On the natural line width of absorption lines in strong magnetic stellar fields

Details On the natural line width of absorption lines in strong magnetic stellar fields On the natural line width of absorption lines in strong magnetic stellar fields

Apr 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994ap%26ss.214..103b&link_type=abstract

Astrophysics and Space Science, Vol. 214, No. 1-2, Proceedings of the second United Nations/European Space Agency Workshop, Bogo

Astronomy and Astrophysics

Astrophysics

Absorption Cross Sections, Absorption Spectra, Gamma Ray Bursts, Spectral Line Width, Stellar Magnetic Fields, X Ray Scattering, X Ray Spectra, Compton Effect, Electron Scattering, Far Ultraviolet Radiation, Scattering Cross Sections

Scientific paper

In the last years, the interest in explaining the existence of a singularity at low frequencies (omega = 0) in the differential cross section of photon scattering by electrons, in a homogeneous magnetic field, for the transitions between the Landau levels N = 1 and N' = 0, has greatly increased. It is the purpose of this paper to present a calculation of the cross section for the absorption of radiation by an electron in a strong magnetic stellar field, using the Wigner-Weisskopf approximation to better understand this kind of singularity in the Compton cross section.

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