15–18 Jun 2026
NTHU
Asia/Taipei timezone

Session

Neutrino Physics

15 Jun 2026, 08:45
Physics Building R124 (NTHU)

Physics Building R124

NTHU

Conveners

Neutrino Physics

  • Martin Spinrath (NTHU)

Neutrino Physics

  • Po-Yen Tseng (National Tsing Hua University, Department of Physics)

Presentation materials

There are no materials yet.

  1. Pedro Machado (Fermilab)
    15/06/2026, 08:45
    Neutrino Physics
    Invited Presentation

    In this talk I will motivate the vibrant BSM program in neutrino experiments, from a broad perspective. As examples, I will present two very distinct BSM scenarios that could lead to interesting signatures: ultralight dark matter coupled to neutrinos, and compositeness as the source of neutrino mass.

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  2. Joao Paulo Pinheiro (TDLI)
    15/06/2026, 09:30
    Neutrino Physics
    Invited Presentation

    Measuring the leptonic CP phase $\delta_{CP}$ and resolving the
    $\theta_{23}$ octant are primary objectives of DUNE and T2HK.
    We show that two distinct effects can compromise the reliability of
    these measurements. First, the poorly constrained $\nu_e$ and
    $\bar{\nu}_e$ cross sections allow energy-dependent distortions that
    partially mimic the $\delta_{CP}$-dependent spectral...

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  3. Jakob EHRING (Academia Sinica, Institute of Physics)
    18/06/2026, 14:15
    Neutrino Physics
    Invited Presentation

    Massive stars end their lives as giant explosions. What starts as a collapse of the stellar core is turned into an explosion driven by energy transfer of neutrinos. The neutrino densities become so high that coherent flavor conversions develop.
    I give an overview of the explosion mechanism and the importance of neutrinos. I will present a set of 76 simulations in axial symmetry initialized...

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  4. Karolin Hymon
    Neutrino Physics
    Invited Presentation

    We present POLARIS, a new sparse radial detector design for an underwater neutrino telescope. The design targets multi-PeV horizontal tracks with a minimal instrumentation density of around 1000 Digital Optical Modules. We evaluate the astronomy potential of this design through 5-sigma point source and diffuse flux detection limit, benchmarking against IceCube, KM3NeT ARCA, TRIDENT, NEON,...

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