8–10 Oct 2025
Nevis Labs, Columbia University
America/New_York timezone

Session

Neutrinos

9 Oct 2025, 15:30
Nevis Labs, Columbia University

Nevis Labs, Columbia University

Presentation materials

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  1. Shuo Zhang (Michigan State University)
    09/10/2025, 15:30

    TeV emission from the Galactic center strongly suggests the existence of a hadronic Pevatron located within ~10 pc of Sgr A*. If there is indeed a PeV proton/ion source and abundant molecular clouds in the surrounding, we expect several different observable effects such as multi-TeV neutrino, gamma-ray photons and electrons. In this presentation, I will discuss our efforts finding traces of...

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  2. Ke Fang
    09/10/2025, 16:00

    Dozens of ultrahigh-energy gamma-ray sources have been detected to date. However, it remains largely unknown which of these sources accelerate hadronic cosmic rays and thus contribute to the mysterious cosmic-ray knee. High-energy neutrinos offer a unique and unambiguous probe of hadronic PeVatrons, as they are most likely produced through interactions of hadronic cosmic rays. In this talk, I...

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  3. Silvia Celli
    09/10/2025, 16:30

    Neutrino astronomy is starting to unveil new features of the extreme non-thermal Universe, thanks to the operation of several large volume Cherenkov neutrino telescopes, as IceCube, Baikal-GVD, and KM3NeT. These instruments benefit of extended and complementary fields of view, coupled to high duty cycle and sub-degree angular resolution, allowing the study of cosmic neutrinos and their...

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