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Reverse Shocks in Short Gamma-Ray Bursts -- The case of GRB 160821B and prospects as gravitational-wave counterparts

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conference contribution
posted on 04.08.2020, 15:46 by Gavin P Lamb
The shock system that produces the afterglow to GRBs consists of a forward- and a reverse-shock. For short GRBs, observational evidence for a reverse-shock has been sparse, however, the afterglow to GRB 160821B requires a reverse-shock at early times to explain the radio observations. GRB 160821B is additionally accompanied by the best-sampled macronova without a gravitational-wave detection, and an interesting late-time X-ray afterglow behaviour indicative of a refreshed-shock. The presence of an observed reverse-shock in an on-axis short GRB means that the reverse-shock should be considered as a potential counterpart to gravitational-wave detected mergers. As a gravitational-wave counterpart, the afterglow to an off-axis GRB jet can reveal the jet structure -- a reverse-shock will exist in these structured jet systems and the signature of these reverse-shocks, if observed, can indicate the degree of magnetisation in the outflow. Here we show the case of GRB 160821B, and how a reverse-shock will appear for an off-axis observer to a structured jet.

History

Author affiliation

Department of Physics and Astronomy

Source

Yamada Conference LXXI: Gamma-ray Bursts in the Gravitational Wave Era 2019, October 28 - November 1, 2019, Yokohama, Kanagawa, Japan

Version

VoR (Version of Record)

Published in

Proceedings of the Yamada Conference LXXI: Gamma-ray Bursts in the Gravitational Wave Era 2019

Copyright date

2020

Available date

10/06/2020

Language

en

Publisher version

http://yokohamagrb2019.wikidot.com/proceedings

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