Resonant spin-flavor precession of neutrinos and the solar neutrino problem.

Details Resonant spin-flavor precession of neutrinos and the solar neutrino problem. Resonant spin-flavor precession of neutrinos and the solar neutrino problem.

Feb 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989jetp...68..250a&link_type=abstract

Sov. Phys. - JETP, Vol. 68, No. 2, p. 250 - 257

Physics

9

Solar Neutrinos, Solar Neutrinos: Solar Activity

Scientific paper

The resonant amplification of spin-flavor precession of neutrinos in solar matter and possible consequences of this phenomenon are discussed. It is shown that resonant spin-flavor neutrino precession may account for the deficit in solar neutrinos in the Davis experiment and for the anticorrelation between the neutrino count rate and solar activity. Experiments that could distinguish between spin-flavor neutrino precession and the Mikheev-Smirnov-Wolfenstein effect are examined. A new limit on the usual spin precession of solar neutrinos is derived.

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