A Natural Explanation of All Solar Neutrino Data by Resonant Spin-Flavor Precession Scenario

Abstract

It is emphasized that the $E_{\nu }$ (neutrino energy) spectrum of the ${\nu }_e$ survival probability in the Resonant Spin-Flavor Precession (RSFP) scenario has very desirable shape to reconcile all existing solar neutrino data. As the result, the RSFP scenario is shown to have rather broad allowed region to reconcile the data in the ($B,\Delta m^2$) plane, with $B$ being the magnetic field strength inside the Sun. The sensitivity of the allowed region on the different choices of the $B$ profile, and the time variations of the solar neutrino event rates in the RSFP scenario are also discussed in some detail.

Latex, 10 pages + 6 uuencoded postscript figures, KEK-TH-416, KOBE-TH-94-02 (KEK-TH number was corrected from 417 to 416)

References in corpus (5)

• Non-adiabatic Level Crossing in Resonant Neutrino Oscillations
• Solar Model Uncertainties, MSW Analysis, and Future Solar Neutrino Experiments
• Implications of Gallium Solar Neutrino Data for the Resonant Spin-Flavor Precession Scenario
• Time Variations of Solar Neutrino Signals and the RSFCN Hypothesis
• Solar Neutrino Data and Its Implications

Cited by in corpus (6)

• Global Analysis of the post-SNO Solar Neutrino Data for Standard and Non-Standard Oscillation Mechanisms
• Current Status of the Resonant Spin-Flavor Precession Solution to the Solar Neutrino Problem
• SNO and the neutrino magnetic moment solution of the solar neutrino problem
• Resonant neutrino spin-flavor precession and supernova shock revival
• On the Resonant Spin Flavor Precession of the Neutrino in the Sun
• Interactions Between Solar Neutrinos and Solar Magnetic Fields