Models of Neutrino Masses from Oscillations with Maximal Mixing

Details Models of Neutrino Masses from Oscillations with Maximal Mixing Models of Neutrino Masses from Oscillations with Maximal Mixing

1998-09-30

arxiv.org/abs/hep-ph/9809596v2

JHEP 9811:021,1998

Physics

High Energy Physics

High Energy Physics - Phenomenology

10 pages, LATEX, no figures; references added; minor changes to clarify the U(1) example

Scientific paper

10.1088/1126-6708/1998/11/021

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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