Simultaneous solutions to the solar and atmospheric neutrino problems via Fritzsch-type lepton mass matrices

Details Simultaneous solutions to the solar and atmospheric neutrino problems via Fritzsch-type lepton mass matrices Simultaneous solutions to the solar and atmospheric neutrino problems via Fritzsch-type lepton mass matrices

Oct 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992phrvd..46.3208d&link_type=abstract

Physical Review D (Particles and Fields), Volume 46, Issue 7, 1 October 1992, pp.3208-3210

Physics

6

Quark And Lepton Masses And Mixing

Scientific paper

We present a simultaneous solution for the solar and atmospheric neutrino problems by constructing a left-right-symmetric model which yields Fritzsch-type leptonic mass matrices. Requiring the two neutrino problems to be solved simultaneously fixes the parameters of the model and leads to a prediction of an expected observation of solar neutrinos at the level of 50 to 120 solar neutrino units in the 71Ga detectors in the GALLEX and SAGE experiments. Our predictions are consistent with results from both experiments, particularly the measured flux and the allowed mixing parameter values recently reported from GALLEX.

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