Ultra-high energy cosmic neutrinos
High Energy Physics - Phenomenology
2017-08-23 v1 Astrophysics
Abstract
Several cosmologically distant astrophysical sources may produce ultra-high energy cosmic neutrinos (E > 10^6 GeV) of all flavors above the atmospheric neutrino background. I study the effects of vacuum neutrino flavor mixing on this cosmic neutrino flux. Prospects for observations of these ultra-high energy cosmic neutrinos in large underwater/ice neutrino telescopes are also briefly discussed.
Keywords
Cite
@article{arxiv.hep-ph/0008121,
title = {Ultra-high energy cosmic neutrinos},
author = {H. Athar},
journal= {arXiv preprint arXiv:hep-ph/0008121},
year = {2017}
}
Comments
3 pages, latex, talk given at the 8th Asia Pacific Physics Conference (APPC2000), 7-10 August, 2000, Taipei, Taiwan (to appear in its proceedings)