Confronting Spin Flavor Solutions of the Solar Neutrino Problem with current and future solar neutrino data

Details Confronting Spin Flavor Solutions of the Solar Neutrino Problem with current and future solar neutrino data Confronting Spin Flavor Solutions of the Solar Neutrino Problem with current and future solar neutrino data

2002-07-26

arxiv.org/abs/hep-ph/0207326v3

Phys.Rev.D66:093009,2002

Physics

High Energy Physics

High Energy Physics - Phenomenology

new appendix added discussing the impact of the KamLAND data. This updates the one published in Phys.Rev.D66:093009,2002

Scientific paper

10.1103/PhysRevD.66.093009

We show that spin flavor precession solutions to the solar neutrino problem,
although preferred by the latest solar data, are ruled out by the first results
from the KamLAND reactor experiment, at more than 3_sigma. An illustrative chi2
plot comparing these descriptions with oscillations is given.

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