70 AIM, UMR 7158, CEA/DRF, CNRS, Université Paris Diderot, Irfu/Service d'Astrophysique,
Centre de Saclay, FR-91191 Gif-sur-Yvette, France

The detection of gravitational waves from binary black-hole mergers by the LIGO–Virgo
Collaboration marks the dawn of an era when general-relativistic dynamics in its most …

Much of the success of gravitational-wave astronomy rests on perturbation theory.
Historically, perturbative analysis of gravitational-wave sources has largely focused on post …

Recently, the gravitational scattering of two black holes (BHs) treated at the leading order in
the weak-field, or post-Minkowskian (PM), approximation to general relativity has been …

We compute the linear metric perturbation to a Schwarzschild black hole generated by a
spinning compact object, specializing to circular equatorial orbits with an (anti-) aligned spin …

We investigate the dynamics of spinning binaries of compact objects at the next-to-leading
order in the quadratic-in-spin effects, which corresponds to the third post-Newtonian order …

Using the self-force approach, we present the premier first-post-adiabatic accuracy
formalism for modeling compact binaries in theories with a massless scalar field …

We establish a new relation between classical observables for scattering and bound orbits
of a massive probe particle in a Kerr background. We find an exact representation of the …

LISA, the Laser Interferometer Space Antenna, will usher in a new era in gravitational-wave
astronomy. As the first anticipated space-based gravitational-wave detector, it will expand …

We complete the post-Newtonian (PN) prediction at the 3.5 PN order for the spin
contributions to the gravitational waveforms emitted by inspiraling compact binaries, in the …