collaborators

9 papers

astro-ph.HE2025

Gravitational Wave Phase shifts of black hole mergers in AGN Disks

Hiromichi Tagawa, Connar Rowan, János Takátsy +4

Ground-based gravitational wave (GW) detectors have discovered about 200 compact object mergers. The astrophysical origins of these events are highly debated, and it is possible th…

gr-qc2025

Importance of relativistic pericenter precession in identifying the presence of a third body near eccentric binaries

Pankaj Saini, Lorenz Zwick, János Takátsy +5

Many astrophysical processes can produce gravitational wave (GW) sources with significant orbital eccentricity. These binaries emit bursts of gravitational radiation during each pe…

astro-ph.HE2025

Hydrodynamic simulations of black hole evolution in AGN discs II: inclination damping for partially embedded satellites

Henry Whitehead, Connar Rowan, Bence Kocsis

We investigate the evolution of black holes on orbits with small inclinations () to the gaseous discs of active galactic nuclei. We perform 3D adiabatic hydrodynamic s…

astro-ph.HE2025

Hydrodynamic simulations of black hole evolution in AGN discs I: orbital alignment of highly inclined satellites

Connar Rowan, Henry Whitehead, Gaia Fabj +3

The frequency of compact object interactions in AGN discs is naturally tied to the number of objects embedded within it. We investigate the evolution of black holes in the nuclear…

astro-ph.GA2025

Gas meets Kozai: the influence of a gas-rich accretion disc on hierarchical triples undergoing von Zeipel-Lidov-Kozai oscillations

Yubo Su, Connar Rowan, Mor Rozner

Active galactic nuclei (AGNs) consist of a central supermassive black hole (SMBH) embedded in a region with both high gas and stellar densities: the gas is present as a thin accret…

astro-ph.HE2025

Environmental effects in stellar mass gravitational wave sources I: Expected fraction of signals with significant dephasing in the dynamical and AGN channels

Lorenz Zwick, János Takátsy, Pankaj Saini +5

We present the first overview of the expected quantity of signals which will showcase significant gravitational wave phase shifts caused by astrophysical environments, considering…