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arXiv · hep-ph/9807319

Generalized Neutrino Mixing from the Atmospheric Anomaly

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

We determine the neutrino mixing and mass parameters that are allowed by the Super-Kamiokande atmospheric neutrino data in a three-neutrino model with one mass-squared difference contributing to the oscillations. We find that although $ν_μ\toν_τ$ oscillations are favored, $ν_μ\to ν_e$ oscillations with amplitude as large as 0.18 are allowed even after accounting for the limit from the CHOOZ reactor experiment. The range of allowed parameters permit observable $ν_μ\leftrightarrowν_e$ and $ν_e\toν_τ$ oscillations in future long-baseline experiments.

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V. Barger, T. J. Weiler, K. Whisnant. 1998-07-09. Generalized Neutrino Mixing from the Atmospheric Anomaly. https://doi.org/10.1016/s0370-2693(98)01143-5

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