Solar-neutrino experiments

Details Solar-neutrino experiments Solar-neutrino experiments

Aug 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989phrvl..63..837b&link_type=abstract

Physical Review Letters (ISSN 0031-9007), vol. 63, Aug. 21, 1989, p. 837-839.

Astronomy and Astrophysics

Astrophysics

17

Nuclear Astrophysics, Particle Mass, Solar Neutrinos, Solar Temperature, Boron Isotopes, Gallium Isotopes, Magnetic Moments, Radiation Detectors

Scientific paper

The observation of solar neutrinos at Kamiokande rules out the Mikheyev-Smirnov (1987) and Wolfenstein (1979) (MSW) theory with a 'large' mass difference between the neutrinos. There remains the MSW theory with a small mass difference between neutrinos 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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