Ultra High Energy Neutrinos from Supernova Remnants

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dc.creatorRoy, Mou
dc.date1999-01-15
dc.date.accessioned2026-07-07T10:51:24Z
dc.date.available2026-07-07T10:51:24Z
dc.descriptionIn 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.
dc.description6 pages, 3 figures, uses revtex
dc.identifierhttps://arxiv.org/abs/astro-ph/9901215
dc.identifierhttp://arxiv.org/abs/astro-ph/9901215
dc.identifierJ.Phys.G25:129-134,1999
dc.identifierdoi:10.1088/0954-3899/25/1/011
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/184807
dc.subjectAstrophysics
dc.titleUltra High Energy Neutrinos from Supernova Remnants
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