The Rosseland mean free-free Gaunt factor of the dense high-temperature stellar plasma

Details The Rosseland mean free-free Gaunt factor of the dense high-temperature stellar plasma The Rosseland mean free-free Gaunt factor of the dense high-temperature stellar plasma

Dec 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991apj...382..636i&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 382, Dec. 1, 1991, p. 636-639.

Statistics

Computation

11

Computational Astrophysics, Dense Plasmas, Stellar Winds, Electron Density (Concentration), Opacity, Relativistic Particles, Stellar Temperature

Scientific paper

The Rosseland mean free-free Gaunt factor of the dense high-temperature stellar plasma is calculated based on both the accurate relativistic cross section and Sommerfeld's exact nonrelativistic cross section. A wide range of electron degeneracy is accurately taken into account. Comparison of the resulting free-free opacity with the electron conduction opacity is made.

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