arXiv · 2203.08096
High-Energy and Ultra-High-Energy Neutrinos
Abstract
Astrophysical neutrinos are excellent probes of astroparticle physics and high-energy physics. With energies far beyond solar, supernovae, atmospheric, and accelerator neutrinos, high-energy and ultra-high-energy neutrinos probe fundamental physics from the TeV scale to the EeV scale and beyond. They are sensitive to physics both within and beyond the Standard Model through their production mechanisms and in their propagation over cosmological distances. They carry unique information about their extreme non-thermal sources by giving insight into regions that are opaque to electromagnetic radiation. This white paper describes the opportunities astrophysical neutrino observations offer for astrophysics and high-energy physics, today and in coming years.
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Markus Ackermann, Sanjib K. Agarwalla, Jaime Alvarez-Muñiz, Rafael Alves Batista, Carlos A. Argüelles, Mauricio Bustamante, Brian A. Clark, Austin Cummings, Sudipta Das, Valentin Decoene, Peter B. Denton, Damien Dornic, Zhan-Arys Dzhilkibaev, Yasaman Farzan, Alfonso Garcia, Maria Vittoria Garzelli, Christian Glaser, Aart Heijboer, Jörg R. Hörandel, Giulia Illuminati, Yu Seon Jeong, John L. Kelley, Kevin J. Kelly, Ali Kheirandish, Spencer R. Klein, John F. Krizmanic, Michael J. Larson, Lu Lu, Kohta Murase, Ashish Narang, Nepomuk Otte, Remy L. Prechelt, Steven Prohira, Mary Hall Reno, Elisa Resconi, Marcos Santander, Olga Vasil'evna Suvorova, Victor B. Valera, Justin Vandenbroucke, Lawrence Wiencke, Stephanie Wissel, Shigeru Yoshida, Tianlu Yuan, Enrique Zas, Pavel Zhelnin, Bei Zhou. 2022-03-15. High-Energy and Ultra-High-Energy Neutrinos. https://arxiv.org/abs/2203.08096
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