Oct 26โ€‰โ€“โ€‰30, 2026
Art Center, Chung-Ang University
Asia/Seoul timezone

Session

Plenary Session

Oct 28, 2026, 8:40โ€ฏAM
CAU Art Hall (Art Center, Chung-Ang University)

CAU Art Hall

Art Center, Chung-Ang University

84 Heukseok-ro, Dongjak District, Seoul

Conveners

Plenary Session: A

  • Sin Kyu Kang (Seoul National University of Science and Technology)

Plenary Session: B

  • Yoomin Oh

Plenary Session: C

  • Jianming Bian

Plenary Session: D

  • Chang Hyon Ha (Chung-Ang University)

Plenary Session: F

  • Guang Yang (Brookhaven Naitonal Laboratory)

Plenary Session: G

  • Eunju Jeon (Institute for Basic Science)

Plenary Session: H

  • Myeonghun Park

Plenary Session: I

  • Mariam Tortola

Plenary Session: J

  • Chris Marshall (University of Rochester)

Plenary Session: K

  • Jay Hyun Jo

Presentation materials

There are no materials yet.

  1. Mariam Tortola
    10/28/26, 8:40โ€ฏAM
  2. Chris Marshall (University of Rochester)
    10/28/26, 9:10โ€ฏAM
  3. Eunju Jeon (Institute for Basic Science)
    10/28/26, 10:10โ€ฏAM
    Oral (Invited)

    Neutrinoless double beta decay offers the most sensitive laboratory access to lepton number violation and to the Majorana nature of the neutrino, and the reach of any search is set directly by detector performance. I will review where the field stands: the leading experiments have set half-life limits above 10^26 yr in 136Xe and 76Ge, while the 130Te and 100Mo programs are now moving to their...

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  4. David Hervas Aguilar (TUM)
    10/28/26, 10:40โ€ฏAM
    Oral (Invited)

    The LEGEND collaboration is searching for neutrinoless double-beta decay
    ($0\nu\beta\beta$) of $^{76}$Ge in the first phase of its experimental
    program, LEGEND-200. Building on key technological innovations from its
    predecessor high-purity germanium experiments, GERDA and the MAJORANA
    DEMONSTRATOR, LEGEND aims to realize the tonne-scale LEGEND-1000
    experiment, with a discovery sensitivity...

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  5. Veronika Palusova
    10/28/26, 11:00โ€ฏAM
    Oral (Contribution)

    Double beta plus decay modes (๐›ฝ+๐›ฝ+, ๐›ฝ+๐ธ๐ถ, and 2๐ธ๐ถ) are rare second-order weak processes converting two protons into two neutrons. Their observation is difficult due to extremely low probabilities, complex signatures, and the low natural abundance of suitable isotopes.
    Studying these decays offers insights into nuclear structure and fundamental symmetries. Decay rates depend on nuclear matrix...

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  6. 10/28/26, 11:20โ€ฏAM
  7. Jiajie Ling
    10/28/26, 2:00โ€ฏPM
  8. Jay Hyun Jo
    10/28/26, 2:30โ€ฏPM
    Oral (Invited)

    Abstract: Short-baseline accelerator neutrino experiments sit at the intersection of several open questions in neutrino physics. Persistent anomalies at L/E ~ 1 m/MeV, most notably the LSND and MiniBooNE electron-flavor excesses, have motivated a dedicated experimental program to test the existence of light sterile neutrinos, while the same detectors provide high-statistics measurements of...

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  9. Ornella Palamara (Fermilab), Ornella Palamara (Fermilab)
    10/28/26, 3:00โ€ฏPM
    Oral (Contribution)

    The Short-Baseline Near Detector (SBND) is one of three liquid argon time projection chamber (LArTPC) neutrino detectors positioned along the axis of the Booster Neutrino Beam (BNB) at Fermilab, and serves as the near detector in the Short-Baseline Neutrino (SBN) Program. The detector just completed its second year of running, collecting over 6.5e20 POT, equivalent to an unprecedented sample...

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  10. Matthias Meier
    10/28/26, 3:20โ€ฏPM
    Oral (Invited)

    After the first detection of coherent elastic neutrino-nucleus scattering (CEฮฝNS) using reactor antineutrinos in the fully coherent regime in 2025, the CONUS+ experiment continued its measurements. Between the just mentioned Run-1 data and the latest Run-2 measurement, three of the four 1 kg germanium detectors were upgraded to 2.4 kg of active volume, which provide similar or even better...

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  11. Graziano Rossi
    10/28/26, 4:10โ€ฏPM
  12. Riya Shah (Kavli IPMU - UTokyo)
    10/28/26, 4:40โ€ฏPM
    Oral (Invited)

    High-energy neutrinos provide a unique window into the most extreme environments in the Universe, carrying information from otherwise inaccessible regions and offering a complementary view to electromagnetic and gravitational-wave observations. Since the discovery of the diffuse flux of high-energy astrophysical neutrinos by the IceCube Neutrino Observatory, IceCube and other large-scale water...

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  13. Juan Pablo Yanez, Juan Pablo Yanez (University of Alberta)
    10/28/26, 5:10โ€ฏPM
    Oral (Invited)

    The IceCube Neutrino Observatory is the largest Cherenkov neutrino telescope in operation. Located deep in the Antarctic ice sheet at the South Pole, IceCube has been operating in its full configuration for over 15 years. With its low-energy extension, DeepCore, the detector has produced precision measurements of neutrino oscillations and stringent limits on new physics. During the last Pole...

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  14. Woosik Kang (Drexel University)
    10/28/26, 5:30โ€ฏPM
    Oral (Contribution)

    The discovery of a diffuse astrophysical neutrino flux by IceCube in 2013 marked the beginning of the TeV-PeV neutrino astronomy era. This was followed by reports of evidence for neutrino emission from two active galaxies (TXS 0506+056 and NGC 1068), as well as an excess of neutrinos from the galactic plane of the Milky Way. However, the source classes responsible for extragalactic neutrinos...

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  15. Prof. Jose Bazo (Pontificia Universidad Catolica del Peru)
    10/28/26, 5:50โ€ฏPM
    Oral (Invited)

    The detection of astrophysical PeV neutrinos by current neutrino observatories has established neutrino astronomy as a powerful tool for exploring the high-energy universe. However, the identification of astrophysical sources remains challenging due to the large background from atmospheric neutrinos. The Tau Air-Shower Mountain-Based Observatory (TAMBO) is a next-generation experiment designed...

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  16. Erin Yandel (Los Alamos National Lab)
    10/29/26, 8:00โ€ฏAM
    Oral (Invited)

    The Deep Underground Neutrino Experiment (DUNE) is a next-generation long-baseline neutrino oscillation experiment designed to make measurements of neutrino oscillations with high precision and probe for new physics. Neutrinos will be measured at two detector facilities, namely a Near Detector (ND) located at Fermilab close to where the neutrino beam is produced by the Long-Baseline Neutrino...

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  17. Anyssa Navrer-Agasson
    10/29/26, 8:20โ€ฏAM
    Oral (Invited)

    The Deep Underground Neutrino Experiment (DUNE), hosted by Fermi National Accelerator Laboratory and with its far detector located at the Sanford Underground Research Facility in South Dakota, represents the flagship next-generation long-baseline neutrino oscillation experiment. As part of DUNE Phase-II, the third far detector module (FD3) is a critical milestone in expanding the experiment's...

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  18. Maritza J. Delgado Gonzalez (INFN Milano Bicocca)
    10/29/26, 8:40โ€ฏAM
    Oral (Contribution)

    DUNE is an international long baseline neutrino experiment and will be the largest of its kind. It will determine the neutrino mass ordering, search for CP violation in the lepton sector, and perform precision tests of the neutrino oscillation paradigm. DUNE will use an intense muon neutrino beam produced, together with a Near Detector located on the Fermilab site and a Far Detector installed...

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  19. Anatael Cabrera (CNRS / Universitรฉ Paris-Saclay)
    10/29/26, 9:00โ€ฏAM
    Oral (Invited)

    The Double Chooz experiment delivered some of the most precise reactor-antineutrino measurements to date. With its legacy established and backgrounds well characterised, the Chooz underground site โ€” powered by two N4-generation PWR cores โ€” remains one of Europeโ€™s most compelling facilities for reactor-antineutrino physics. Two new programmes are now charting the siteโ€™s next chapter (3rd...

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  20. Robert Kralik (King's College London)
    10/29/26, 10:00โ€ฏAM
    Oral (Contribution)

    Hyper-Kamiokande is the next-generation large-scale water Cherenkov neutrino experiment, currently under construction in Japan. Its ambitious physics programme, including precision measurements of neutrino oscillations, searches for nucleon decay, and observations of neutrinos from astrophysical sources, places demanding requirements on detector performance and instrumentation.

    This...

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  21. Minfang Yeh
    10/29/26, 10:20โ€ฏAM
  22. Andrew Santos (Kavli IPMU - UTokyo)
    10/29/26, 10:40โ€ฏAM
    Oral (Invited)

    The Super-Kamiokande (SK) experiment is a world-leading, 50-kton water Cherenkov detector in Japan. Gadolinium sulfate has been loaded into the tank at 0.01% and 0.03% by mass in 2020 and 2022, respectively, to start the SK-Gd era and significantly improve the identification of neutron captures. Here, we discuss the status of SK-Gd, its latest results, and some prospects for the future. Topics...

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  23. Sunhong Kim
    10/29/26, 11:00โ€ฏAM
    Oral (Contribution)

    We evaluate the expected performance of a water Cherenkov detector for reactor antineutrino--electron elastic scattering at the RENO near-detector site. The reactor-spectrum normalization is extracted from the reconstructed recoil-electron directional distribution using a constrained profile-likelihood analysis, while the effects of different event-selection thresholds and relevant background...

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  24. Yechan Kim (KAIST)
    10/29/26, 11:15โ€ฏAM
    Oral (Contribution)

    Fundamental properties of neutrinos need not remain constant, but may become dynamical through a non-standard interaction with the dark sector. An oscillating wave dark matter can induce periodic variations in neutrino mass or transitions between Dirac and Majorana types. The resulting dynamics can modulate rare neutrino processes, including neutrinoless double beta decay and cosmic neutrino...

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  25. Lorenzo Perisse (ILANCE (CNRS - UTokyo))
    10/29/26, 2:00โ€ฏPM
    Oral (Contribution)

    Hyper-Kamiokande (HK) is the next generation of water Cherenkov detector in Japan,currently under construction and scheduled to begin data-taking in 2028. With a fiducial volume about 8 times larger than Super-Kamiokande's (SK), HK will record an unprecedented number of neutrino interactions, enabling precise measurements of neutrino oscillation parameters, searches for CP violation in the...

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  26. Jianming Bian
    10/29/26, 2:20โ€ฏPM
  27. Kazuhiro Terao
    10/29/26, 2:40โ€ฏPM

    Deep learning, particularly techniques adapted from modern computer vision, has substantially advanced the analysis capabilities of particle and nuclear physics experiments, neutrino experiments in particular. Most of these applications, however, rely on supervised learning: the model is trained on simulated events with known labels, and therefore inherits the assumptions and imperfections of...

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  28. Jeong In Yun
    10/29/26, 3:40โ€ฏPM
  29. Giulia Ricciardi (Dipartimento di Fisica E. Pancini, Universita' di Napoli Federico II)
    10/29/26, 3:55โ€ฏPM
    Oral (Contribution)

    The neutrino signal from SN1987A offers a unique opportunity to study the
    dynamics of core-collapse supernovae, but its interpretation has been hindered
    by detector timing uncertainties and ambiguities in the origin of the earliest
    events. I will present a new statistical analysis combining neutrino energies,
    arrival times, and angular distributions within a realistic parametric...

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  30. Guang Yang (Brookhaven National Laboratory)
    10/29/26, 4:15โ€ฏPM
    Oral (Contribution)

    Next-generation neutrino oscillation experiments such as the Deep Underground Neutrino Experiment require percent-level knowledge of neutrino-nucleon interaction cross sections. The Electron-Ion Collider and future nuclear collider has the capability of selecting certain spin and isospin state with controlled incident particle energy. Given that, there are a few ways to constrain a few key...

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  31. Cong Guo
    10/30/26, 8:00โ€ฏAM
    Oral (Invited)

    The Jiangmen Underground Neutrino Observatory (JUNO) is a 20โ€‘kt liquidโ€‘scintillator detector operating at a baseline of ~53โ€ฏkm from two nuclear reactor complexes in southern China. Its primary goal is to determine the neutrino mass ordering via reactor antineutrinos, exploiting excellent energy resolution and low background.

    Since detector commissioning in 2025, JUNO has been taking stable...

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  32. Rhiannon Smith-Jones (University of Sheffield)
    10/30/26, 8:30โ€ฏAM
    Oral (Invited)

    DUNE is a next-generation long-baseline neutrino oscillation experiment and underground neutrino observatory using liquid argon time projection chamber technology. DUNE will measure neutrino and antineutrino oscillations as a function of energy over more than a full oscillation period. It will definitively resolve the neutrino mass ordering and measure the mixing matrix parameters, including...

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  33. Christophe Bronner (Yokohama National University)
    10/30/26, 9:00โ€ฏAM
    Oral (Invited)

    Hyper-Kamiokande is the next generation Water Cherenkov experiment in Japan, following the highly successful Kamiokande and Super-Kamiokande experiments. It is currently under construction and will start taking data in 2028. The experiment is located in two sites separated by 295 km, with a massive 258 kilotonne water Cherenkov detector located in Kamioka town on one side, and a neutrino...

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  34. Tomoko Ariga
    10/30/26, 9:50โ€ฏAM

    The Large Hadron Collider (LHC) produces the highest-energy accelerator
    neutrinos, providing new opportunities to study neutrino interactions at
    TeV energies. The FASER and SND@LHC experiments have successfully
    detected neutrinos originating from LHC collisions and have begun
    exploring this previously unmeasured energy regime with accelerator
    neutrinos.

    In this talk, I will review...

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  35. Yun-Tse Tsai
    10/30/26, 10:20โ€ฏAM

    Coherent elastic neutrinoโ€“nucleus scattering (CEvNS) is a neutral-current weak interaction in which a neutrino scatters coherently from an entire nucleus at low momentum transfer. The coherent enhancement of the nuclear weak charge yields a cross section that scales approximately as N^2, while the associated nuclear recoils are typically at the keV or sub-keV scale. The Standard-Model...

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  36. Manfred Lindner (Max-Planck-Institute fรผr Kernphysik)
    10/30/26, 10:50โ€ฏAM
  37. 10/30/26, 11:20โ€ฏAM
  38. Riya Shah
  39. Kazuhiro Terao
  40. Kazuhiro Terao
  41. Andrew Santos
  42. Juseong Park (CAU)

    Thank you for coming to Seoul.
    Test!

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