Abstract
We describe the current status of solar modeling and focus on the problems originating with the introduction of solar abundance determinations with low CNO abundance values. We use models computed with solar abundance compilations obtained during the last decade, including the newest published abundances by Asplund and collaborators. The results presented here focus on both helioseismic properties and models as well as neutrino flux predictions. We also discuss changes in radiative opacities to restore agreement between helioseismology, solar models, and solar abundances and show the effect of such modifications on solar neutrino fluxes.
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Serenelli, A.M. New results on standard solar models. Astrophys Space Sci 328, 13–21 (2010). https://doi.org/10.1007/s10509-009-0174-8
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DOI: https://doi.org/10.1007/s10509-009-0174-8