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Post-Newtonian evolution of massive black hole triplets in galactic nuclei -- III. A robust lower limit to the nHz stochastic background of gravitational waves
Matteo Bonetti, Alberto Sesana, Enrico Barausse +1
Inspiraling massive black-hole binaries (MBHBs) forming in the aftermath of galaxy mergers are expected to be the loudest gravitational-wave (GW) sources relevant for pulsar-timing…
Post-Newtonian evolution of massive black hole triplets in galactic nuclei -- II. Survey of the parameter space
Matteo Bonetti, Francesco Haardt, Alberto Sesana +1
Massive black hole binaries (MBHBs) are expected to form at the centre of merging galaxies during the hierarchical assembly of the cosmic structure, and are expected to be the loud…
About gravitational-wave generation by a three-body system
Matteo Bonetti, Enrico Barausse, Guillaume Faye +2
We highlight some subtleties that affect naive implementations of quadrupolar and octupolar gravitational waveforms from numerically-integrated trajectories of three-body systems.…