A tabulation of thermodynamical properties of fully ionized matter in stellar interiors

Details A tabulation of thermodynamical properties of fully ionized matter in stellar interiors A tabulation of thermodynamical properties of fully ionized matter in stellar interiors

Dec 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988a%26as...76..157s&link_type=abstract

Astronomy and Astrophysics Supplement Series (ISSN 0365-0138), vol. 76, no. 2, Dec. 1988, p. 157-184.

Statistics

Computation

74

Computational Astrophysics, Equations Of State, Ionization, Stellar Interiors, Thermodynamic Properties, Coulomb Collisions, Electron-Positron Pairs, Ideal Gas, Stellar Structure

Scientific paper

An equation of state for fully ionized matter is presented between 106 ≤ T ≤ 1010K. Degeneration and relativistic effects for electrons have been taken into account together with pairs' production and Coulomb interactions. Tables are presented for pure hydrogen, helium, carbon and oxygen mixtures which allow for the evaluation of stellar interiors before the carbon ignition. Tables for heavier elements are available upon request. The influences of this equation of state on stellar evolution are briefly discussed together with the main departures from the ideal gas approximation in astrophysical environments.

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