Back to Search Start Over

High-Energy and Ultra-High-Energy Neutrinos

Authors :
Ackermann, Markus
Agarwalla, Sanjib K.
Alvarez-Muñiz, Jaime
Batista, Rafael Alves
Argüelles, Carlos A.
Bustamante, Mauricio
Clark, Brian A.
Cummings, Austin
Das, Sudipta
Decoene, Valentin
Denton, Peter B.
Dornic, Damien
Dzhilkibaev, Zhan-Arys
Farzan, Yasaman
Garcia, Alfonso
Garzelli, Maria Vittoria
Glaser, Christian
Heijboer, Aart
Hörandel, Jörg R.
Illuminati, Giulia
Jeong, Yu Seon
Kelley, John L.
Kelly, Kevin J.
Kheirandish, Ali
Klein, Spencer R.
Krizmanic, John F.
Larson, Michael J.
Lu, Lu
Murase, Kohta
Narang, Ashish
Otte, Nepomuk
Prechelt, Remy L.
Prohira, Steven
Reno, Mary Hall
Resconi, Elisa
Santander, Marcos
Suvorova, Olga Vasil'evna
Valera, Victor B.
Vandenbroucke, Justin
Wiencke, Lawrence
Wissel, Stephanie
Yoshida, Shigeru
Yuan, Tianlu
Zas, Enrique
Zhelnin, Pavel
Zhou, Bei
Publication Year :
2022

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.<br />Comment: Contribution to Snowmass 2021, updated to include community feedback

Details

Database :
arXiv
Publication Type :
Report
Accession number :
edsarx.2203.08096
Document Type :
Working Paper