Runaway Eccentricity Growth: A Pathway for Binary Black Hole Mergers in AGN Disks

Binary black holes (BBHs) embedded within the accretion disks that fuel active galactic nuclei (AGN) are promising progenitors for the source of gravitational wave (GW) events detected by LIGO/VIRGO. Several recent studies have shown that when these binaries form, they are likely to be highly eccent...

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Hlavní autoři:	Josh Calcino, Adam M. Dempsey, Alexander J. Dittmann, Hui Li
Médium:	Artigo
Jazyk:	Inglês
Vydáno:	IOP Publishing 2024-01-01
Edice:	The Astrophysical Journal
Témata:	Astrophysical fluid dynamics Active galactic nuclei Black holes Accretion Gravitational wave sources
On-line přístup:	https://doi.org/10.3847/1538-4357/ad4a53
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