Hybrid solution of the solar neutrino problem in anticorrelation with sunspot activity

Details Hybrid solution of the solar neutrino problem in anticorrelation with sunspot activity Hybrid solution of the solar neutrino problem in anticorrelation with sunspot activity

Jul 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989phrvl..63..121m&link_type=abstract

Physical Review Letters (ISSN 0031-9007), vol. 63, July 10, 1989, p. 121-124.

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50

Computational Astrophysics, Solar Activity Effects, Solar Neutrinos, Sunspots, Convection Currents, Magnetic Flux, Particle Spin, Solar Magnetic Field, Stellar Models

Scientific paper

A mechanism for a new type of solution to the solar neutrino problem is proposed which provides a natural explanation for the observation that the solar neutrino flux is apparently in anticorrelation with the sunspot number. The mechanism is found to require the simultaneous presence of neutrino flavor mixing and a magnetic (or transition) moment as large as muB of about 10 to the -10th, where mu is in units of the Bohr magneton and B is in kG. The present mechanism results in an about 20 percent deficit in the net neutrino flux. It is pointed out that for low-energy pp-chain neutrinos, the spin rotation does not play an important role.

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