Neutrino Astronomy: Physics Goals, Detector Parameters

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dc.creatorGaisser, T. K.
dc.date1997-07-25
dc.date.accessioned2026-07-07T02:23:53Z
dc.date.available2026-07-07T02:23:53Z
dc.descriptionThis is a review of high energy neutrino astronomy that might be done with a kilometer-scale detector. The emphasis is on diffuse neutrinos of extragalactic origin and their relation to possible sources of the highest energy cosmic rays, such as active galaxies, cosmological gamma-ray burst sources and topological defects.
dc.description10 pages, LaTeX plus 9 postscript figures. (Talk given at the OECD Megascience Forum Workshop, Taormina, Sicily, 22/23 May, 1997.)
dc.identifierhttps://arxiv.org/abs/astro-ph/9707283
dc.identifierhttp://arxiv.org/abs/astro-ph/9707283
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/11424
dc.subjectAstrophysics
dc.titleNeutrino Astronomy: Physics Goals, Detector Parameters
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