Adiabatic resonant oscillations of solar neutrinos in three generations

Details Adiabatic resonant oscillations of solar neutrinos in three generations Adiabatic resonant oscillations of solar neutrinos in three generations

Feb 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987phrvd..35.1404k&link_type=abstract

Physical Review D (Particles and Fields), Volume 35, Issue 4, 15 February 1987, pp.1404-1408

Physics

33

Quark And Lepton Masses And Mixing

Scientific paper

The Mikheyev-Smirnov-Wolfenstein model of resonant solar-neutrino oscillations is discussed for three generations of leptons. Assuming adiabatic transitions, bounds for the μ- and e-neutrinos mass-squared difference Δ21,0 are obtained as a function of the e-μ mixing angle theta1. The allowed region in the Δ21,0-theta1 plot that would solve the solar-neutrino problem is shown to be substantially larger than that of the two-generation case. In particular, the difference between the two- and three-generation cases becomes significant for theta1 larger than ~20°.

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