Large neutrino mixing and normal mass hierarchy: a discrete understanding

preprint2004arXivOpen access

Abstract

We discuss the possibility of flavor symmetries to explain the pattern of charged lepton and neutrino masses and mixing angles. We emphasize what are the obstacles for the generation of an almost maximal atmospheric mixing and what are the minimal ingredients to obtain it. A model based on the discrete symmetry S3S_3 is constructed, which leads to the dominant μτμτ-block in the neutrino mass matrix, thus predicting normal hierarchy. This symmetry makes it possible to reproduce current data and predicts 0.01≲θ13≲0.030.01\lesssimθ_{13}\lesssim 0.03 and strongly suppressed neutrinoless 2β2β-decay. Moreover, it implies a relation between lepton and quark mixing angles: θ23q≈2(π/4−θ23)θ_{23}^q \approx 2(π/4-θ_{23}). The Cabibbo mixing can also be reproduced and θ13q∼θ12qθ23qθ_{13}^q\sim θ_{12}^qθ_{23}^q. S3S_3 is thus a candidate to describe all the basic features of Standard Model fermion masses and mixing.

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