Ultrahigh Energy Neutrinos
High Energy Physics - Phenomenology
2016-12-21 v1
Abstract
The ultrahigh energy neutrino cross section is well understood in the standard model for neutrino energies up to 10 GeV. Test of neutrino oscillations () from extragalactic sources of neutrinos are possible with large underground detectors. Measurments of horizontal air shower event rates at neutrino energies above 10 GeV will be able to constrain nonstandard model contributions to the neutrino-nucleon cross section, e.g., from mini-black hole production.
Keywords
Cite
@article{arxiv.hep-ph/0302178,
title = {Ultrahigh Energy Neutrinos},
author = {Sharada Iyer Dutta and Mary Hall Reno and Ina Sarcevic},
journal= {arXiv preprint arXiv:hep-ph/0302178},
year = {2016}
}
Comments
7 pages, presented at Neutrinos and Implications for Physics Beyond the Standard Model, Stony Brook, NY, October 11-13, 2002