arXiv · hep-ph/9806534
Interpreting the Atmospheric Neutrino Anomaly
Abstract
We suggest that the atmospheric neutrino anomaly observed in the Super-Kamiokande (and other) experiments results from the combined effects of muon-neutrino to tau-neutrino oscillations with a Delta m^2 value of approximately 0.4 eV^2 and oscillations between muon neutrinos and electron neutrinos (and vice-versa) with 0.0001 < Delta m^2 < 0.001 eV^2. With an appropriate choice of a three-neutrino mixing matrix, such a hypothesis is consistent with essentially all neutrino observations.
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R. P. Thun, S. McKee. 1998-08-05. Interpreting the Atmospheric Neutrino Anomaly. https://doi.org/10.1016/s0370-2693(98)01021-1
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