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.
Keywords
Cite
@article{arxiv.2203.08096,
title = {High-Energy and Ultra-High-Energy Neutrinos},
author = {Markus Ackermann and Sanjib K. Agarwalla and Jaime Alvarez-Muñiz and Rafael Alves Batista and Carlos A. Argüelles and Mauricio Bustamante and Brian A. Clark and Austin Cummings and Sudipta Das and Valentin Decoene and Peter B. Denton and Damien Dornic and Zhan-Arys Dzhilkibaev and Yasaman Farzan and Alfonso Garcia and Maria Vittoria Garzelli and Christian Glaser and Aart Heijboer and Jörg R. Hörandel and Giulia Illuminati and Yu Seon Jeong and John L. Kelley and Kevin J. Kelly and Ali Kheirandish and Spencer R. Klein and John F. Krizmanic and Michael J. Larson and Lu Lu and Kohta Murase and Ashish Narang and Nepomuk Otte and Remy L. Prechelt and Steven Prohira and Mary Hall Reno and Elisa Resconi and Marcos Santander and Olga Vasil'evna Suvorova and Victor B. Valera and Justin Vandenbroucke and Lawrence Wiencke and Stephanie Wissel and Shigeru Yoshida and Tianlu Yuan and Enrique Zas and Pavel Zhelnin and Bei Zhou},
journal= {arXiv preprint arXiv:2203.08096},
year = {2022}
}
Comments
Contribution to Snowmass 2021, updated to include community feedback