New look at the solar neutrino problem

Details New look at the solar neutrino problem New look at the solar neutrino problem

Jan 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993phrvl..70..375w&link_type=abstract

Physical Review Letters (ISSN 0031-9007), vol. 70, no. 4, p. 375-378.

Statistics

Computation

13

Computational Astrophysics, Solar Neutrinos, Stellar Models, Confidence Limits, Monte Carlo Method, Normal Density Functions, Solar Flux, Solar Observatories, Stellar Interiors

Scientific paper

We present a graphical and statistical comparison of observations of solar neutrinos with theoretical predictions for the Mikheyev-Smirnov-Wolfenstein effect and a class of 'nonstandard' solar 'models'. The method used to compare the results makes the level of agreement or nonagreement between theory and observation more readily apparent. Included in our analysis are the standard-solar-model flux uncertainties. We also present predictions for Solar Neutrino Observatory charged-current rates.

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