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 …

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 …

We review the properties of the established Scaling Relations (SRs) of galaxies and active
galactic nuclei (AGN), focusing on their origin and expected evolution back in time, providing …

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 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 …

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 …

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) …

Extreme mass ratio inspirals (EMRIs) occur when stellar-mass compact objects begin a
gravitational wave (GW) driven inspiral into massive black holes. EMRI waveforms can …

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

We model here the merger histories of the supermassive black hole (SMBH) population in
the late stages of a cosmological simulation of a∼ 2× 10 13 M⊙ galaxy group. The …