Physics – High Energy Physics – High Energy Physics - Phenomenology
Scientific paper
1993-01-14
Phys.Lett.B303:85-94,1993
Physics
High Energy Physics
High Energy Physics - Phenomenology
LaTeX, 16 pages, 5 figures (not included by available upon request by fax or ordinary mail)
Scientific paper
10.1016/0370-2693(93)90048-M
We consider the implications of the recent results of SAGE and GALLEX experiments for the solution of the solar neutrino problem in the framework of the resonant neutrino spin-flavor precession scenario. It is shown that this scenario is consistent with all the existing solar neutrino data including the gallium results. The quality of the fit of the data depends crucially on the magnetic field profile used which makes it possible to get information about the magnetic field in the solar interior. In particular, the magnetic field in the core of the sun must not be too strong ($<3 \times 10^6$ G). The detection rate in the gallium detectors turns out to be especially sensitive to the magnitude of $\Delta m^2$. Predictions for forthcoming solar-neutrino experiments are made.
Akhmedov Eugene Kh.
Lanza Antonio
Petcov Serguey T.
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