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Atmospheric neutrino tests of neutrino oscillation mechanisms

โœ Scribed by R Foot; C.N Leung; O Yasuda


Book ID
108440024
Publisher
Elsevier Science
Year
1998
Tongue
English
Weight
128 KB
Volume
443
Category
Article
ISSN
0370-2693

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The Sun is a source of high energy neutrinos (E > 10 GeV) produced by cosmic ray interactions in the solar atmosphere. We study the impact of three-flavor oscillations on the solar atmosphere neutrino fluxes observable at Earth. We find that peculiar matter oscillation effects in the Sun do exist, b