[HTML][HTML] Astrophysics with the laser interferometer space antenna
P Amaro-Seoane, J Andrews, M Arca Sedda… - Living Reviews in …, 2023 - Springer
Abstract The Laser Interferometer Space Antenna (LISA) will be a transformative experiment
for gravitational wave astronomy, and, as such, it will offer unique opportunities to address …
for gravitational wave astronomy, and, as such, it will offer unique opportunities to address …
Black holes, gravitational waves and fundamental physics: a roadmap
L Barack, V Cardoso, S Nissanke… - … and quantum gravity, 2019 - iopscience.iop.org
70 AIM, UMR 7158, CEA/DRF, CNRS, Université Paris Diderot, Irfu/Service d'Astrophysique,
Centre de Saclay, FR-91191 Gif-sur-Yvette, France
Centre de Saclay, FR-91191 Gif-sur-Yvette, France
[HTML][HTML] Formation and evolution of compact-object binaries in AGN disks
The astrophysical origin of gravitational wave (GW) events discovered by LIGO/VIRGO
remains an outstanding puzzle. In active galactic nuclei (AGNs), compact-object binaries …
remains an outstanding puzzle. In active galactic nuclei (AGNs), compact-object binaries …
Constraining stellar-mass black hole mergers in AGN disks detectable with LIGO
B McKernan, KES Ford, J Bellovary… - The Astrophysical …, 2018 - iopscience.iop.org
Black hole (BH) mergers detectable with the Laser Interferometer Gravitational-wave
Observatory (LIGO) can occur in active galactic nucleus (AGN) disks. Here we parameterize …
Observatory (LIGO) can occur in active galactic nucleus (AGN) disks. Here we parameterize …
Stellar evolution in AGN disks
M Cantiello, AS Jermyn, DNC Lin - The Astrophysical Journal, 2021 - iopscience.iop.org
Active galactic nuclei (AGNs) are powered by geometrically thin accretion disks surrounding
a central supermassive black hole. Here we explore the evolution of stars embedded in …
a central supermassive black hole. Here we explore the evolution of stars embedded in …
Formation rate of extreme mass ratio inspirals in active galactic nuclei
Extreme mass ratio inspirals (EMRIs) are important sources for space-borne gravitational
wave detectors, such as the laser interferometer space antenna and TianQin. Previous EMRI …
wave detectors, such as the laser interferometer space antenna and TianQin. Previous EMRI …
Capture of stars into gaseous discs around massive black holes: alignment, circularization, and growth
A Generozov, HB Perets - Monthly Notices of the Royal …, 2023 - academic.oup.com
The majority of massive black holes (MBHs) likely hosted gas discs during their lifetimes.
These could either be long-lived active galactic nuclei (AGN) discs, or shorter-lived discs …
These could either be long-lived active galactic nuclei (AGN) discs, or shorter-lived discs …
Stellar/BH population in AGN discs: direct binary formation from capture objects in nuclei clusters
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 …
merger of binary black holes. The population of massive stars and black holes in AGN discs …
The host galaxies of tidal disruption events
Abstract Recent studies of Tidal Disruption Events (TDEs) have revealed unexpected
correlations between the TDE rate and the large-scale properties of the host galaxies. In this …
correlations between the TDE rate and the large-scale properties of the host galaxies. In this …
Aligning nuclear cluster orbits with an active galactic nucleus accretion disc
Active galactic nuclei (AGN) are powered by the accretion of discs of gas on to
supermassive black holes (SMBHs). Stars and stellar remnants orbiting the SMBH in the …
supermassive black holes (SMBHs). Stars and stellar remnants orbiting the SMBH in the …