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Ten recently-published solar models give neutrino fluxes that lie within a range of % of the average value, a convergence that is independent of uncertainties in the measured laboratory rate of the reaction. If nothing happens to solar neutrinos after they are created ({\it a la} standard electroweak theory) and the operating solar neutrino experiments are correct, then the solar neutrino flux must be less than 50% of the solar model value. At least three of the four existing solar neutrino experiments must be wrong {\it if}: (1) standard electroweak theory is correct, and (2) the true neutrino flux lies within the range predicted by standard solar models.

生成讲解博客的中文版本

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