Family replicated gauge groups and large mixing angle solar neutrino solution

Details Family replicated gauge groups and large mixing angle solar neutrino solution Family replicated gauge groups and large mixing angle solar neutrino solution

2002-01-17

arxiv.org/abs/hep-ph/0201152v3

Nucl.Phys. B631 (2002) 285-306

Physics

High Energy Physics

High Energy Physics - Phenomenology

24 pages, 4 figures, Latex2e using Feynmf (included); ref. added, typos corrected; to appear in Nuclear Physics B

Scientific paper

10.1016/S0550-3213(02)00212-2

We present a modification of our previous family replicated gauge group model, which now generates the Large Mixing Angle MSW solution rather than the experimentally disfavoured Small Mixing Angle MSW solution to the solar neutrino oscillation problem. The model is based on each family of quarks and leptons having its own set of gauge fields, each containing a replica of the Standard Model gauge fields plus a (B-L)-coupled gauge field. By a careful choice of the Higgs field gauge quantum numbers, we avoid our previous prediction that the solar neutrino mixing angle is equal order of magnitudewise to the Cabibbo angle, replacing it and the well-known Fritzsch relation with the relation \theta_{c}\sim (\theta_{\odot})^{-1/3} (m_d/m_s)^{2/3}. At the same time we retain a phenomenologically successful structure for the charged quark and lepton mass matrices. A fit of all the seventeen quark-lepton mass and mixing angle observables, using just six new Higgs field vacuum expectation values, agrees with the experimental data within the theoretically expected uncertainty of about 64%, i.e. it fits perfectly order of magnitudewise.

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