The solar-neutrino problem, 1995.

Details The solar-neutrino problem, 1995. The solar-neutrino problem, 1995.

Dec 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995ncimc..18..671b&link_type=abstract

Nuovo Cimento C, Vol. 18C, N. 6, p. 671 - 684

Astronomy and Astrophysics

Astrophysics

1

Solar Neutrinos

Scientific paper

The status of the solar-neutrino problem (SNP), as is seen in 1995, is reviewed. Basically, there are two principal solutions to the SNP: (i) with standard neutrino (neutrino of SM of electroweak interactions) and (ii) with non-standard neutrino (neutrino beyond the SM). Actually, one can distinguish three solar-neutrino problems: the deficit of 8B neutrinos, the deficit of 7Be neutrinos and the HOMESTAKE/KAMIOKANDE conflict. The first problem probably can be solved with small correlated changes of nuclear cross-sections and the change of the central temperature of the Sun. The deficit of 7Be neutrinos looks like the key problem. The HOMESTAKE/KAMIOKANDE conflict strongly disfavours or excludes the standard neutrino (nuclear/astrophysical solution to the SNP). MSW conversion gives a most plausible explanation to the SNP.

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