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Rates and Beaming Angles of Gamma-Ray Bursts Associated with Compact Binary Coalescences

Some, if not all, binary neutron star (BNS) coalescences, and a fraction of neutron star–black hole (NSBH) mergers, are thought to produce sufficient mass ejection to power gamma-ray bursts (GRBs). However, this fraction, as well as the distribution of beaming angles of BNS-associated GRBs, is poorl...

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Principais autores: Shasvath J. Kapadia, Dimple, Dhruv Jain, Kuntal Misra, K. G. Arun, Resmi Lekshmi
Format: Artigo
Jezik:Inglês
Izdano: IOP Publishing 2024-01-01
Serija:The Astrophysical Journal Letters
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Online dostop:https://doi.org/10.3847/2041-8213/ad8dc7
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