1992/05/29 by Eugeni Akhmedov, Akhmedov, Eugeni
Physics and Astronomy · #FOS: Physical sciences #High Energy Physics - Phenomenology (hep-ph) #hep-ph
paper · pdf · doi:10.48550/arxiv.hep-ph/9205244
12 pages, 1 figure (not included), SISSA-49/92/EP
arxiv created 1992/05/29 · arxiv updated 2009/11/30
Recent developments of the resonant neutrino spin-flavor precession scenario and its applications to the solar neutrino problem are reviewed. We discuss in particular the possibilities of reconciliation of strong time variations of the solar neutrino flux observed in the Homestake 37$Cl experiment with little or no time variation seen in the Kamiokande II experiment.