Three neutrino flavors: Oscillations, mixing, and the solar-neutrino problem

Details Three neutrino flavors: Oscillations, mixing, and the solar-neutrino problem Three neutrino flavors: Oscillations, mixing, and the solar-neutrino problem

Feb 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991phrvd..43..641p&link_type=abstract

Physical Review D (Particles and Fields), Volume 43, Issue 3, 1 February 1991, pp.R641-R645

Mathematics

Probability

10

Quark And Lepton Masses And Mixing

Scientific paper

An analytical, quantitative description of solar-neutrino propagation is presented which includes three flavors, matter dependence, and long-wavelength effects. Using the derived expression for the electron-neutrino survival probability, it is demonstrated that mixing is possible between the two-flavor Mikheyev-Smirnov-Wolfenstein and two-flavor long-wavelength solutions to the solar-neutrino problem. However, adiabatic conversion of a neutrino mass eigenstate tends to suppress all subsequent long-wavelength effects such as ``seasonal'' variations in the solar-neutrino flux.

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