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Solar MHD Waves and Solar Neutrinos
Authors:Reggiani  N  Guzzo  MM  de Holanda  PC
Institution:(1) Faculdade de Matemática, Centro de Ciências Exatas Ambientais e de Tecnologias, Pontifí cia, Universidade Católica de Campinas, 13086-900 Campinas-SP, Brazil;(2) Instituto de Fí sica Gleb Wataghin, Universidade Estadual de Campinas, Brazil;(3) The Abdus Salam International Centre for Theoretical Physics, I-34100 Trieste, Italy
Abstract:We analyze here how solar neutrino experiments could detect time fluctuations of the solar neutrino flux due to magnetohydrodynamics (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. This revised version was published online in August 2006 with corrections to the Cover Date.
Keywords:magnetic perturbations  neutrino  oscillation
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