Dynamical Neutrino Mass Matrix: Large (Small) Mixing Solution to Atmospheric (Solar) Neutrino Oscillations
Abstract
In the wake of the SuperKamiokande announcement of atmospheric neutrino oscillations which favor the large mixing of μ with τ, there is considerable theoretical activity towards a possible understanding of the solar neutrino deficit also in terms of the mixing of e 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.
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