SAHA-S Equation of State in Solar Modelling and Heavy Elements Content

Details SAHA-S Equation of State in Solar Modelling and Heavy Elements Content SAHA-S Equation of State in Solar Modelling and Heavy Elements Content

Nov 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aipc..948..213b&link_type=abstract

UNSOLVED PROBLEMS IN STELLAR PHYSICS: A Conference in Honor of Douglas Gough. AIP Conference Proceedings, Volume 948, pp. 213-2

Physics

1

Stellar Structure, Interiors, Evolution, Nucleosynthesis, Ages, Thermodynamic Processes, Conduction, Convection, Equations Of State, Solar Interior, Composition

Scientific paper

The definition of the equation of state and its role in stellar structure are discussed. With the example of the recently developed SAHA-S EOS, the principal features of an astrophysical EOS are illustrated. The phenomenon of sequential ionization of small impurities is described and numerically estimated for the heavy elements in the solar convection zone. The approach may be applied to the determination of the chemical composition based on the Γ1 profile.

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