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=1989zhetf..95..442a&link_type=abstract

Zhurnal Eksperimental'noi i Teoreticheskoi Fiziki (ISSN 0044-4510), vol. 95, Feb. 1989, p. 442-457. In Russian.

Physics

7

Flavor (Particle Physics), Precession, Solar Neutrinos, Spin Resonance, Dirac Equation, Electromagnetic Fields, Neutrino Beams, Particle Interactions, Solar Activity, Solar Magnetic Field

Scientific paper

The resonance amplification of spin-flavor precession of neutrinos in solar matter is considered. It is shown that resonant spin-flavor neutrino precession may account for the deficit of solar neutrinos in Davis' (1986, 1988) experiment and the observed anticorrelation between the rate of neutrino counting and solar activity. Experiments are considered which should make it possible to distinguish between spin-flavor neutrino precession and the Mikheyev-Smirnov-Wolfenstein effect.

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