Resonant Compton cooling and annihilation line production in gamma-ray bursts

Statistics – Computation

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

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.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

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.

Rate now

     

Profile ID: LFWR-SCP-O-1046478

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.