What Do Solar Models Tell Us About Solar Neutrino Experiments?

Details What Do Solar Models Tell Us About Solar Neutrino Experiments? What Do Solar Models Tell Us About Solar Neutrino Experiments?

1992-11-20

arxiv.org/abs/hep-ph/9211291v1

Physics

High Energy Physics

High Energy Physics - Phenomenology

4 pages (LaTeX file, figures not included)

Scientific paper

10.1063/1.43282

If the published event rates of the chlorine and Kamiokande solar neutrino experiments are correct, then the energy spectrum of neutrinos produced by the decay of $^8$B in the sun must be different from the energy spectrum determined from laboratory nuclear physics measurements. This change in the energy spectrum requires physics beyond the standard electroweak model. In addition, the GALLEX and SAGE experiments, which currently have large statistical uncertainties, differ from the predictions of the standard solar model by $2 \sigma$ and $3 \sigma$, respectively.

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