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Gamma-ray burst afterglow theory

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arxiv 1309.3869 v1 pith:HK74CTNO submitted 2013-09-16 astro-ph.HE

classification astro-ph.HE
keywords theoreticalafterglowafterglowsburstgamma-raymanyquestionsradiation
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It is by now fairly well established that gamma-ray burst afterglows result from initially relativistic outflows interacting with the medium surrounding the burster and emitting non-thermal radiation ranging from radio to X-rays. However, beyond that, many big and small questions remain about afterglows, with the accumulating amount of observational data at the various frequencies raising as many questions as they answer. In this review I highlight a number of current theoretical issues and how they fit or do not fit within our basic theoretical framework. In addition to theoretical progress I will also emphasize the increasing role and usefulness of numerical studies of afterglow blast waves and their radiation.

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Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. OpenAlex reports about 10 citations worldwide. Full citation record

  1. TeV afterglow emission from a structured GRB jet using the kinetic approach

    astro-ph.HE 2025-01 conditional novelty 6.0 of 10

    Jet angular structure changes the TeV inverse-Compton emission from GRB afterglows, and a kinetic-model fit to GRB 170817A predicts no CTAO TeV detection even on-axis.

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