Hydrodynamic Timescales and Temporal Structure of Gamma-Ray Bursts

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© 1995. The American Astronomical Society. All rights reserved. Printed in U.S.A.
, , Citation Re'em Sari and Tsvi Piran 1995 ApJ 455 L143 DOI 10.1086/309835

1538-4357/455/2/L143

Abstract

We calculate the hydrodynamic timescales for a spherical ultrarelativistic shell that is decelerated by the ISM and discuss the possible relations between these timescales and the observed temporal structure in γ-ray bursts. We suggest that the bursts' duration is related to the deceleration time, the variability is related to the ISM inhomogeneities, and that precursors are related to internal shocks within the shell. Good agreement can be achieved for these quantities with reasonable, not fine-tuned, astrophysical parameters. The difference between Newtonian and relativistic reverse shocks may lead to the observed bimodal distribution of bursts' durations.

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10.1086/309835