Possible solution to the discrepancy between the Homestake and KAMIOKANDE solar-neutrino experiments

Details Possible solution to the discrepancy between the Homestake and KAMIOKANDE solar-neutrino experiments Possible solution to the discrepancy between the Homestake and KAMIOKANDE solar-neutrino experiments

Oct 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990phrvl..65.1975f&link_type=abstract

Physical Review Letters (ISSN 0031-9007), vol. 65, Oct. 15, 1990, p. 1975-1978.

Physics

14

Magnetic Moments, Particle Interactions, Solar Activity Effects, Solar Neutrinos, Leptons, Stellar Evolution

Scientific paper

A possible particle-physics solution is proposed to the recently reported discrepancy between the Homestake and Kamiokande II experiments concerning the time variation of the solar-neutrino flux. It is pointed out that some of the models giving rise to a large magnetic moment of electron neutrinos include the possibility that the right-handed neutrino interacts with electrons strongly enough so that Kamiokande does not see the time variation, while the Homestake experiment shows the time variation in anticorrelation with solar activity due to the neutrino helicity flip in the sun.

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