Current Status of the Resonant Spin-Flavor Precession Solution to the Solar Neutrino Problem

Preprint

20 October 1998

preprint
Published by arXiv in arXiv

Abstract

We discuss the current status of the resonant spin-flavor precession (RSFP) solution to the solar neutrino problem. We perform a fit to all the latest solar neutrino data for various assumed magnetic field profiles in the sun. We show that the RSFP can account for all the solar neutrino experiments, giving as good fit as other alternative solutions such as MSW or Just so, and therefore can be a viable solution to the solar neutrino problem

Keywords

SPIN FLAVOR PRECESSION
RESONANT SPIN FLAVOR
NEUTRINO PROBLEM
SOLAR NEUTRINO
MAGNETIC FIELD

All Related Versions

Version 1, 1998-10-20, ArXiv
Version 2, 1999-04-26, ArXiv
Published version: Astroparticle Physics, 12 (1-2), 87.

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