrotron (MR) of Japan Proton Accelerator Research Complex (J-PARC) provides high power and high intensity beams for the neutrino and hadron experiments. We have been upgrading hardware from the summer of 2021 to shorten the repetition period aiming at 1.3 MW user operation for the neutrino experiments by 2028. The upgrades are progressing smoothly, and 760 kW equivalent beams...

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  136. Eduard Samigullin
    25/08/2023, 11:00
    WG5: Neutrinos Beyond PMNS
    Oral

    The latest results of the DANSS experiment are presented. The plastic scintillator detector is located under 3.1 GW industrial reactor core of Kalinin Nuclear Power Plant, and its main purpose is the search for the short baseline neutrino oscillations. The inverse beta decay reaction is used for the antineutrino detection. The data are collected at three distances – 10.9, 11.9 and 12.9 meters...

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  137. 25/08/2023, 11:00
  138. Mr Seowon Choi (Sungkyunkwan Universitiy)
    25/08/2023, 11:00

    The IceCube Neutrino Observatory is the largest neutrino telescope located deep within the South Pole ice. Currently, an upgrade with denser spaced sensors is being built and one of the goals of the IceCube Upgrade is a precise characterization of the optical properties of the Antarctic ice, which is the source of the largest systematic uncertainty for most IceCube analysis. Calibration...

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  139. Prof. Un-ki Yang (Seoul National University)
    25/08/2023, 11:00
    WG2: Neutrino Scattering Physics
    Oral

    This talk will present the status of the Bodek-Yang model.

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  140. Jaroslaw Pasternak
    25/08/2023, 11:18
    WG3: Accelerator Physics
    Oral

    A rich cross-section and "beyond the Standard Model" (BSM) search programme will be served by the intense $\nu_e$ and $\nu_\mu$ beams that will be provided by the neutrinos from stored muons (nuSTORM) facility. Exceptional precision in cross section measurement and exquisite sensitivity in BSM searches are afforded at nuSTORM by the precise knowledge of the flavour composition and the energy...

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  141. Simon Corrodi
    25/08/2023, 11:20
    WG4: Muon Physics
    Oral

    The Muon g-2 experiment at Fermilab measures the muon magnetic-moment anomaly, $a_\mu=(g-2)/2$, with the ultimate goal of 140 parts per billion (ppb) precision. This requires determining the absolute magnetic field, averaged over space and time, experienced by the muons, expressed as the nuclear magnetic resonance frequency of protons in a spherical pure water sample at a specified reference...

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  142. Dr Alfonso Andres Garcia Soto (IFIC)
    25/08/2023, 11:20
    WG2: Neutrino Scattering Physics
    Oral

    Accurate theory calculations for neutrino-nucleus scattering rates are essential in the interpretation of neutrino experiments, from oscillation measurements to astroparticle physics at neutrino telescopes. In the deep-inelastic (DIS) regime, neutrino structure functions can be reliably evaluated in the framework of perturbative QCD. However, large uncertainties affect these structure...

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  143. Lluis Marti
    25/08/2023, 11:20
    WG6: Detector Physics
    Oral

    The Super-Kamiokande water Cherenkov underground neutrino observatory is located in Japan. Since 2020, it has undergone two loadings with gadolinium sulfate. In the first loading during summer 2020, 13 tons of gadolinium sulfate octahydrate were dissolved, corresponding to a mass concentration of 0.02% gadolinium sulfate. In the second loading, 26 tons were diluted, resulting in a mass...

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  144. Jonggeon Kim (SungKyunKwan university)
    25/08/2023, 11:25
    WG1: Neutrino Oscillation Physics
    Oral

    NEOS is an experiment to search for a sterile neutrino oscillation from a nuclear reactor core at a short baseline. The detector was deployed at a 24-m distance from a 2.8 gigawatt-thermal-power reactor core in the tendon gallery of the Hanbit-5 reactor. NEOS-II has recorded 388 (112) live-days of reactor-on (-off) data including a full reactor operation cycle and the reactor maintenance...

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  145. Prof. Jianming Bian (University of California Irvine (US))
    25/08/2023, 11:36
    WG3: Accelerator Physics
    Oral

    The Forward Physics Facility (FPF) is a proposed program to build an underground cavern with the space and infrastructure to support a suite of far-forward experiments at the Large Hadron Collider during the High Luminosity era (HL-LHC). The Forward Liquid Argon Experiment (FLArE) is a Liquid Argon Time Projection Chamber (LArTPC) based experiment designed to detect very high-energy neutrinos...

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  146. Haemin Jeong
    25/08/2023, 11:40
    WG6: Detector Physics
    Oral

    Coherent elastic neutrino-nucleus scattering (CEvNS) was predicted in 1974 as a consequence of the weak neutral current. 43 years later, the COHERENT collaboration first observed CEvNS using a 14.6-kg CsI detector. After 3 years, CEvNS on argon was measured using COH-Ar-10 (CENNS-10), 24-kg liquid argon detector. There are many physics opportunities related to CEvNS, but COH-Ar-10 has ~30%...

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  147. Dr Paolo Girotti (Istituto Nazionale di Fisica Nucleare Pisa)
    25/08/2023, 11:40
    WG4: Muon Physics
    Oral

    The Fermilab Muon g-2 experiment was designed to measure the muon's anomalous magnetic moment $a_\mu = (g-2)/2$ to 140 parts per billion. The value of $a_\mu$ is proportional to the difference frequency $\omega_a = \omega_s - \omega_c$ between the muon's cyclotron frequency and spin precession frequency in the uniform magnetic field of the g-2 storage ring. The frequency $\omega_a$ is...

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  148. Ji Young Yu (southern methodist university)
    25/08/2023, 11:40
    WG2: Neutrino Scattering Physics
    Oral

    Global analyses of nuclear Parton distribution functions (nPDFs) play a crucial role in making precise predictions for a wide range of processes in lepton-nucleus (lA), proton-nucleus (pA), and heavy ion collisions (AA). In this context, the inclusion of neutrino deep inelastic scattering (DIS) data is particularly important as it enables an improved flavour separation of the parton...

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  149. ChangDong Shin
    25/08/2023, 11:50
    WG1: Neutrino Oscillation Physics
    Oral

    The JSNS2 (J-PARC Sterile Neutrino Search at the J-PARC Spallation Neutron Source) is an experiment with a neutrino detector utilizing a 3GeV proton beam on a mercury target in the J-PARC Materials and Life Science Experimental Facility. The primary goal of the JSNS2 experiment is to search for the sterile neutrino with Δm2 ~ 1eV by measuring a neutrino...

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  150. Moses Chung
    25/08/2023, 11:54
    WG3: Accelerator Physics
    Oral

    Korea has several cutting-edge accelerator user facilities that are currently operational or in the commissioning phase. These include the 3rd Generation Synchrotron Light Source (PLS-II) and the X-ray Free Electron Laser (PAL-XFEL) situated in Pohang, the Korea Multi-purpose Accelerator Complex (KOMAC) located in Gyeongju, and the Rare Isotope Accelerator complex for ON-line experiments...

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  151. Prabhjot Singh
    25/08/2023, 12:00
    WG2: Neutrino Scattering Physics
    Oral

    NOvA is a long-baseline accelerator-based neutrino experiment based in the USA. NOvA uses an intense neutrino beam produced at Fermilab’s accelerator complex to make physics measurements of neutrino oscillations, neutrino cross sections, and much more. For its physics goals, NOvA uses two functionally-identical detectors. The Near Detector (ND) is situated at Fermilab, 1 km from the neutrino...

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  152. Avinay Bhat (University of Chicago)
    25/08/2023, 12:00
    WG6: Detector Physics
    Oral

    The Short Baseline Near Detector (SBND), a 112 ton liquid argon time projection chamber (LArTPC), is the near detector of the Short Baseline Neutrino Program at Fermilab. In a LArTPC, ionization electrons from a charged particle track drift along the electric field lines, inducing bipolar signals on the induction planes, and a unipolar signal collected on the collection plane. In this talk, I...

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  153. Yuta Okazaki (KEK)
    25/08/2023, 12:00
    WG4: Muon Physics
    Oral

    In 2021, the anomalous magnetic moment of the muon, a_µ = (g_µ-2)/2, was measured at the Fermilab National Accelerator Laboratory (FNAL) with a precision of 0.46 ppm. This measurement result is consistent with the previously value measured more than a decade ago at the Brookhaven National Laboratory (BNL), and the deviation from the Standard Model (SM) prediction has been reported with a...

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  154. Roberto Mandujano
    25/08/2023, 12:20
    WG6: Detector Physics
    Oral

    The Deep Underground Neutrino Experiment (DUNE) is a precision long-baseline neutrino oscillation experiment that will employ LArTPC technology in a near detector placed at Fermilab and a far detector at the Sanford Underground Research Facility, at a baseline of 1300 km. The DUNE Liquid Argon Near Detector (ND-LAr) design takes into account the high neutrino intensity expected from the LBNF...

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  155. Andrea Longhin
    25/08/2023, 14:00
    WG3: Accelerator Physics
    Oral

    Monitored neutrino beams represent a powerful and cost effective tool to suppress cross section related systematics for the full exploitation of data collected in long baseline oscillation projects like DUNE and Hyper-Kamiokande. In the last years the NP06/ENUBET project has demonstrated that the systematic uncertainties on the neutrino flux can be suppressed to 1% in an accelerator based...

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  156. Michael Schmidt (UNSW Sydney)
    25/08/2023, 14:00
    WG5: Neutrinos Beyond PMNS
    Oral

    The neutrino sector is currently not well constrained and may be hiding new physics beyond neutrino masses. I will consider a model-independent approach using effective field theory and discuss different ways to probe interactions between neutrinos and quarks using a range of different processes from coherent elastic neutrino nucleus scattering (CE$\nu$NS) and invisible meson decays to lepton...

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  157. Wuming Luo (Institute of High Energy Physics, Chinese Academy of Science)
    25/08/2023, 14:00
    WG1: Neutrino Oscillation Physics
    Oral

    Jiangmen Underground Neutrino Observatory (JUNO), located in the southern part of China, will be the world’s largest liquid scintillator (LS) detector upon completion. Equipped with 20 kton LS, about 17612 20-inch PMTs and 25600 3-inch PMTs in the central detector (CD), JUNO will provide a unique apparatus to probe the mysteries of neutrinos, particularly the neutrino mass ordering puzzle. One...

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  158. Maria Liubarska (University of Alberta)
    25/08/2023, 14:00
    WG2: Neutrino Scattering Physics
    Oral

    IceCube DeepCore, a sub-array of the IceCube neutrino observatory, has a high-density configuration and it is sensitive to neutrinos with energies above a few GeV. In this contribution, we present a measurement of the shape of differential cross section as a function of inelasticity for neutrino-nucleon interactions in the energy range from 100 GeV to 1 TeV. The measurement is based on a...

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  159. 25/08/2023, 14:00
  160. 25/08/2023, 14:00
  161. Prof. Jianming Bian (University of California Irvine (US))
    25/08/2023, 14:20
    WG1: Neutrino Oscillation Physics
    Oral

    DUNE, the flagship next-generation neutrino experiment in the United States, is designed to decisively measure neutrino CP violation and the mass hierarchy. Its far detector modules utilize Liquid Argon Time Projection Chamber (LArTPC) technology, which provides exceptional spatial resolution and the potential to accurately identify final state particles and neutrino events. However, this...

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  162. Vaniya Ansari (Aligarh Muslim University)
    25/08/2023, 14:20
    WG2: Neutrino Scattering Physics
    Oral

    MINERvA is an experiment designed to precisely study neutrino-nucleus interactions in the 1-20 GeV energy range using the NuMI high-intensity neutrino beam at the Fermi National Accelerator Laboratory. MINERvA has improved our knowledge of neutrino cross sections at low energy, low $Q^2$, and the A-dependence in these interactions. These data are interesting in their own right, and have been...

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  163. Meghna Bhattacharya (Fermilab)
    25/08/2023, 14:20
    WG3: Accelerator Physics
    Oral

    The upcoming long baseline neutrino experiments have the goal of enhancing proton beam power to a multi-MW scale and utilizing large-scale detectors to address the challenge of limited event statistics. The DUNE experiment at LBNF will test the three neutrino flavor paradigm and directly search for CP violation by studying oscillation signatures in the high intensity $\nu_{\mu}$...

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  164. Kaare Endrup Iversen (Lund University (SE))
    25/08/2023, 14:40
    WG6: Detector Physics
    Oral

    Accurate and fast event reconstruction is central for the design and performance of the ESSnuSB detectors. While precise, the currently proposed likelihood-based method for event reconstruction is computationally expensive. In recent years, machine learning methods have been implemented for reconstruction in several high energy physics experiments, including neutrino experiments, enabling fast...

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  165. Rudra Majhi
    25/08/2023, 14:40
    WG3: Accelerator Physics
    Oral

    We have studied the capability of different long-baseline experiment options at the KM3NeT facility i.e., P2O, Upgraded P2O and P2SO to probe the light sterile neutrino and compare their sensitivities with DUNE. The P2O option will have neutrinos from a 90 KW beam at Protvino to be detected at the ORCA detector, the Upgraded P2O will have neutrinos from the upgraded 450 KW beam to be detected...

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  166. Andrew Furmanski (University of Minnesota (US))
    25/08/2023, 14:40
    WG2: Neutrino Scattering Physics
    Oral

    The Short-Baseline Near Detector (SBND) is a 100-ton scale Liquid Argon Time Projection Chamber (LArTPC) neutrino detector positioned in the Booster Neutrino Beam at Fermilab, as part of the Short-Baseline Neutrino (SBN) program. The detector is currently under construction and is anticipated to be filled with liquid argon in fall 2023. Located only 110 m from the neutrino production target,...

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  167. Dr. Rukmani Mohanta
    25/08/2023, 14:45
    WG5: Neutrinos Beyond PMNS
    Oral

    In the current epoch of neutrino physics, many experiments are aiming for precision measurements of oscillation parameters. Thus, various new physics scenarios which alter the neutrino oscillation probabilities in matter deserve careful investigation. Recent results from NOvA and T2K show a slight tension on their reported values of the CP violating phase $\delta_{CP}$. Since the baseline of...

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  168. Yusuke Koshio
    25/08/2023, 15:00

    In long-baseline neutrino oscillation experiments, understanding hadron reactions is essential for neutrino generation. Neutrinos are produced by striking a carbon target with proton beam and then decaying the emitted hadrons such as pions and kaons. The hadron interaction is a primary source of the neutrino beam flux prediction uncertainty. Therefore, accurate hadron production and...

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  169. Laura Munteanu (CERN)
    25/08/2023, 15:00
    WG1: Neutrino Oscillation Physics
    Oral

    Neutrino oscillation physics has now entered the precision era. In parallel with needing larger detectors with which to collect more data, future experiments further require a significant reduction of systematic uncertainties with respect to what is currently available. In the neutrino oscillation measurements from the T2K experiment the systematic uncertainties related to neutrino interaction...

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  170. Afroditi Papadopoulou
    25/08/2023, 15:00
    WG2: Neutrino Scattering Physics
    Oral

    The MicroBooNE liquid argon time projection chamber (LArTPC) experiment operated in the Fermilab Booster Neutrino and Neutrinos at the Main Injector beams from 2015-2021. Among the major physics goals of the experiment is a detailed investigation of neutrino-nucleus interactions. MicroBooNE currently possesses the world's largest neutrino-argon scattering data set, with eight published...

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  171. Masato Yamanaka (Yokohama National University)
    25/08/2023, 15:10
    WG4: Muon Physics
    Oral

    The standard model of particle physics is far from accounting for mysteries about our universe, --e.g., what is origin of neutrino masses and their hierarchy?-- and it must be extended to a more fundamental description of nature. Such new physics models allow Charged Lepton Flavor Violating (CLFV) reactions which are exactly forbidden in the standard model. Hence search for CLFV is a clue to...

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  172. Prof. David Caratelli (UC Santa Barbara)
    25/08/2023, 15:20
    WG2: Neutrino Scattering Physics
    Oral

    The modeling of resonant neutrino interactions on argon is a critical aspect of the neutrino oscillation and beyond the standard model physics programs being carried out by the DUNE and Short Baseline Neutrino experiments. Resonant interactions are typically studied in events with pions in the final state. The measurement of 𝜂 production provides a powerful new probe of resonant interactions,...

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  173. Katharina Lachner (University of Warwick)
    25/08/2023, 15:20
    WG6: Detector Physics
    Oral

    The T2K magnetized near detector (ND280) at J-PARC is undergoing a major upgrade with a new 3D fine-granularity scintillator active targe with 3D imaging capabilities as well as ~3mm spatial resolution and sub-ns time resolution, two novel Time Projection Chambers (TPC), surrounded by a precise scintillator-based Time of Flight detector (ToF) with 200 ps time resolution.
    Thanks to such...

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  174. Noah Steinberg (Fermi National Accelerator Laboratory)
    25/08/2023, 15:40
    WG2: Neutrino Scattering Physics
    Oral

    The ability of current and next generation accelerator based neutrino oscillation measurements to reach their desired sensitivity and provide new insight into the nature of our Universe, requires a high-level of understanding of the neutrino-nucleus interactions. These include precise estimation of the relevant cross sections and the reconstruction of the incident neutrino energy from the...

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  175. Adrien Blanchet (University of Geneva)
    25/08/2023, 16:11
    WG1: Neutrino Oscillation Physics
    Oral

    T2K is a long baseline neutrino experiment which exploits a neutrino and antineutrino beam produced at the Japan Particle Accelerator Research Centre (J-PARC) to provide world-leading measurements of the parameters governing neutrino oscillation. Neutrino oscillations are measured by comparing neutrino rates and spectra at a near detector complex, located at J-PARC, and at the water-Cherenkov...

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  176. Yeong Gyun Kim (Gwangju National University of Education)
    25/08/2023, 16:30
    WG2: Neutrino Scattering Physics
    Oral

    SND@LHC is a compact and stand-alone experiment to perform measurements with neutrinos produced at the LHC in a hitherto unexplored pseudo-rapidity region of 7.2 < 𝜂 < 8.6, complementary to all the other experiments at the LHC. The experiment is located 480 m downstream of IP1 in the unused TI18 tunnel. The detector is composed of a hybrid system based on a 800 kg target mass of tungsten...

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  177. 25/08/2023, 16:30
  178. 25/08/2023, 16:30
  179. Minjin Jeong (Sungkyunkwan University)
    25/08/2023, 16:30
    WG5: Neutrinos Beyond PMNS
    Oral

    Although the existence of dark matter has been well established by numerous observations, its nature remains unknown. Dark Matter could be detected indirectly through the observation of neutrinos produced in self-annihilations or decays of dark matter. Objects with large dark matter accumulations such as galaxy clusters or the Galactic dark matter halo are primary targets. Searches for such...

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  180. Ljiljana Morvaj (Paul Scherrer Institute (CH))
    25/08/2023, 16:30
    WG4: Muon Physics
    Oral

    Permanent electric dipole moment (EDM) of a fundamental particle breaks both parity (P) and time-reversal (T) symmetries, implying the violation of charge-parity (CP) symmetry, assuming CPT invariance. With the current experimental sensitivities, an observation of a non-zero muon EDM would indicate new CP violating sources from physics beyond the Standard Model. The experiment at the Paul...

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  181. Adam Aurisano (University of Cincinnati)
    25/08/2023, 16:31

    NOvA is a long-baseline neutrino experiment placed in the muon neutrino-dominated NuMI beam based at the Fermi National Accelerator Laboratory, USA. Utilizing two functionally-identical tracking calorimeters placed 809 km apart, NOvA observes the appearance of electron neutrinos and the disappearance of muon neutrinos. By observing these neutrino oscillations along with their antineutrino...

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  182. Jeremy Atkinson (Universitaet Bern (CH))
    25/08/2023, 16:50
    WG2: Neutrino Scattering Physics
    Oral

    FASER, the ForwArd Search ExpeRiment, at the CERN LHC, is designed to search for new, light, weakly-interacting particles, and investigate high-energy collider neutrino interactions in the TeV regime, extending current cross-section measurements. Located $480$ m downstream from the ATLAS IP, it is aligned with the collision axis line-of-sight, covering a previously unexplored pseudorapidity...

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  183. Dr Luke Pickering (Royal Holloway, University of London)
    25/08/2023, 16:51
    WG1: Neutrino Oscillation Physics
    Oral

    The Deep Underground Neutrino Experiment (DUNE) is a next generation long baseline neutrino experiment for oscillation physics and proton decay studies. The primary physics goals of the DUNE experiment are to perform neutrino oscillation physics studies, search for proton decay, detect supernova burst neutrinos, make solar neutrino measurements and BSM searches. The liquid argon prototype...

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  184. Yechan Kim (KAIST)
    25/08/2023, 16:54
    WG5: Neutrinos Beyond PMNS
    Oral

    Some properties of a neutrino may differ significantly depending on whether it is Dirac or Majorana type. The type is determined by the relative size of Dirac and Majorana masses, which may vary if they arise from an oscillating scalar dark matter. We show that the change can be significant enough to convert the neutrino type between Dirac and Majorana while satisfying constraints on the dark...

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  185. Patrick Strasser (KEK)
    25/08/2023, 17:00
    WG4: Muon Physics
    Oral

    At the J-PARC Muon Science Facility (MUSE), the MuSEUM collaboration is planning new measurements of the ground state hyperfine structure (HFS) of both muonium and muonic helium atom.
    Muonium (a bound state of a positive muon and an electron) and muonic helium (a helium atom with one of its electrons replaced by a negative muon) are both hydrogen-like atoms. Their respective ground-state HFS...

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  186. Hitoshi Oshima (ICRR, the University of Tokyo)
    25/08/2023, 17:10
    WG2: Neutrino Scattering Physics
    Oral

    The NINJA collaboration aims to study neutrino-nucleus interactions in the energy range of hundreds of MeV to a few GeV using an emulsion-based detector. A series of neutrino-nucleus interaction measurements was conducted using the emulsion detector with water and iron targets in the near detector hall of the T2K experiment at J-PARC. The emulsion detector is suitable for precision...

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  187. Charlie Naseby
    25/08/2023, 17:11
    WG1: Neutrino Oscillation Physics
    Oral

    The next-generation water Cherenkov experiment Hyper-Kamiokande (HK) includes a rich long-baseline neutrino oscillation component. This will make use of a 1.3MW proton beam from J-PARC, coupled with a suite of near detectors, including an upgraded ND280 and a new Intermediate Water Cherenkov Detector (IWCD). The 185 kton fiducial mass Hyper-Kamiokande will be used for the far detector. The...

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  188. salvador urrea (Instituto de Física Corpuscular(IFIC) Valencia, Spain)
    25/08/2023, 17:18
    WG5: Neutrinos Beyond PMNS
    Oral

    The exquisite capabilities of liquid Argon Time Projection Chambers make them ideal to search for weakly interacting particles in Beyond the Standard Model scenarios. Given their location at CERN the ProtoDUNE detectors may be exposed to a flux of such particles, produced in the collisions of 400 GeV protons (extracted from the Super Proton Synchrotron accelerator) on a target. Here we point...

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  189. Andrew Sutton
    25/08/2023, 17:30
    WG2: Neutrino Scattering Physics
    Oral

    The Accelerator Neutrino Neutron Interaction Experiment (ANNIE) is a Gadolinium-loaded water Cherenkov detector placed in the Booster Neutrino Beam (BNB) at the Fermi National Accelerator Laboratory, USA. The primary physics goal of ANNIE is to perform neutrino cross-section measurements that will constrain systematic uncertainties in the next generation of long-baseline neutrino experiments....

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  190. Youngwan Kim (Seoul National University (KR))
    25/08/2023, 17:30

    Several experimental observations lead to the availability of lepton-flavor violating(LFV) processes, which is also thoroughly examined by the CMS experiment. In this presentation, several recent LFV results from CMS within different sectors are presented.

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  191. Papia Panda
    25/08/2023, 17:31
    WG1: Neutrino Oscillation Physics
    Oral

    In this paper we study the possibility of determining the neutrino mass ordering sensitivity from the future supernova neutrino events at the DUNE and T2HK detectors. We estimate the expected neutrino event rates from a future supernova explosion assuming GKVM flux model corresponding to different processes that are responsible for detecting the supernova neutrinos at these detectors. We...

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  192. Jacob Zettlemoyer
    25/08/2023, 17:42
    WG5: Neutrinos Beyond PMNS
    Oral

    The accelerator complex at Fermilab is currently undergoing improvements which will increase the available beam power to the complex and is known as Proton Improvement Plan-II (PIP-II). The PIP-II Linac is slated for operation near the end of this decade and will be the main proton driver for Fermilab experiments moving forward and provide the beam to LBNF/DUNE. However, the DUNE physics...

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  193. Yuri V Efremenko
    25/08/2023, 17:50
    WG2: Neutrino Scattering Physics
    Oral

    COHERENT collaboration at the Spallation Neutrino Source (SNS) at ORNL utilizing intensive low energy neutrino flux to measure various neutrino interactions. Range of interest is from Coherent Elastic Neutrino Scattering (CEvNS) up to nuclear charge current and neutral current interactions of interest for the support of Supernova neutrino detection in large detectors. We will review present...

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  194. Lluis Marti
    25/08/2023, 17:51
    WG1: Neutrino Oscillation Physics
    Oral

    Super-Kamiokande, a 50 kton water Cherenkov underground neutrino detector, has been instrumental in studying neutrinos across a wide energy range, from a few MeV to hundreds of GeV. Alongside SNO, Super-Kamiokande has played a pivotal role in providing evidence for solar neutrino oscillations. Specifically, the detection of Boron-8 neutrinos highlighted the deficit in the observed neutrino...

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  195. Francesca Dordei (INFN, Cagliari (IT))
    25/08/2023, 18:00
    WG4: Muon Physics
    Oral

    In this talk, I will present recent results with heavy flavour decays at the LHCb experiment. Future prospects will be highlighted in view of the recent start of Run 3 of the LHC. In particular, I will focus on searches for new physics and tests of lepton flavour universality that are particularly sensitive to the presence of physics beyond the Standard Model.

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  196. Xiao Luo
    25/08/2023, 18:06
    WG5: Neutrinos Beyond PMNS
    Oral

    The Short-Baseline Near Detector (SBND) is a 112-ton liquid argon time projection chamber (LArTPC) detector located 110-meters downstream the Booster Neutrino Beam target at Fermilab. As the near detector of the Short-Baseline Neutrino Program, SBND is especially sensitive to any new particles produced in the beam. In addition to the excellent spatial and energy resolution of the LArTPC...

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  197. Lukas Koch (Johannes Gutenberg Universitaet Mainz (DE))
    25/08/2023, 18:10
    WG2: Neutrino Scattering Physics
    Oral

    Precise knowledge of how neutrinos interact with matter is essential for measuring neutrino oscillations in long-baseline experiments. At T2K, the near detector complex measures neutrino interactions to constrain cross-section models for oscillation studies and to characterise the beam flux. The near detector complex provides a platform for performing neutrino-nucleon cross section...

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  198. Roberto Mandujano
    25/08/2023, 18:11
    WG1: Neutrino Oscillation Physics
    Oral

    The Jiangmen Underground Neutrino Observatory (JUNO) is a 20 kton liquid scintillator detector scheduled to come online in 2024 with a main physics goal of precisely measuring reactor antineutrino oscillations. JUNO is located at a distance of 53 km from eight nuclear reactors in Southern China. The detector will be instrumented by 17,612 20-inch and 25,600 3-inch photomultiplier tubes,...

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  199. Adam Aurisano (University of Cincinnati)
    26/08/2023, 08:30
  200. Christophe Bronner
    26/08/2023, 08:50
  201. Natalia Milas (European Spallation Source)
    26/08/2023, 09:10
  202. Yuki Fujii (Monash University (AU)), Yuki Fujii
    26/08/2023, 09:30
  203. koun choi (IBS)
    26/08/2023, 09:50
  204. Yasuhiro NISHIMURA (Keio University)
    26/08/2023, 10:10
  205. Francesca Dordei (INFN, Cagliari (IT))
    26/08/2023, 10:30
  206. Kevin McFarland (University of Rochester)
    26/08/2023, 11:10
  207. Prof. Siyeon Kim
    26/08/2023, 11:40
  208. Prof. Jonghee YOO (Seoul National University)
    26/08/2023, 12:00
  209. Jeong Yeol Yang
    WG1: Neutrino Oscillation Physics
    Poster

    We report a study of time variations of solar Neutrino flux using 5,804 live days of Super-Kamiokande data. The data used in this analysis were obtained from 31 May 1996 to 30 May 2018. The measured exact time of high-yield solar neutrino events for 22 calendar years of accumulated data allows for studying solar neutrino modulations with unprecedented precision. The measured time variation of...

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  210. Dr Sang Yong KIM (Chonnam National University)
    WG1: Neutrino Oscillation Physics
    Poster

    The RENO Collaboration reports a measured value of the smallest neutrino mixing angle ($\theta_{13}$) based on ~2800 days of reactor electron antineutrino events with a delayed signal of neutron capture on hydrogen (H). The neutron captures on H emitting a 2.2 MeV $\gamma$-ray are not easily detected because of high environmental radioactivity below 3.5 MeV, Due to satisfactory purification of...

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  211. Eli Mygatt Ward
    WG2: Neutrino Scattering Physics
    Poster

    At Oak Ridge National Laboratory (ORNL), the COHERENT collaboration has been building a heavy water Cherenkov detector to measure the neutrino flux coming from the Spallation Neutron Source (SNS). This detector is a steel cylinder filled with light water with an inner acrylic vessel holding heavy water and twelve PMTs lining the inside of the top lid. It began accumulating statistics in summer...

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  212. Naoto Onda (Kyoto University)
    WG6: Detector Physics
    Poster

    T2K experiment is a long-baseline neutrino oscillation experiment in Japan. One of the T2K goals is to obtain evidence of CP-violation in the leptonic sector at 3σ confidence level. To archive this goal, the reduction of systematic errors is needed, and a new plastic scintillator tracker (Super-FGD) will be installed in the near detector in 2023.
    However, in the era of Hyper-Kamiokande (HK)...

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  213. Nari Kim (Chonnam national University)
    WG6: Detector Physics
    Poster

    Linear alkyl benzene (LAB)-based liquid scintillator (LS) has been widely used as the target for neutrino detectors in recent decades due to its environmentally friendly and economic characteristics. The reconstruction of neutrino events is based on the scintillation light emitted from the LS; thus, understanding the LS response helps to understand the reconstructed neutrino event. It has been...

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  214. Dr. Rukmani Mohanta
    WG5: Neutrinos Beyond PMNS
    Poster

    In the current era of precision measurements, one of the prime objectives of various neutrino oscillation experiments is to look for the signals of sub-leading effects in the three flavour neutrino oscillation framework. It is therefore, crucial to distinguish between the different new physics scenarios so that they their origin and implications can be well understood theoretically. As the...

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  215. mitesh behera
    WG5: Neutrinos Beyond PMNS
    Poster

    We typically prioritize discrete symmetries when exploring neutrino phenomenology. In this context, we examine neutrino masses and mixing within the linear seesaw framework by utilizing a simple permutation group known as $S_3$ symmetry. To simplify the complexity of vacuum alignments and avoid the need for multiple flavon fields, we incorporate modular symmetries, which prove advantageous....

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  216. Mr Abinash Medhi (Tezpur University, Assam, India)
    WG5: Neutrinos Beyond PMNS
    Poster

    The experimental observation of the phenomena of neutrino oscillations was the first firm experimental evidence of physics beyond the Standard Model (SM). The SM of particle physics needs an extension to explain the neutrino masses and mixing. The models describing beyond SM physics usually comes with some additional unknown couplings of neutrinos termed as Non Standard Interactions (NSIs)....

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  217. Mr Arnab Sarker (Tezpur University, Assam, India)
    WG5: Neutrinos Beyond PMNS
    Poster

    The theoretical possibility of a small deviation from the fundamental space-time symmetry is referred to as Lorentz invariance violation (LIV). This violation of the Lorentz invariance symmetry implies that laws of physics can vary under Lorentz transformation. LIV is intrinsic in nature and can exist even in a vacuum. The weakly interacting neutrinos can be a probe for better understanding...

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  218. Afroditi Papadopoulou
    Poster

    Making high-precision measurements of neutrino oscillation parameters requires an unprecedented understanding of neutrino-nucleus scattering. In this work, we present the first charged current double-differential cross sections in kinematic imbalance variables. These variables characterize the imbalance in the plane transverse to an incoming neutrino. We use events with a single muon above 100...

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  219. Ji-Young CHOI
    WG6: Detector Physics
    Poster

    This paper attempts to perform spectral discrimination of fluorescence images of liquid scintillators acquired by complementary metal oxide semiconductor (CMOS) image sensors using the discriminative ability of deep convolutional neural networks without any special effort. As semiconductor fab-processing technology has advanced, so has the processing technology of optical elements in image...

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  220. Anjan Giri
    WG5: Neutrinos Beyond PMNS
    Poster

    The upcoming long-baseline (LBL) neutrino experiments will be sensitive to non-standard interaction effects and can provide information on the unknown oscillation parameter values. We explore the parameter degeneracies that can occur in DUNE, T2HK experiments, and a combination of both due to nonstandard interactions (NSI) arising simultaneously from two different off-diagonal sectors, i.e.,...

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  221. prameet kumar gaur (Aligarh Muslim University, Aligarh(202001), India)
    WG2: Neutrino Scattering Physics
    Poster

    The MINERvA experiment at Fermilab uses $\approx$ 3 GeV(LE) and $\approx$ 6 GeV(ME) NuMI neutrino and antineutrinos beams interacting on different nuclear targets (He, C, Fe, Pb, Water and CH) located throughout the detector. Reported here is the ME antineutrino measurement of the inclusive double differential charged current cross section as a function of Bjorken x and four momentum...

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  222. Dinesh Kumar Singha
    WG5: Neutrinos Beyond PMNS
    Poster

    Neutrinos can interact with some scalar fields through some unknown couplings referred as scalar non-standard interaction (SNSI). Unlike vector NSI, SNSI parameters do not appear as potential term in neutrino oscillation rather appeared as a correction to neutrino mass term. Significant effects of SNSI parameters on neutrino oscillation can be observed at neutrino long baseline experiments....

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  223. Katsuya Yonehara
    WG3: Accelerator Physics
    Poster

    With the Main Injector Neutrino Oscillation Search (MINOS) experiment decommissioned, muon and hadron monitors became an important diagnostic tool for the NuMI Off-axis $v_\mu$ Appearance (NOvA) experiment at Fermilab to monitor the Neutrinos at the Main Injector (NuMI) beam. The goal of this study is to maintain the quality of the monitor signals and to establish correlations with the...

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  224. Jiaxi Liu
    Poster

    The Jiangmen Underground Neutrino Observatory (JUNO) is a next-generation large (20 kton) liquid-scintillator neutrino detector, which is designed to determine the neutrino mass ordering from its precise reactor neutrino spectrum measurement. Moreover, high-energy (GeV-level) atmospheric neutrino measurements could also improve its sensitivity to mass ordering via matter effects on...

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  225. Dojin Kim
    WG1: Neutrino Oscillation Physics
    Poster

    The RENO experiment reports the separated reactor antineutrino spectra of 235U and 239Pu from the data sets of 2500 days of near data. As the fission fractions changes as the fuel cycle evolve, the contribution from different fissile isotopes to the measured spectrum can be identified. The separated prompt spectra are unfolded to antielectron neutrino spectra where the detector effect is...

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  226. ILMA - (ALIGARH MUSLIM UNIVERSITY)
    WG5: Neutrinos Beyond PMNS
    Poster

    New physics beyond the Standard Model (SM) may appear in the form of unknown couplings, typically termed non-standard neutrino interactions (NSIs) can manifest in neutrino interactions. To explain such a process, NSI offers a general "Effective Field Theory"(EFT)-style framework. While the elements of a given model may differ in weak interactions, they are broadly categorized as charge current...

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  227. Dr Sohtaro Kanda
    WG4: Muon Physics
    Poster

    Muons have been widely used as probes in searches for new physics via precision measurements and rare decay searches. Muon sources with a high-intensity proton beam have enabled experiments requiring high statistics. However, techniques for muon cooling with high efficiency are essential for further breakthroughs in searches for physics beyond the Standard Model.
    The ultra-slow muon (USM) at...

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  228. Lalnuntluanga R
    WG2: Neutrino Scattering Physics
    Poster

    Heavy nuclear targets are used in neutrino oscillation experiments to boost the statistics of neutrino interactions. The complex nuclear environment contributes to the systematic uncertainty as the inevitable nuclear effects. Inadequate knowledge of the neutrino interaction with the nuclear target along with the imperfect reconstruction of neutrino energy seeds uncertainty in the...

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  229. Wonjun Lee
    WG1: Neutrino Oscillation Physics
    Poster

    We report a conceptual design of Reactor Experiment for Neutrinos and Exotics (RENE), which primarily aims to search for the sterile neutrino oscillation at $\Delta m_{41}^2 \sim 2 eV^2$.
    The joint study of RENO and NEOS experiments showed a hint for the sterile neutrinos at $\Delta m_{41}^2 \sim 2.4 eV^2$ and $\sim 1.7 eV^2$, which overlap with the allowed region by the Reactor...

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  230. Ananya Mukherjee
    WG5: Neutrinos Beyond PMNS
    Poster

    The generic inverse seesaw (ISS) framework is unable to produce an adequate amount of lepton asymmetry, which consequently fails to generate the observed baryon asymmetry of the Universe (BAU). This happens due to mainly two reasons, (i) partial cancellation of the lepton asymmetries
    among the pseudo-Dirac pairs, and (ii) strong wash out caused by the inverse decays. In this work we offer two...

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  231. Seunghyun Jung
    WG1: Neutrino Oscillation Physics
    Poster

    It is crucial to understand the atmospheric neutrino interaction (ATM-$\nu$) in order to search for the nucleon decay (NDK) in the Super-Kamiokande (SK). In this poster, neutron tagging for ATM-$\nu$ background reduction will be introduced and sensitivity obtained by spectrum analysis for $\pi$ momentum distributions from ATM-$\nu$ background and NDK signal MC will be reported using improved...

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  232. Jun Kai Ng (Shanghai Jiao Tong University)
    WG4: Muon Physics
    Poster

    The proposed muEDM experiment at the Paul Scherrer Institute (PSI) in Switzerland is designed to search for a muon EDM with a sensitivity of 6×10^(-23) e⋅cm. It leverages the frozen-spin technique, which cancels the muon's anomalous precession within a compact storage solenoid. This approach considerably enhances the sensitivity of the search compared to the parasitic method using a storage...

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  233. Mun Jung Jung (University of Chicago)
    WG2: Neutrino Scattering Physics
    Poster

    The Short-Baseline Near Detector (SBND), a liquid argon time projection chamber (LArTPC) located at Fermilab, will soon start collecting over a million neutrino events per year. For SBND and other neutrino experiments like DUNE, modeling neutrino-nucleus interactions with heavy nuclei at the few-GeV energy range is a significant challenge. In this range, neutrinos scatter on heavy nuclei...

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  234. 지웅 이
    WG6: Detector Physics
    Poster

    The IceCube Neutrino Observatory, located at the geographic South Pole, has currently the largest volume among neutrino detectors. IceCube detects neutrinos using Cherenkov light emissions from charged particles produced in neutrino interactions. The optical properties of the ice in the detector is one of the major systematic uncertainties for analyses using IceCube data. One of the major...

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  235. Hyeon Woo Park (Chonnam National University, Department of physics)
    WG6: Detector Physics
    Poster

    Bi-alkali photomultiplier tube (PMT) has a maximum quantum efficiency (QE) around 430nm. Fluor components dissolved in liquid scintillator (LS) are needed to have an emission wavelength in the PMT’s QE region. We analyzed digital images for estimating the spectrum of LS, instead of using a spectrophotometer. Digital image was taken by camera based on complementary metal oxide semiconductor...

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