Time variation of the solar-neutrino flux and the resonant spin-flavor rotation mechanism

Details Time variation of the solar-neutrino flux and the resonant spin-flavor rotation mechanism Time variation of the solar-neutrino flux and the resonant spin-flavor rotation mechanism

Jan 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991phrvd..43..297m&link_type=abstract

Physical Review D (Particles and Fields), Volume 43, Issue 2, 15 January 1991, pp.297-300

Physics

5

Scientific paper

The recent observation at the 37Cl experiment suggests that the (anti)correlation between the solar-neutrino flux and the sunspot activity seems to be real. We analyze the characteristic features of the time variation of the solar-neutrino flux in terms of the resonant spin-flavor rotation mechanism. Implications for the ongoing Kamiokande II experiment are discussed.

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