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A numerical jet model for the prompt emission of gamma-ray bursts

A numerical jet model for the prompt emission of gamma-ray bursts

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2476744253

A numerical jet model for the prompt emission of gamma-ray bursts

About this item

Full title

A numerical jet model for the prompt emission of gamma-ray bursts

Publisher

Ithaca: Cornell University Library, arXiv.org

Journal title

arXiv.org, 2021-01

Language

English

Formats

Publication information

Publisher

Ithaca: Cornell University Library, arXiv.org

More information

Scope and Contents

Contents

Gamma-ray bursts (GRBs) are known to be highly collimated events, and are mostly detectable when they are seen on-axis or very nearly on-axis. However, GRBs can be seen from off-axis angles, and the recent detection of a short GRB associated to a gravitational wave event has conclusively shown such a scenario. The observer viewing angle plays an im...

Alternative Titles

Full title

A numerical jet model for the prompt emission of gamma-ray bursts

Identifiers

Primary Identifiers

Record Identifier

TN_cdi_proquest_journals_2476744253

Permalink

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2476744253

Other Identifiers

E-ISSN

2331-8422

DOI

10.48550/arxiv.2101.02984

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