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DOE OSTI · 22280711

Recent developments for realistic solar models

Serenelli, Aldo M.
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Abstract

The 'solar abundance problem' has triggered a renewed interest in revising the concept of SSM from different perspectives: 1) constituent microphysics: equation of state, nuclear rates, radiative opacities; 2) constituent macrophysics: the physical processes impact the evolution of the Sun and its present-day structure, e.g. dynamical processes induced by rotation, presence of magnetic fields; 3) challenge the hypothesis that the young Sun was chemically homogeneous: the possible interaction of the young Sun with its protoplanetary disk. Here, I briefly review and then present a (personal) view on recent advances and developments on solar modeling, part of them carried out as attempts to solve the solar abundance problem.

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79 ASTRONOMY AND ASTROPHYSICSASTROPHYSICSELEMENT ABUNDANCEEQUATIONS OF STATEMAGNETIC FIELDSOPACITYPROTOPLANETSROTATIONSTAR EVOLUTIONSTAR MODELSSUN

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Serenelli, Aldo M.. 2014-05-02. Recent developments for realistic solar models. https://doi.org/10.1063/1.4874058

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