Resonant Raman-cyclotron scattering in very strong magnetic fields

Details Resonant Raman-cyclotron scattering in very strong magnetic fields Resonant Raman-cyclotron scattering in very strong magnetic fields

Jun 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987apj...317..282m&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 317, June 1, 1987, p. 282-289.

Astronomy and Astrophysics

Astrophysics

1

Cyclotron Resonance, Magnetic Fields, Radiative Transfer, Raman Spectra, Resonance Scattering, Transition Probabilities, Eigenvalues, Electron Energy, High Temperature Plasmas, Scattering Cross Sections, Space Plasmas, Wave Functions

Scientific paper

Radiation transfer in strongly magnetized hot astrophysical plasmas is dominated by resonant Compton-cyclotron scattering. Raman scattering of hard photons is a potential mechanism of first electron excitation and then creation of secondary cyclotron photon. In this paper, transition probabilities and cross sections for Raman diffusion on strongly magnetized electrons are derived.

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