It is shown that the experiments on solar neutrinos can be accounted in terms of the Mikheyev-Smirnov-Wolfestein theory with DELTAm2 = 6 x 10(-6) eV2 and sin2 2theta = 7 X 10(-3). In the scenario proposed here the high energy neutrinos, from B-8, have a survival probability around 1/3, the intermediate ones, around the Be-7 line a very small one approximately 2 x 10(-3) axid the low energy neutrinos, the ones coming from pp reactions, do not oscillate.
THE SOLAR-NEUTRINO PROBLEM WITHIN MSW THEORY / Esposito, S. - In: MODERN PHYSICS LETTERS A. - ISSN 0217-7323. - 8:17(1993), pp. 1557-1562. [10.1142/S021773239300129X]
THE SOLAR-NEUTRINO PROBLEM WITHIN MSW THEORY
ESPOSITO S
1993
Abstract
It is shown that the experiments on solar neutrinos can be accounted in terms of the Mikheyev-Smirnov-Wolfestein theory with DELTAm2 = 6 x 10(-6) eV2 and sin2 2theta = 7 X 10(-3). In the scenario proposed here the high energy neutrinos, from B-8, have a survival probability around 1/3, the intermediate ones, around the Be-7 line a very small one approximately 2 x 10(-3) axid the low energy neutrinos, the ones coming from pp reactions, do not oscillate.File in questo prodotto:
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