Dynamical Neutrino Mass Matrix: Large (Small) Mixing Solution to Atmospheric (Solar) Neutrino Oscillations
arXiv:hep-ph/9807386 · doi:10.1016/S0370-2693(98)01275-1
Abstract
In the wake of the SuperKamiokande announcement of atmospheric neutrino oscillations which favor the large mixing of with , there is considerable theoretical activity towards a possible understanding of the solar neutrino deficit also in terms of the mixing of with the other two neutrinos. A specific dynamical model is presented here for the first time which naturally chooses the large (small) mixing solution to atmospheric (solar) neutrino oscillations.
11 pages including 4 figures, Eq.(13) corrected, conclusions unchanged
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