A solution of the solar-neutrino problem

Details A solution of the solar-neutrino problem A solution of the solar-neutrino problem

Oct 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990phrvl..65.2233b&link_type=abstract

Physical Review Letters (ISSN 0031-9007), vol. 65, Oct. 29, 1990, p. 2233-2235.

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Electron Scattering, Elementary Particle Interactions, Solar Neutrinos, Solar Physics, Chlorine, Computational Astrophysics, Stellar Models

Scientific paper

The results from the Kamiokande neutrino-electron scattering experiments are compared with those from a chlorine experiment and with solar models. The comparison shows that the standard electroweak model with zero neutrino masses is probably inadequate to explain the findings. It is concluded that the nonadiabatic Mikheyev-Smirnov-Wolfenstein solution is the most likely explanation of the problem.

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