Statistics – Computation
Scientific paper
Feb 1992
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992apj...386..308p&link_type=abstract
Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 386, Feb. 10, 1992, p. 308-324.
Statistics
Computation
2
Annihilation Reactions, Compton Effect, Gamma Ray Bursts, Line Spectra, Astronomical Models, Astronomical Spectroscopy, Computational Astrophysics, Electron Distribution, Pair Production, Scattering Cross Sections
Scientific paper
Attention is given to a synchrotron self-Compton emission model for gamma-ray bursts which produces narrow annihilation features for a variety of field strengths, primary electron injection energies, and injection rates. In this model, primary electrons are injected and cooled by synchrotron emission in a strong, homogeneous magnetic field, resulting in a pair cascade. Multiple resonant scattering with cyclotron photons efficiently traps and cools pairs in the ground state to an average energy where the Compton energy loss rate is zero, which is in agreement with previous estimates of a Compton temperature. The particle distributions in the ground state are determined by numerically solving the Fokker-Planck equation in the steady state. In the case of isotropic injection of primary electrons, a significant narrow-line feature appears in the overall emission. In the case of beamed injection, the annihilation line is broadened to the extent that it would not be observable.
Harding Alice K.
Preece Rob D.
No associations
LandOfFree
Resonant Compton cooling and annihilation line production in gamma-ray bursts does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Resonant Compton cooling and annihilation line production in gamma-ray bursts, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Resonant Compton cooling and annihilation line production in gamma-ray bursts will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1046478