Class of models leading to depletions of solar νe and atmospheric νμ fluxes

Details Class of models leading to depletions of solar νe and atmospheric νμ fluxes Class of models leading to depletions of solar νe and atmospheric νμ fluxes

Feb 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992phrvd..45..725a&link_type=abstract

Physical Review D (Particles and Fields), Volume 45, Issue 3, 1 February 1992, pp.R725-R728

Physics

11

Quark And Lepton Masses And Mixing

Scientific paper

A model incorporating three left-handed SU(2)L×U(1)Y-doublet neutrinos and three right-handed singlet neutrinos, with leptonic Dirac mass submatrices similar to empirical forms which work well for quarks, is required to yield both the nonadiabatic Mikheyev-Smirnov-Wolfenstein solar neutrino effect and the depleted flux of atmospheric muon neutrinos observed by Kamiokande. We find a small segment of the δm223 vs sin22θ23 plane exists where such solutions can be achieved and identify the class or right-handed Majorana submatrices required.

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