New Interpretation on the Solar Neutrino Flux with Flavor Mixing and Majorana Magnetic Moment
Abstract
Description
A simple and model-independent method is proposed to extract information on solar $ν_e$ transition into antineutrinos via the spin flavor precession (SFP) from the measurements of solar neutrino flux at SNO and Super-Kamiokande. Incorporating the KamLAND experimental results, we examine how large the suppression of the solar neutrino flux could be due to the SFP mechanism in the context of the hybrid scenario with two-flavor neutrino and antineutrino mixings.
12 pages, RevTeX, 2 eps figures
12 pages, RevTeX, 2 eps figures