High energy astrophysical neutrinos

Details High energy astrophysical neutrinos High energy astrophysical neutrinos

2002-09-12

arxiv.org/abs/hep-ph/0209130v1

Physics

High Energy Physics

High Energy Physics - Phenomenology

4 pages, 1 figure, talk given at IAU 8th Asian Pacific Regional Meeting, 2-5 July, 2002, Tokyo, Japan (to appear in its procee

Scientific paper

High energy neutrinos with energy typically greater than tens of thousands of GeV may originate from several astrophysical sources. The sources may include, for instance, our galaxy, the active centers of nearby galaxies, as well as possibly the distant sites of gamma ray bursts. I briefly review some aspects of production and propagation as well as prospects for observations of these high energy astrophysical neutrinos.

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