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Ve present neutrino fluxes from a sequence of solar models that differ from one another in regard to opacity, equation of state, and nuclear cross-section factors. Using current estimates of the relevant input parameters, we obtain capture rates that range between 3 and 10 times the most recent result of the Davis neutrino-capture experiment. The contribution to a theoretical capture rate due to neutrinos from all reactions other than 8B decay ranges from 0.5 to 1.5 times the latest observational result. Comparison with results of other solar model calculations indicates reasonable agreement when results are normalixed to the same input parameters.
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Abraham et al. (1971) studied this question.
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