Optical flashes and radio flares in GRB afterglows: Numerical study

Physics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

1

Jets And Bursts, Galactic Winds And Fountains, Observational Cosmology, Gamma-Ray Sources, Gamma-Ray Bursts

Scientific paper

We numerically study the evolution of an adiabatic relativistic fireball interacting with an ambient uniform medium, both in the initial energy transfer stage and in its late evolution. It is shown that the Blandford-McKee solution adequately describes the evolution of the shocked ejecta quite early on and for as long as the fire-ball material has relativistic temperatures. In the case where the reverse shock is only mildly relativistic, the shocked ejecta becomes cold almost immediately and the evolution deviates from the Blandford-McKee solution. We derive analytical expressions for the ejecta evolution in its cold regime. This solution gives a good approximation to the numerical results. We estimate the radiation from the fireball ejecta using the numerical hydrodynamic evolution in both cases: cold and hot ejecta. Surprisingly, we find that both evolutions give rather similar light curves, decaying approximately as t-2 in the optical and peaking after about one day in the radio, even though the hydrodynamics is different. .

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

Optical flashes and radio flares in GRB afterglows: Numerical study 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 Optical flashes and radio flares in GRB afterglows: Numerical study, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Optical flashes and radio flares in GRB afterglows: Numerical study will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-1522936

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