Solar Neutrinos: Spin Flavour Precession and LMA
High Energy Physics - Phenomenology
2016-12-07 v1
Abstract
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.
Cite
@article{arxiv.hep-ph/0511341,
title = {Solar Neutrinos: Spin Flavour Precession and LMA},
author = {Joao Pulido and B. C. Chauhan and R. S. Raghavan},
journal= {arXiv preprint arXiv:hep-ph/0511341},
year = {2016}
}
Comments
6 pages, 3 figures, contribution to 12th Lomonosov Conference in Elementary Particle Physics, Moscow, Aug 24-31 (2005)