High-energy and ultra-high-energy neutrinos: A Snowmass white paper

Publikation: Bidrag til tidsskriftTidsskriftartikelForskningfagfællebedømt

  • Markus Ackermann
  • Sanjib K. Agarwalla
  • Jaime Alvarez-Muniz
  • Rafael Alves Batista
  • Carlos A. Arguelles
  • 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
  • Jorg R. Horandel
  • 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
  • Justin Vandenbroucke
  • Olga Vasil'evna Suvorova
  • Lawrence Wiencke
  • Stephanie Wissel
  • Shigeru Yoshida
  • Tianlu Yuan
  • Enrique Zas
  • Pavel Zhelning
  • Bei Zhou

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 ultrahigh-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. (C) 2022 Elsevier B.V. All rights reserved.

OriginalsprogEngelsk
TidsskriftJournal of High Energy Astrophysics
Vol/bind36
Sider (fra-til)55-110
Antal sider56
ISSN2214-4048
DOI
StatusUdgivet - nov. 2022

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