Physics – High Energy Physics – High Energy Physics - Phenomenology
Scientific paper
2001-01-18
Nucl.Phys.Proc.Suppl.95:123-129,2001; Part.Nucl.Lett.104:71-78,2001
Physics
High Energy Physics
High Energy Physics - Phenomenology
7 pages, 7 postscript figures, espcrc2.sty. Talk given at the EuroConference on Frontiers in Particle Astrophysics and Cosmolo
Scientific paper
10.1016/S0920-5632(01)01067-2
The analysis of the resonant spin-flavour (RSF) solutions to the solar neutrino problem in the framework of simplest analytic solutions to the solar magneto-hydrodynamics (MHD) equations is presented. We performed the global fit of the recent solar neutrino data, including event rates as well as day and night recoil electron spectra induced by solar neutrino interactions in SuperKamiokande. We compare quantitatively our simplest MHD-RSF fit with vacuum oscillation (VAC) and MSW--type (SMA, LMA and LOW) solutions to the solar neutrino problem using a common well-calibrated theoretical calculation and fit procedure and find MHD-RSF fit to be somewhat better than those obtained for the favored neutrino oscillation solutions. We made the predictions for future experiments to disentangle the MHD-RSF scenario from other scenarios.
Miranda Omar Gustavo
Penya-Garay C.
Rashba Timur I.
Semikoz Victor B.
Valle Jose W. F.
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