The accretion disks of active galactic nuclei (AGNs) are promising locations for the merger of
compact objects detected by gravitational wave (GW) observatories. Embedded within a …

The origin of stellar-mass black hole mergers discovered through gravitational waves is
being widely debated. Mergers in the disks of active galactic nuclei (AGNs) represent a …

GW190521, the most massive binary black hole merger confidently detected by the LIGO-
Virgo-KAGRA Collaboration, is the first gravitational-wave observation of an intermediate …

Some Seyfert galaxies are detected in high-energy gamma rays, but the mechanism and site
of gamma-ray emission are unknown. Also, the origins of the cosmic high-energy neutrino …

Stellar-mass BHs (sBHs) are predicted to be embedded in active galactic nucleus (AGN)
disks owing to gravitational drag and in situ star formation. However, we find that, due to a …

We perform a series of 3D simulations to study the accretion of giant planet embedded in
protoplanetary discs (PPDs) over gap-opening time-scales. We find that the accretion mass …

Stellar-mass black holes (BHs) are predicted to be embedded in the disks of active galactic
nuclei (AGNs) due to gravitational drag and in situ star formation. However, clear evidence …

Compact objects (COs) can exist and evolve in an active galactic nuclei (AGN) disk,
triggering a series of attractive CO-related multimessenger events around a supermassive …

Long and short γ-ray bursts (GRBs) are traditionally associated with galactic environments,
where circumburst densities are small or moderate (few to hundreds of protons per cubic …

Accretion disks of active galactic nuclei (AGNs) have been proposed as promising sites for
producing both (stellar-mass) compact object mergers and extreme mass ratio inspirals …