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 …

Dense star clusters are spectacular self-gravitating stellar systems in our Galaxy and across
the Universe—in many respects. They populate disks and spheroids of galaxies as well as …

Understanding the formation and growth of supermassive black holes (SMBHs) at high
redshift represents a major challenge for theoretical models. In this work, we investigate the …

Tidal disruption events (TDEs) of stars operated by massive black holes (MBHs) will be
detected in thousands by upcoming facilities such as the Vera Rubin Observatory. In this …

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) …

Third-generation ground-based gravitational wave interferometers, like the Einstein
Telescope (ET), Cosmic Explorer, and the Laser Interferometer Space Antenna (LISA), will …

ABSTRACT A tidal disruption event (TDE) occurs when a star is destroyed by the strong tidal
shear of a massive black hole (MBH). The accumulation of TDE observations over the last …

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 …

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 …

The observation of a population of massive black hole binaries (MBHBs) is key for our
complete understanding of galaxy mergers and for the characterization of the expected …