On the origin of neutrino flavour symmetry
Abstract
We study classes of models which are based on some discrete family symmetry which is completely broken such that the observed neutrino flavour symmetry emerges indirectly as an accidental symmetry. For such "indirect" models we discuss the D-term flavon vacuum alignments which are required for such an accidental flavour symmetry consistent with tri-bimaximal lepton mixing to emerge. We identify large classes of suitable discrete family symmetries, namely the and groups, together with other examples such as . In such indirect models the implementation of the type I see-saw mechanism is straightforward using constrained sequential dominance. However the accidental neutrino flavour symmetry may be easily violated, for example leading to a large reactor angle, while maintaining accurately the tri-bimaximal solar and atmospheric predictions.
Keywords
Cite
@article{arxiv.0908.1897,
title = {On the origin of neutrino flavour symmetry},
author = {Stephen F. King and Christoph Luhn},
journal= {arXiv preprint arXiv:0908.1897},
year = {2009}
}
Comments
24 pages; version to be published in JHEP