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arXiv · astro-ph/9910208

The sun as a high energy neutrino source

Christian Hettlage·Karl Mannheim·John G. Learned
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Abstract

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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Christian Hettlage, Karl Mannheim, John G. Learned. 1999-10-12. The sun as a high energy neutrino source. https://doi.org/10.1016/s0927-6505(99)00120-6

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