MHD solar fluctuations and solar neutrinos

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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Veröffentlicht in:Brazilian journal of physics 2003-12, Vol.33 (4), p.707-774
Hauptverfasser: Reggiani, N., Guzzo, M.M., Holanda, P.C. de
Format: Artikel
Sprache:eng
Schlagworte:
PHYSICS, MULTIDISCIPLINARY
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Zusammenfassung: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