Solar Neutrinos: Spin Flavour Precession and LMA

Details Solar Neutrinos: Spin Flavour Precession and LMA Solar Neutrinos: Spin Flavour Precession and LMA

2005-11-30

arxiv.org/abs/hep-ph/0511341v1

Physics

High Energy Physics

High Energy Physics - Phenomenology

6 pages, 3 figures, contribution to 12th Lomonosov Conference in Elementary Particle Physics, Moscow, Aug 24-31 (2005)

Scientific paper

The time dependence that appears to be hinted by the data from the first 13 years of the solar neutrino Gallium experiments is viewed as resulting from a partial conversion of active neutrinos to light sterile ones through the resonant interaction between the magnetic moment of the neutrino and a varying solar field. A summary of the model and its predictions are presented for the forthcoming experiments Borexino and LENS.

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