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arXiv · hep-ph/9809596

Models of Neutrino Masses from Oscillations with Maximal Mixing

Abstract

We discuss models of neutrino masses that lead to a large mixing angle for atmospheric neutrino oscillations. In particular we study a mechanism where a simple texture for the Dirac matrix leads to the observed pattern of mixings for a continuous range of Majorana matrices in a reasonably natural way. Both nearly maximal and small mixing solutions for solar neutrinos are compatible with this model. Possible dynamical realizations are discussed and a detailed example in terms of horizontal U(1) charges is presented.

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Guido Altarelli, Ferruccio Feruglio. 1998-10-16. Models of Neutrino Masses from Oscillations with Maximal Mixing. https://doi.org/10.1088/1126-6708%2F1998%2F11%2F021

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