arXiv · hep-ph/9711421
Zenith distribution of atmospheric neutrino events and electron neutrino mixing
Abstract
Assuming atmospheric neutrino oscillations with dominant nu_mu<--->nu_tau transitions, we discuss how subdominant nu_e mixing (within the Chooz reactor bounds) can alter the zenith distributions of neutrino-induced electrons and muons. We isolate two peculiar distortion effects, one mainly related to nu_e mixing in vacuum and the other to matter oscillations, that may be sufficiently large to be detected by the SuperKamiokande atmospheric nu experiment. These effects (absent for pure two-flavor nu_mu<--->nu_tau transitions) do not vanish in the limit of energy-averaged oscillations.
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G. L. Fogli, E. Lisi, A. Marrone, D. Montanino. 1997-11-21. Zenith distribution of atmospheric neutrino events and electron neutrino mixing. https://doi.org/10.1016/s0370-2693(98)00077-x
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