MHD solar fluctuations and solar neutrinos

We analyze how solar neutrino experiments could detect time fluctuations of the solar neutrino flux due to magnetohydrodynamic (MHD) perturbations of the solar plasma. We state that if such time fluctuations are detected, this would provide a unique signature of the Resonant Spin-Flavor Precession (...

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Bibliographic Details
Published inBrazilian journal of physics Vol. 33; no. 4; pp. 707 - 774
Main Authors Reggiani, N., Guzzo, M.M., Holanda, P.C. de
Format Journal Article
LanguageEnglish
Published Sociedade Brasileira de Física 01.12.2003
Subjects
PHYSICS, MULTIDISCIPLINARY
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Summary:We analyze how solar neutrino experiments could detect time fluctuations of the solar neutrino flux due to magnetohydrodynamic (MHD) perturbations of the solar plasma. We state that if such time fluctuations are detected, this would provide a unique signature of the Resonant Spin-Flavor Precession (RSFP) mechanism as a solution to the Solar Neutrino Problem.
ISSN:0103-9733
1678-4448
DOI:10.1590/S0103-97332003000400028