English

Ultra High Energy Neutrinos from Supernova Remnants

Astrophysics 2008-11-26 v1

Abstract

In this paper we discuss possible ultra high energy (\ge TeV) neutrino emission from Supernova Remnants (SNRs), specifically the hadronic gamma ray production models. Recent very high energy (VHE) γ\gamma ray observation from SNRs is the main motivation behind this study.

Keywords

Cite

@article{arxiv.astro-ph/9901215,
  title  = {Ultra High Energy Neutrinos from Supernova Remnants},
  author = {Mou Roy},
  journal= {arXiv preprint arXiv:astro-ph/9901215},
  year   = {2008}
}

Comments

6 pages, 3 figures, uses revtex