A Semi-relativistic Equation of State for Stellar Interiors

Details A Semi-relativistic Equation of State for Stellar Interiors A Semi-relativistic Equation of State for Stellar Interiors

1998-11-12

arxiv.org/abs/astro-ph/9811200v1

Astronomy and Astrophysics

Astrophysics

4 pages including 2 PostScript figures, also available from http://www.speckle.mpifr-bonn.mpg.de/publications.html, accepted f

Scientific paper

10.1002/ctpp.2150390126

Using the technique of Pade Approximants for the correlation contributions of charged particles we are able to reproduce complex mathematical expressions by simple algebraic formulas. The Pade formulas are analytical expressions, which interpolate between certain density-temperature regions and are characterized by exact asymptotics. We present a semi-relativistic description of the thermodynamics applicable for stellar interiors. Comparisons with equation-of-state data obtained by other calculational schemes are presented.

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