SO(3) Gauge model for neutrino masses and oscillations
arXiv:hep-ph/9908436 · doi:10.1016/S0920-5632(00)00506-5
Abstract
I mainly describe neutrino masses and oscillations in the gauge model with lepton flavor symmetry and with two Higgs triplets. It is shown how the maximal mixing between and neutrinos comes out naturally after spontaneous breaking of the symmetry. The nearly two-flavor mixing scenario is resulted naturally from an approximate permutation symmetry between the two Higgs triplets. The hierarchy between the neutrino mass-squared differences, which is needed for reconciling both solar and atmospheric neutrino data, leads to an almost maximal mixing between and neutrinos. Thus the model favors the intriguing bi-maximal mixing scenario.The three Majorana neutrino masses are allowed to be nearly degenerate and large enough to play a significant cosmological role. The model can also lead to interesting phenomena on lepton-flavor violations via the gauge interactions.
latex, no figures, invited talk at the Sixth Topical Seminar on Neutrino and Astroparticle Physics, San Miniato, Italy, May 1999, to appear in Nucl. Phys. B (Proc. Suppl.)
References in corpus (5)
- Bi-Maximal Mixing of Three Neutrinos
- Constraints on neutrino oscillation parameters from the measurement of day-night solar neutrino fluxes at Super-Kamiokande
- Measurement of the solar neutrino energy spectrum using neutrino-electron scattering
- Do hep neutrinos affect the solar neutrino energy spectrum?
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Cited by in corpus (5)
- SU(3) Gauge Family Symmetry and Prediction for the Lepton-Flavor Mixing and Neutrino Masses with Maximal Spontaneous CP Violation
- Gauge Theory Model of the Neutrino and New Physics Beyond the Standard Model
- Leptonic CP Violation and Wolfenstein Parametrization for Lepton Mixing
- SO(3) Gauge Symmetry and Nearly Tri-bimaximal Neutrino Mixing
- The Mass Difference of with SO(3) Family Gauge Symmetry