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arXiv:hep-ph/9911275·v2·High Energy Physics — Phenomenology

Fermion Masses and Neutrino Oscillations in SO(10) SUSY GUT with D_3 x U(1) Family Symmetry

R. Dermisek🇺🇸 · S. Raby (The Ohio State University)🇺🇸

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Abstract

Discrete nonabelian gauge symmetries appear to be the most advantageous candidates for a family symmetry. We present a predictive SO(10) SUSY GUT model with family symmetry (D_3 is the dihedral group of order 6). The hierarchy in fermion masses is generated by the family symmetry breaking nothing. This model fits the low energy data in the charged fermion sector quite well and naturally provides large angle - mixing describing atmospheric neutrino oscillation data and small angle - mixing consistent with the small mixing angle MSW solution to the solar neutrino data. In addition, the non-abelian family symmetry D_3 is sufficient to suppress large flavor violations.

Comments: 24 pages, 2 figures, added a footnote and an acknowledgement

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