Fermion Mixings in SU(9) Family Unification

Details Fermion Mixings in SU(9) Family Unification Fermion Mixings in SU(9) Family Unification

2009-04-20

arxiv.org/abs/0904.3084v3

Phys.Lett.B681:343-346,2009

Physics

High Energy Physics

High Energy Physics - Phenomenology

Explanation of mixing angles

Scientific paper

10.1016/j.physletb.2009.10.031

In an SU(9) model of gauged family unification, we propose an explanation for why angles observed in the lepton flavor ({\it PMNS}) mixing matrix are significantly larger than those measured for any analagous quark flavor ({\it KM}) mixing angle. It is directly related to a see-saw mechanism that we assume to be responsible for the generation of neutrino masses. Our model is more constrained and therefore even more predictive than a model previously proposed by Barr.

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