Ultra High Energy Neutrinos from Supernova Remnants

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) $\gamma$ ray observation from SNRs is the main motivation behind this study.

6 pages, 3 figures, uses revtex

References in corpus (7)

• Discovery of TeV Gamma Rays from SN1006: Further Evidence for the SNR Origin of Cosmic Rays
• Gamma-ray production in supernova remnants
• Detection of Gamma Rays of Up to 50 TeV From the Crab Nebula
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Cited by in corpus (1)

• Probing maximum energy of cosmic rays in SNR through gamma rays and neutrinos from the molecular clouds around SNR W28