English

SO(3) Gauge model for neutrino masses and oscillations

High Energy Physics - Phenomenology 2009-10-31 v1

Abstract

I mainly describe neutrino masses and oscillations in the gauge model with SO(3)FSO(3)_{F} lepton flavor symmetry and with two Higgs triplets. It is shown how the maximal mixing between νμ\nu_{\mu} and ντ\nu_{\tau} 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 νe\nu_{e} and νμ\nu_{\mu} 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 SO(3)FSO(3)_{F} gauge interactions.

Keywords

Cite

@article{arxiv.hep-ph/9908436,
  title  = {SO(3) Gauge model for neutrino masses and oscillations},
  author = {Yue-Liang Wu},
  journal= {arXiv preprint arXiv:hep-ph/9908436},
  year   = {2009}
}

Comments

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.)