Generation dependent Peccei Quinn symmetry and neutrino masses

Details Generation dependent Peccei Quinn symmetry and neutrino masses Generation dependent Peccei Quinn symmetry and neutrino masses

Sep 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988zphyc..38..479j&link_type=abstract

Zeitschrift für Physik C Particles and Fields, Volume 38, Issue 3, pp.479-482

Physics

4

Scientific paper

Possibility of relating three distinct physical phenomena—removal of strong CP violations, neutrino masses and fermion mixing—through a global U (1) symmetry is considered. Both the allowed range of neutrino masses and mixing angles could be tightly constrained in this scheme. A concrete model is proposed where the Fritzsch type of structure for quark mass matrices lead to a determination of neutrino mixing parameters. The resulting v e - v μ masses and mixing could solve the solar neutrino problem via Mikheyev-Smirnov-Wolfenstein mechanism. The v μ - v τ oscillations could occur in the model at an observable rate.

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