Solar-neutrino experiments

descriptionPublicationkeyboard_double_arrow_right Article 21 Aug 1989 English Publisher:American Physical Society (APS)Journal:Physical Review Letters, volume 63, pages 837-839 (issn: 0031-9007,

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Authors: , Bethe;

doi: 10.1103/physrevlett.63.837

pmid: 10041198

Solar-neutrino experiments

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Abstract

The observation of solar neutrinos at Kamiokande rules out the Mikheyev-Smirnov-Wolfenstein (MSW) theory with a large'' mass difference between the neutrinos, {Delta}{ital m}{sup 2}{congruent}10{sup {minus}4} eV{sup 2}. There remain the MSW theory with a small {Delta}{ital m}{sup 2}{congruent}10{sup {minus}7} eV{sup 2} or the assumption of unexpectedly low central temperature in the Sun. A decision between these two alternatives will be possible on the basis of the future gallium experiment, and the Sudbury experiment with heavy water.

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