Electron-photon interaction in hot strongly magnetized plasmas

Details Electron-photon interaction in hot strongly magnetized plasmas Electron-photon interaction in hot strongly magnetized plasmas

Oct 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982acns.rept..296h&link_type=abstract

In Max-Planck Inst. Phys. and Astrophys. Accreting Neutron Stars p 296-298 (SEE N83-15179 05-88)

Astronomy and Astrophysics

Astrophysics

High Temperature Plasmas, Neutron Stars, Photon-Electron Interaction, Stellar Magnetic Fields, Stellar Mass Accretion, Cyclotron Resonance, Electron Spin, Electron Transitions, Emission Spectra, Relativistic Effects

Scientific paper

Results of calculations of electron-photon interaction processes in hot, strongly magnetized plasmas are given. Special emphasis is given to the relativistic effects. It was concluded that relativistic effects are much greater than of the order of B/B sub cr (approximately 0.1), contrary to expectations. Locations and shapes of cyclotron lines depend strongly on the emission angle, which is important for the interpretation of the observed variations of the line features during the pulse period.

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