Relativistic free-free Gaunt factor of the dense high-temperature stellar plasma

Details Relativistic free-free Gaunt factor of the dense high-temperature stellar plasma Relativistic free-free Gaunt factor of the dense high-temperature stellar plasma

Mar 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987apjs...63..661n&link_type=abstract

Astrophysical Journal Supplement Series (ISSN 0067-0049), vol. 63, March 1987, p. 661-684.

Physics

Atomic Physics

18

Atomic Physics, Cosmic Plasma, High Temperature Plasmas, Relativistic Plasmas, Stellar Atmospheres, Dense Plasmas, Opacity

Scientific paper

The free-free Gaunt factor of the dense high-temperature stellar plasma is calculated by using the accurate relativistic cross section and is compared with the Gaunt factor derived by using Sommerfeld's exact nonrelativistic cross section. A wide range of electron degeneracy is accurately taken into account. Significant deviations from the nonrelativistic results are found for high-temperature cases. Results are presented in the form of extensive tables to facilitate applications.

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