Particle-physics model for the Voloshin-Vysotski-Okun solution to the solar-neutrino problem

Details Particle-physics model for the Voloshin-Vysotski-Okun solution to the solar-neutrino problem Particle-physics model for the Voloshin-Vysotski-Okun solution to the solar-neutrino problem

May 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987phrvl..58.1807f&link_type=abstract

Physical Review Letters (ISSN 0031-9007), vol. 58, May 4, 1987, p. 1807-1809.

Mathematics

Logic

104

Solar Neutrinos, Stellar Models, Magnetic Moments, Particle Theory

Scientific paper

A particle-physics model is presented for the large magnetic moment of the electron neutrino required to explain the anticorrelation between the solar neutrino flux and the sunspot number. The model is shown to be consistent with cosmological constraints as well as with existing laboratory experiments. Possible experimental tests of the model are discussed.

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