Solar models using the SAHA-S equation of state

Details Solar models using the SAHA-S equation of state Solar models using the SAHA-S equation of state

Oct 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004aipc..731..178a&link_type=abstract

EQUATION-OF-STATE AND PHASE-TRANSITION ISSUES IN MODELS OF ORDINARY ASTROPHYSICAL MATTER. AIP Conference Proceedings, Volume 73

Astronomy and Astrophysics

Astrophysics

4

Magnetohydrodynamics And Plasmas, Thermodynamic Processes, Conduction, Convection, Equations Of State, Solar Interior

Scientific paper

We present solar models computed with a newly developed equation of state (EOS) of solar plasma, SAHA-S. SAHA-S is a solar version of the SAHA-* family of EOS designed for various states of matter. It incorporates modern state-of-the-art features such as arbitrary degenerated and slightly relativistic electron gas, improved formalism for Debye correction and generalized Planck-Larkin function which refines bound states contributions. We discuss standard solar models computed with SAHA-S and two versions of OPAL.

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