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Review Article
Open Access
High-Energy to Ultrahigh-Energy Neutrino Interactions
- Mary Hall Reno1
- Vol. 73:181-204 (Volume publication date September 2023) https://doi.org/10.1146/annurev-nucl-111422-040200
- First published as a Review in Advance on July 17, 2023
-
Copyright © 2023 by the author(s).This work is licensed under a Creative Commons Attribution 4.0 International License, which permits unrestricted use, distribution, and reproduction in any medium, provided the original author and source are credited. See credit lines of images or other third-party material in this article for license information
Abstract
The cross sections for neutrino interactions with nucleons have been measured directly in accelerator experiments and through the zenith-angle and energy dependence of neutrino events at the IceCube Neutrino Observatory. Fluxes of high-energy neutrinos are produced at the Large Hadron Collider and by cosmic rays in the atmosphere. High-energy neutrinos also come from astrophysical and cosmic sources. The theory of neutrino interactions is reviewed. Current cross-section measurements and prospects for the future are discussed. The focus here is on neutrino interactions for energies larger than 1 TeV.
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2023-09-25
2024-05-15
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/content/journals/10.1146/annurev-nucl-111422-040200
High-Energy to Ultrahigh-Energy Neutrino Interactions
Annual Review of Nuclear and Particle Science 73, 181 (2023); https://doi.org/10.1146/annurev-nucl-111422-040200
/content/journals/10.1146/annurev-nucl-111422-040200
/content/journals/10.1146/annurev-nucl-111422-040200
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