Ultra High Energy Neutrinos from Supernova Remnants
Abstract
Description
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) $γ$ ray observation from SNRs is the main motivation behind this study.
6 pages, 3 figures, uses revtex
6 pages, 3 figures, uses revtex