Radiation from a strongly-magnetized plasma: The case of predominant scattering

DOI10.1007/BF00683336zbMath0502.76126OpenAlexW2008348982MaRDI QIDQ1172998

G. G. Pavlov, A. D. Kaminker, Yu. A. Shibanov

Publication date: 1982

Published in: Astrophysics and Space Science (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1007/bf00683336

zbMATH Keywords

scatteringanalytic solutionsneutron starsstrong magnetic fieldcold plasmadiffusion approach for normal modeseffects of electron-positron vacuum polarizationoptically thick tenuous plasmaspectra, angular dependences and polarization of outgoing radiationtransfer coefficientsX- ray and gamma-ray radiation

Mathematics Subject Classification ID

Galactic and stellar dynamics (85A05) Ionized gas flow in electromagnetic fields; plasmic flow (76X05) Radiative transfer in astronomy and astrophysics (85A25)

Cites Work

• The radiation of a hot magnetized plasma accreted by degenerate stars with a strong magnetic field
• Quantum effects in cyclotron plasma absorption

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