Dynamical Neutrino Mass Matrix: Large (Small) Mixing Solution to Atmospheric (Solar) Neutrino Oscillations

Details Dynamical Neutrino Mass Matrix: Large (Small) Mixing Solution to Atmospheric (Solar) Neutrino Oscillations Dynamical Neutrino Mass Matrix: Large (Small) Mixing Solution to Atmospheric (Solar) Neutrino Oscillations

1998-07-15

arxiv.org/abs/hep-ph/9807386v2

Phys.Lett. B442 (1998) 238-242

Physics

High Energy Physics

High Energy Physics - Phenomenology

11 pages including 4 figures, Eq.(13) corrected, conclusions unchanged

Scientific paper

10.1016/S0370-2693(98)01275-1

In the wake of the SuperKamiokande announcement of atmospheric neutrino oscillations which favor the large mixing of $\nu_\mu$ with $\nu_\tau$, there is considerable theoretical activity towards a possible understanding of the solar neutrino deficit also in terms of the mixing of $\nu_e$ 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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