-
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...
Go to contribution page -
Ke Fang09/10/2025, 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...
Go to contribution page -
Silvia Celli09/10/2025, 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...
Go to contribution page -
Choose timezone
Your profile timezone: