The Simplest Resonant Spin–Flavour Solution to the Solar Neutrino Problem

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 1 E-mail: [email protected] 2 E-mail: [email protected] 3 E-mail: [email protected] 4 E-mail: [email protected] 5 E-mail: [email protected] 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 with ∆m2 ≈ 10−8eV 2 and sin 2θ = 0. We briefly discuss the prospects to disentangle our MHD-RSF scenario from oscillation–type solutions to the solar neutrino problem at future solar neutrino experiments, giving some predictions for the SNO experiment.