Neutrinos from galactic sources of cosmic rays with known gamma-ray spectra

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dc.creatorVissani, Francesco
dc.date2006-07-12
dc.date.accessioned2026-07-07T10:39:34Z
dc.date.available2026-07-07T10:39:34Z
dc.descriptionWe describe a simple procedure to estimate the high-energy neutrino flux from the observed gamma-ray spectra of galactic cosmic ray sources that are transparent to their gamma radiation. We evaluate in this way the neutrino flux from the supernova remnant RX J1713.7-3946, whose very high-energy gamma-ray spectrum (assumed to be of hadronic origin) is not a power law distribution according to H.E.S.S. observations. The corresponding muon signal in neutrino telescopes is found to be about 5 events per square kilometer per year in an ideal detector.
dc.description6 pages, 1 figure; accepted in Astroparticle Physics
dc.identifierhttps://arxiv.org/abs/astro-ph/0607249
dc.identifierhttp://arxiv.org/abs/astro-ph/0607249
dc.identifierAstropart.Phys.26:310-313,2006
dc.identifierdoi:10.1016/j.astropartphys.2006.07.005
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/181071
dc.subjectAstrophysics
dc.titleNeutrinos from galactic sources of cosmic rays with known gamma-ray spectra
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