High energy astrophysical processes

dc.creatorStanev, Todor
dc.date2005-04-18
dc.date.accessioned2026-07-07T02:17:29Z
dc.date.available2026-07-07T02:17:29Z
dc.descriptionWe briefly review the high energy astrophysical processes that are related to the production of high energy $γ$-ray and neutrino signals and are likely to be important for the energy loss of high and ultrahigh energy cosmic rays. We also give examples for neutrino fluxes generated by different astrophysical objects and describe the cosmological link provided by cosmogenic neutrinos.
dc.description16 pages, 10 postscript figures, to appear in Proceedings of the Venice 2005 Workshop on neutrino telescopes
dc.identifierhttps://arxiv.org/abs/astro-ph/0504401
dc.identifierhttp://arxiv.org/abs/astro-ph/0504401
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/9189
dc.subjectAstrophysics
dc.titleHigh energy astrophysical processes
dc.typetext

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