Afterglow calculation in the Blandford-Lyutikov electromagnetic model of GRBs

Details Afterglow calculation in the Blandford-Lyutikov electromagnetic model of GRBs Afterglow calculation in the Blandford-Lyutikov electromagnetic model of GRBs

May 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006aipc..836..452g&link_type=abstract

GAMMA-RAY BURSTS IN THE SWIFT ERA: Sixteenth Maryland Astrophysics Conference. AIP Conference Proceedings, Volume 836, pp. 452-

Astronomy and Astrophysics

Astrophysics

Gamma-Ray Sources, Gamma-Ray Bursts

Scientific paper

We compute the afterglow of GRBs produced by electromagnetic outflows as
proposed by Lyutikov and Blandford (2003). Using a simple model for the
injection of electromagnetic energy to the forward shock we obtain the
afterglow evolution both during the period of activity of the central
source and after. Our method applies even to a variable central source.

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