Interaction between a high-temperature plasma situated in a gravitational field and electromagnetic radiation. I. II - Nonrelativistic temperatures kappa/b/T/e/ much less than m/e/c-squared

Details Interaction between a high-temperature plasma situated in a gravitational field and electromagnetic radiation. I. II - Nonrelativistic temperatures kappa/b/T/e/ much less than m/e/c-squared Interaction between a high-temperature plasma situated in a gravitational field and electromagnetic radiation. I. II - Nonrelativistic temperatures kappa/b/T/e/ much less than m/e/c-squared

Jun 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975fiz....18....7i&link_type=abstract

Fizika, vol. 18, no. 6, 1975, p. 7-15, 109-119. In Russian.

Astronomy and Astrophysics

Astronomy

Cosmic Plasma, Gravitational Fields, High Temperature Plasmas, Plasma-Electromagnetic Interaction, Relativistic Plasmas, Astronomical Models, Electromagnetic Radiation, Plasma Temperature, Schwarzschild Metric, Stellar Atmospheres

Scientific paper

A linearized relativistic kinetic equation is used to study the interaction between a high-frequency electromagnetic radiation and a fully ionized plasma situated in a gravitational field. The pseudotensors of complex conductance, permittivity, and energy absorption are obtained. The results are applied to analysis of a plasma in the Schwarzschild field. Enhancement of electromagnetic radiation and reasons accounting for negative absorption are discussed.

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