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NuFact 2026 - The 27th International Workshop on Neutrinos from Accelerators

August 31, 2026 to September 5, 2026
Tsung-Dao Lee Institute
Asia/Shanghai timezone
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Session

WG6 — Simulation, Backgrounds & Low-Energy Performance

Sep 3, 2026, 3:25 PM
Tsung-Dao Lee Institute

Tsung-Dao Lee Institute

No.1 Lisuo Road, Pudong New District, Shanghai, 201210, China

Conveners

WG6 — Simulation, Backgrounds & Low-Energy Performance

  • Akira Takenaka (Tsung-Dao Lee Institute, Shanghai Jiao Tong University)

Presentation materials

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  1. 32. A Simulation Study of Neutrino-Induced Backgrounds in the Intermediate Water Cherenkov Detector for Hyper-Kamiokande
    Akari Oka (Keio Univertsity)
    9/3/26, 3:25 PM
    WG6: Detector Physics
    Oral contribution

    In the Hyper-Kamiokande experiment, controlling systematic uncertainties is essential to achieve the projected precision of long-baseline neutrino oscillation measurements. To constrain uncertainties associated with neutrino interaction cross sections, the Intermediate Water Cherenkov Detector (IWCD) is being developed as a movable water Cherenkov detector located 870 m from J-PARC along the...

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  2. 92. 9Li/8He estimation and reduction in JUNO
    赖浩菁 （Haojing Lai) (Shanghai Jiao Tong University)
    9/3/26, 3:50 PM
    WG6: Detector Physics
    Oral contribution

    In the Jiangmen Underground Neutrino Observatory (JUNO), cosmogenic muon-induced radioactive isotopes, particularly ⁹Li/⁸He, which undergo β-n decays, produce correlated signals that closely mimic the inverse beta decay (IBD) signature. This constitutes one of the major backgrounds for reactor antineutrino oscillation analyses, with an initial rate of ~60/day before applying any muon veto....

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  3. 82. Core-Collapse Supernova Neutrino Monitoring System in JUNO
    Aman Gupta (Institute of High Energy Physics (IHEP), Beijing)
    9/3/26, 4:15 PM
    WG6: Detector Physics
    Oral contribution

    The Jiangmen Underground Neutrino Observatory (JUNO) is a 20-kiloton liquid scintillator detector with excellent sensitivity to detect neutrinos from the next Core-Collapse Supernova (CCSN). The real-time CCSN monitoring system of JUNO is designed to provide fast and reliable alerts by tracking the increasing event rate of supernova burst neutrinos and pre-supernova neutrinos.

    The...

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