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GRB fireball physics: prompt and early emission

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Published 20 September 2006 Published under licence by IOP Publishing Ltd
, , Focus on Gamma-Ray Bursts in the Swift Era Citation D B Fox and P Mészáros 2006 New J. Phys. 8 199 DOI 10.1088/1367-2630/8/9/199

1367-2630/8/9/199

Abstract

We review the fireball shock model of gamma-ray burst (GRB) prompt and early afterglow emission in the light of rapid follow-up measurements made and enabled by the multi-wavelength Swift satellite. These observations are leading to a reappraisal and expansion of the previous standard view of the GRB and its fireball. New information on the behaviour of the burst and afterglow on minutes to hour timescales has led, among other results, to the discovery and follow-up of short GRB afterglows, the opening up of the z ≳ 6 redshift range, and the first prompt multi-wavelength observations of a long GRB-supernova. We discuss the salient observational results and some associated theoretical issues.

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