Metallicity, opacity coefficients and the solar standard model

descriptionPublicationkeyboard_double_arrow_right Article 01 Jul 1990 English Publisher:Springer Science and Business Media LLCJournal:Solar Physics, volume 128, pages 49-60 (issn: 0038-0938, eissn: 1573-093X,

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Authors: D. Courtaud; G. Damamme; E. Genot; M. Vuillemin; S. Turck-Chi�ze;

doi: 10.1007/bf00154146

Metallicity, opacity coefficients and the solar standard model

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Abstract

We discuss the effect of the uncertainties affecting the opacities on the derived characteristics of the Sun. We consider two sources of uncertainty: the relative composition of the Sun at birth and the difference between two opacity calculations. As an illustration, we discuss the effect of the choice of photospheric or meteoritic iron abundance on the predicted chlorine neutrino capture rate and present comparisons between the Los Alamos and Limeil opacity calculations.

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