New Interpretation on the Solar Neutrino Flux with Flavor Mixing and Majorana Magnetic Moment

Details New Interpretation on the Solar Neutrino Flux with Flavor Mixing and Majorana Magnetic Moment New Interpretation on the Solar Neutrino Flux with Flavor Mixing and Majorana Magnetic Moment

2003-06-23

arxiv.org/abs/hep-ph/0306210v1

Physics

High Energy Physics

High Energy Physics - Phenomenology

12 pages, RevTeX, 2 eps figures

Scientific paper

A simple and model-independent method is proposed to extract information on solar $\nu_e$ 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.

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