Metallicity, opacity coefficients and the solar standard model

Details Metallicity, opacity coefficients and the solar standard model Metallicity, opacity coefficients and the solar standard model

Jul 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990soph..128...49c&link_type=abstract

(IAU, The Inside the Sun Colloquium, 121st, Versailles, France, May 22-26, 1989) Solar Physics (ISSN 0038-0938), vol. 128, July

Physics

17

Metallicity, Solar Physics, Stellar Models, Abundance, Iron, Opacity, Solar Neutrinos, Solar Oscillations, Stellar Evolution

Scientific paper

The effect of the uncertainties affecting the opacities on the derived characteristics of the sun is discussed. Two sources of uncertainty are considered: the relative composition of the sun at birth and the difference between two opacity calculations. As an illustration, the effect of the choice of photospheric or meteoritic iron abundance on the predicted chlorine neutrino capture rate is discussed, and comparisons between the Los Alamos and Limeil opacity calculations are presented.

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