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 …

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 …

Massive black hole binaries are predicted to form during the hierarchical assembly of cosmic
structures and will represent the loudest sources of low-frequency gravitational waves (GWs) …

For a pair of supermassive black holes (SMBHs) in the remnant of a dual galaxy merger,
well-known models exist to describe their dynamical evolution until the final coalescence …

ABSTRACT The forthcoming Laser Interferometer Space Antenna (LISA) will probe the
population of coalescing massive black hole (MBH) binaries up to the onset of structure …

We examine massive black hole (MBH) mergers and their associated gravitational wave
signals from the large-volume cosmological simulation Astrid. Astrid includes galaxy …

We analyse how drag forces modify the orbits of objects moving through extended gaseous
distributions. We consider how hydrodynamic (surface area) drag forces and dynamical …

It has recently become possible to zoom-in from cosmological to sub-pc scales in galaxy
simulations to follow accretion onto supermassive black holes (SMBHs). However, at some …

ABSTRACT A long-standing problem in galactic simulations is to resolve the dynamical
friction (DF) force acting on massive black hole particles when their masses are comparable …

ABSTRACT The detection of Intermediate-Mass Black Holes (IMBHs) in dwarf galaxies is
crucial to closing the gap in the wide mass distribution of black holes (to). IMBHs originally …