English

Effective Compton Cross Section in Non-Degenerate High Temperature Media

Astrophysics 2009-11-10 v1

Abstract

The effective compton cross section in a non-degenerate plasma(n{(kT/c)2+2mkTh2}3/2n\ll\{\frac{(kT/c)^{2}+2mkT}{h^{2}}\}^{^{3/2}}) is investigated in a wide range of temperatures. The results show a decreasing behavior with temperature especially for kTmec2kT\gg m_{e}c^{2}. The $may be important in phenomena like accretion discs or ultra-relativistic blast waves in GRB models, where the emitted radiation has to pass through a medium containing high energy electrons.

Keywords

Cite

@article{arxiv.astro-ph/0402194,
  title  = {Effective Compton Cross Section in Non-Degenerate High Temperature Media},
  author = {F. Shekh-Momeni and J. Samimi},
  journal= {arXiv preprint arXiv:astro-ph/0402194},
  year   = {2009}
}

Comments

12 pages, 7 figures

R2 v1 2026-07-22T08:34:36.871Z