GW190521 formation scenarios via relativistic accretion

The recent gravitational wave transient GW190521 has been interpreted by the LIGO-Virgo collaboration (LVC) as sourced by a binary black hole (BH) merger. According to the LVC parameter estimation, at least one of these progenitors falls into the so-called pair-instability supernova mass gap. This r...

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Bibliographic Details
Main Author: Cruz-Osorio, Alejandro (author)
Other Authors: Lora-Clavijo, Fabio D. (author), Herdeiro, Carlos (author)
Format: article
Language:eng
Published: 2021
Subjects:
Accretion
Astrophysical black holes
Hydrodynamical simulations
Primordial black holes
Online Access:http://hdl.handle.net/10773/31612
Country:Portugal
Oai:oai:ria.ua.pt:10773/31612

Internet

http://hdl.handle.net/10773/31612

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