Astronomy and Astrophysics – Astrophysics
Scientific paper
Nov 1985
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985a%26a...152..336w&link_type=abstract
Astronomy and Astrophysics (ISSN 0004-6361), vol. 152, no. 2, Nov. 1985, p. 336-342.
Astronomy and Astrophysics
Astrophysics
4
Electron Scattering, Maxwell-Boltzmann Density Function, Photon-Electron Interaction, Relativistic Theory, Scattering Cross Sections, Compton Effect, Electron Energy, Kernel Functions, Least Squares Method, Temperature Dependence
Scientific paper
A set of temperature-corrected, photon-Maxwellian electron cross sections, which complement the static Klein-Nishina set, are developed for radiative physics applications. Algorithms using static expressions can easily use the fitted forms generated in the analysis. The fit has been effected with a minimal number of parameters, evolves naturally from the relativistic (exact) scattering kernal, is excellent in predicting total cross sections, and is good in predicting differential scattering cross sections over the photon energy range (0-1 MeV) and background temperature (0-100 keV).
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