The sun as a high energy neutrino source
classification
🌌 astro-ph
hep-ph
keywords
neutrinoenergyfluxhighsourceatmospherecerenkovcomment
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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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