Resonant spin-flavor precession of solar and supernova neutrinos

Details Resonant spin-flavor precession of solar and supernova neutrinos Resonant spin-flavor precession of solar and supernova neutrinos

Mar 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988phrvd..37.1368l&link_type=abstract

Physical Review D (Particles and Fields), Volume 37, Issue 6, 15 March 1988, pp.1368-1373

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Applications Of Electroweak Models To Specific Processes

Scientific paper

The combined effect of matter and magnetic fields on neutrino spin and flavor precession is examined. We find a potential new kind of resonant & or & (for Dirac neutrinos) or νe-->ν¯μ or ν¯τ (for Majorana neutrinos). Such a resonance could help account for the lower than expected solar-neutrino νe flux and/or indications of an anticorrelation between fluctuations in the νe flux and sunspot activity. Consequences of spin-flavor precession for supernova neutrinos are also briefly discussed.

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