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 …

We review recent works on the dynamics of circumbinary accretion, including time variability,
angular momentum transfer between the disk and the binary, and the secular evolution of …

We present the to-date largest parameter space exploration of binaries in circumbinary discs
(CBDs), deriving orbital evolution prescriptions for eccentric, unequal mass binaries from our …

Supermassive black hole binaries source gravitational waves measured by Pulsar Timing
Arrays. The frequency spectrum of this stochastic background is predicted more precisely …

Coalescing massive black hole binaries (MBHBs) of, forming in the aftermath of galaxy
mergers, are primary targets of the space mission LISA, the Laser Interferometer Space …

We characterize the population of wandering black holes, defined as those physically offset
from their halo centres, in the romulus cosmological simulations. Unlike most other currently …

The stochastic gravitational-wave background is imprinted on the times of arrival of radio
pulses from millisecond pulsars. Traditional pulsar timing analyses fit a timing model to each …

We study supermassive black hole (SMBH) binary eccentricity of equal-mass galaxy
mergers in N-body simulations with the ketju code, which combines the gadget-4 fast …

Coalescing supermassive black hole binaries (BHBs) are expected to be the loudest
sources of gravitational waves (GWs) in the Universe. Detection rates for ground or space …

Using few-body simulations, we investigate the evolution of supermassive black holes
(SMBHs) in galaxies (M*= 1010–1012 M⊙ at z= 0) at 0< z< 4. Following galaxy merger trees …