Best-Bet Astrophysical Neutrino Sources

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dc.creatorDermer, Charles D.
dc.date2006-11-06
dc.date.accessioned2026-07-07T10:24:11Z
dc.date.available2026-07-07T10:24:11Z
dc.descriptionLikely astrophysical sources of detectable high-energy (>> TeV) neutrinos are considered. Based on gamma-ray emission properties, the most probable sources of neutrinos are argued to be GRBs, blazars, microquasars, and supernova remnants. Diffuse neutrino sources are also briefly considered.
dc.description6 pages, 2 figures, in Proc. of TeV-Particle Astrophysics II, Madison, WI, 28-31 Aug, 2006
dc.identifierhttps://arxiv.org/abs/astro-ph/0611191
dc.identifierhttp://arxiv.org/abs/astro-ph/0611191
dc.identifierJ.Phys.Conf.Ser.60:8-13,2007
dc.identifierdoi:10.1088/1742-6596/60/1/002
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/176096
dc.subjectAstrophysics
dc.titleBest-Bet Astrophysical Neutrino Sources
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