SuperGZK neutrinos: testing physics beyond the Standard Model
高能物理 - 唯象学
2017-08-23 v1 天体物理学
摘要
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.
引用
@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}
}
备注
JD talk at XXI Texas Symposium (Florence)