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arXiv · hep-ph/9712495

Four-Way Neutrino Oscillations

V. Barger·T. J. Weiler·K. Whisnant
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Abstract

We present a four-neutrino model with three active neutrinos and one sterile neutrino which naturally has maximal $ν_μ\toν_τ$ oscillations of atmospheric neutrinos and can explain the solar neutrino and LSND results. The model predicts $ν_e \to ν_τ$ and $ν_e \to ν_μ$ oscillations in long-baseline experiments with $L/E \gg 1$ km/GeV with amplitudes that are determined by the LSND oscillation amplitude and argument controlled by the atmospheric $δm^2$.

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V. Barger, T. J. Weiler, K. Whisnant. 1997-12-22. Four-Way Neutrino Oscillations. https://doi.org/10.1016/s0370-2693(98)00325-6

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