REVIEW 1 cited by
Gamma-ray burst afterglow theory
Not yet reviewed by Pith; the record is open.
This paper has not been read by Pith yet. Machine review is queued; the pith claim, tier, and objections will appear here once it completes.
SPECIMEN: schema-true, not a live event
T0 review · schema-true
One-sentence machine reading of the paper's core claim.
pith:XXXXXXXX · record.json · timestamp
read the original abstract
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.
Forward citations
Cited by 1 Pith paper
-
TeV afterglow emission from a structured GRB jet using the kinetic approach
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.
Discussion (0). Continue with ORCID to comment.