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

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

1998-06-30

arxiv.org/abs/hep-ph/9806540v1

Phys.Rev.Lett. 81 (1998) 5730-5733

Physics

High Energy Physics

High Energy Physics - Phenomenology

10 pages, latex, revtex source, two postscript figures

Scientific paper

10.1103/PhysRevLett.81.5730

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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