SuperGZK neutrinos: testing physics beyond the Standard Model
High Energy Physics - Phenomenology
2017-08-23 v1 Astrophysics
Abstract
The sources and fluxes of superGZK neutrinos, eV, are discussed. The most promising sources are reionization bright phase, topological defects, superheavy dark matter and mirror matter. The energy of neutrinos can be above the GUT scale ( GeV). The predicted fluxes are observable by future space detectors EUSO and OWL.
Cite
@article{arxiv.hep-ph/0303091,
title = {SuperGZK neutrinos: testing physics beyond the Standard Model},
author = {Veniamin Berezinsky},
journal= {arXiv preprint arXiv:hep-ph/0303091},
year = {2017}
}
Comments
JD talk at XXI Texas Symposium (Florence)