New Results on Standard Solar Models

Details New Results on Standard Solar Models New Results on Standard Solar Models

2009-10-19

arxiv.org/abs/0910.3690v1

Astrophys.Space Sci.328:13-21,2010

Astronomy and Astrophysics

Astrophysics

Solar and Stellar Astrophysics

9 pages. Review talk presented at "Synergies between solar and stellar modelling", Rome, June 2009. To be published by Astroph

Scientific paper

10.1007/s10509-009-0174-8

We describe the current status of solar modelling and focus on the problems originated 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. Results presented here make focus both on helioseismic properties and the models as well as in the neutrino fluxes 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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