The active galactic nucleus (AGN) disc has been proposed as a potential channel for the
merger of binary black holes. The population of massive stars and black holes in AGN discs …

Stellar-mass black holes (sBHs) embedded in gaseous disks of active galactic nuclei (AGN)
can be important sources of detectable gravitational radiation for LIGO/Virgo when they form …

The black hole (BH) binaries in active galactic nuclei (AGN) are expected to form mainly
through scattering encounters in the ambient gaseous medium. Recent simulations …

Many stellar-mass black holes (sBHs) are expected to orbit supermassive black holes at
galactic centers. For galaxies with active galactic nuclei, it is likely that the sBHs reside in a …

Context. Dynamical encounters of stellar-mass black holes (BHs) in a disc of compact
objects around a supermassive BH (SMBH) can accelerate the formation and coalescence …

Despite the increasing number of gravitational wave (GW) detections, the astrophysical
origin of binary black hole (BBH) mergers remains elusive. A promising formation channel …

The accretion disks that fuel active galactic nuclei (AGNs) may house numerous stars and
compact objects, formed in situ or captured from nearby star clusters. Embedded neutron …

Binary black holes (BBHs) in eccentric orbits produce distinct modulations the emitted
gravitational waves (GWs). The measurement of orbital eccentricity can provide robust …

Accretion discs in active galactic nuclei (AGNs) foster black hole (BH) formation, growth, and
mergers. Stellar mass BHs migrate inwards under the influence of hydrodynamical torques …

The astrophysical origin of stellar-mass black hole (BH) mergers discovered through
gravitational waves (GWs) is widely debated. Mergers in the disks of active galactic nuclei …