The prompt GRB high energy emission from internal shocks: synchrotron vs inverse Compton component

Physics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

Gamma-Ray Sources, Gamma-Ray Bursts, X- And Gamma-Ray Telescopes And Instrumentation, Radiation Belts

Scientific paper

We performed a detailed calculation of gamma-ray burst (GRB) prompt emission in the framework of the internal shock scenario, focusing on the high energy (GeV) bands. In order to follow the evolution of the ultrarelativistic inhomogeneous wind, we combined a model for the dynamics of internal shocks with a detailed calculation of the radiative processes occurring in the shocked medium. We present the resulting synthetic GRB light curves and spectra. We show the spectral evolution that can be expected for different sets of microphysics parameters and parameters of the dynamical evolution, and how the relative importance of synchrotron and inverse Compton components is varying during a burst.

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

The prompt GRB high energy emission from internal shocks: synchrotron vs inverse Compton component 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 The prompt GRB high energy emission from internal shocks: synchrotron vs inverse Compton component, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The prompt GRB high energy emission from internal shocks: synchrotron vs inverse Compton component will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-1111532

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