Physics – High Energy Physics – High Energy Physics - Phenomenology
Scientific paper
2000-05-25
Nucl.Phys.B595:360-380,2001
Physics
High Energy Physics
High Energy Physics - Phenomenology
26 pages with 6 postscript figures included. Improved presentation and misprints corrected. Final version to appear in Nucl. P
Scientific paper
10.1016/S0550-3213(00)00546-0
We re-analyse the resonant spin-flavour (RSF) solutions to the solar neutrino problem in the framework of analytic solutions to the solar magneto-hydrodynamics (MHD) equations. By substantially eliminating the arbitrariness associated to the magnetic field profile due to both mathematical consistency and physical requirements we propose the simplest scheme (MHD-RSF, for short) for solar neutrino conversion using realistic static MHD solutions. Using such effective two-parameter scheme we perform the first global fit of the recent solar neutrino data, including event rates as well as zenith angle distributions and 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. We find our MHD-RSF fit to be somewhat better than those obtained for the favored neutrino oscillation solutions, though not in a statistically significant way. We briefly discuss the prospects to disentangle our MHD-RSF scenario at future solar neutrino experiments, giving some predictions for the SNO experiment.
Miranda Omar Gustavo
Peã-Garay C.
Rashba Timur I.
Semikoz Victor B.
Valle Jose W. F.
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