Solar neutrinos and other problems and their relation to energy production in the sun

Physics

Scientific paper

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Nuclear Reactions, Solar Neutrinos, Solar Physics, Helium, Nuclear Fusion, Quarks, Solar Temperature, Stellar Structure

Scientific paper

Models of the solar interior, based on the usual physical assumptions, predict a neutrino flux several times greater than that observed in the Davis 37Cl experiment. The author points out some less well known discrepancies between theoretical predictions of the standard solar model and relevant observations. It is suggested that an additional source of energy production that competes with the proton-proton chain and carbon-nitrogen cycles, can reduce these discrepancies if it has a sufficiently strong temperature dependence.

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