The sun as a high energy neutrino source

Astronomy and Astrophysics – Astrophysics

Scientific paper

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8 pages, 3 figures, to be published in Astroparticle Physics

Scientific paper

10.1016/S0927-6505(99)00120-6

Cosmic ray interactions in the solar atmosphere yield a flux of electron and
muon neutrinos with energies greater than 10 GeV. We discuss the influence of
neutrino oscillations on the event rates in water-based Cerenkov detectors due
to this neutrino flux and comment on the possibility of detecting the sun as a
high energy neutrino source.

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