Simulation of Binary-single Interactions in AGN Disk. I. Gas-enhanced Binary Orbital Hardening

Simulation of Binary-single Interactions in AGN Disk. I. Gas-enhanced Binary Orbital Hardening

Stellar-mass binary black hole (BBH) mergers within the accretion disks of active galactic nuclei may contribute to gravitational wave (GW) events detected by ground-based GW detectors. In particular, the interaction between a BBH and a single stellar-mass black hole (sBH), known as the binary-singl...

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Bibliographic Details
Main Authors: Mengye Wang, Yiqiu Ma, Hui Li, Qingwen Wu, Ya-Ping Li, Xiangli Lei, Jiancheng Wu
Format: Article
Language:English
Published: IOP Publishing 2025-01-01
Series:The Astrophysical Journal
Subjects:
Active galactic nuclei
Gravitational waves
Hydrodynamical simulations
Gravitational interaction
Online Access:https://doi.org/10.3847/1538-4357/adbf8e
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https://doi.org/10.3847/1538-4357/adbf8e

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