Resonant Spin-Flavor Precession of Neutrinos As a Possible Solution to the Solar Neutrino Problem

Details Resonant Spin-Flavor Precession of Neutrinos As a Possible Solution to the Solar Neutrino Problem Resonant Spin-Flavor Precession of Neutrinos As a Possible Solution to the Solar Neutrino Problem

1992-05-29

arxiv.org/abs/hep-ph/9205244v1

Physics

High Energy Physics

High Energy Physics - Phenomenology

12 pages, 1 figure (not included), SISSA-49/92/EP

Scientific paper

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.

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