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 …

Despite solid theoretical and observational grounds for the pairing of supermassive black
holes (SMBHs) after galaxy mergers, definitive evidence for the existence of close (sub …

Modern numerical hydrodynamics tools have recently enabled detailed examinations of
binaries accreting from prograde circumbinary discs. These have reframed the current …

We present a suite of high-resolution hydrodynamic simulations of binaries immersed in
circumbinary accretion discs (CBDs). For the first time, we investigate the preferential …

The occurrence of dual active galactic nuclei (AGN) on scales of a few tens of kpc can be
used to study merger-induced accretion on massive black holes (MBHs) and to derive clues …

The study of the interaction of a massive black hole binary with its gaseous environment is
crucial in order to be able to predict merger rates and possible electromagnetic counterparts …

Galactic bars are prominent dynamical structures within disk galaxies whose size, formation
time, strength, and pattern speed influence the dynamical evolution of their hosts' galaxies …

We analyse the effect of stochastic torque fluctuations on the orbital evolution and the
gravitational wave (GW) emission of gas-embedded sources with intermediate and extreme …

We examine expected effective spin () and orbital eccentricity () correlations for a population
of observable equal-mass massive black hole binaries (MBHBs) with total redshifted mass …

In this study of the 'Resolving supermAssive Black hole Binaries In galacTic hydrodynamical
Simulations'(RABBITS) series, we focus on the hardening and coalescing process of …