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Models of Neutrino Masses from Oscillations with Maximal Mixing

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.

preprint1998arXivOpen access
Guido AltarelliFerruccio Feruglio
hep-ph
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Guido AltarelliFerruccio Feruglio

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