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arXiv · hep-ph/9806540

The Solar Neutrino Puzzle: An Oscillation Solution with Maximal Neutrino Mixing

Anthony J. Baltz·Alfred Scharff Goldhaber·Maurice Goldhaber
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Abstract

If, as suggested by the SuperKamiokande results, the mu neutrino and tau neutrino are maximally and ``rapidly'' mixed, this alone determines the mapping from current to mass eigenstates up to one rotation angle (theta) mixing the electron neutrino ``more slowly'', with an equal combination of the mu neutrino and tau neutrino. For sin 2 theta = 1, the resulting minimal number of free parameters, yet maximal mixing, shows agreement between extant observations of solar neutrinos and predictions by the standard solar model with minor modifications.

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Anthony J. Baltz, Alfred Scharff Goldhaber, Maurice Goldhaber. 1998-06-30. The Solar Neutrino Puzzle: An Oscillation Solution with Maximal Neutrino Mixing. https://doi.org/10.1103/physrevlett.81.5730

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