349 citations · 5.4k across the 67 of their papers we have counts for
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Next-to-next-to-leading order spin-orbit effects in the near-zone metric and precession equations of compact binaries
Alejandro Bohé, Sylvain Marsat, Guillaume Faye +1
We extend our previous work devoted to the computation of the next-to-next-to-leading order spin-orbit correction (corresponding to 3.5PN order) in the equations of motion of spinn…
Post-Newtonian prediction for the (2,2) mode of the gravitational wave emitted by compact binaries
Guillaume Faye, Sylvain Marsat, Luc Blanchet +1
We present our 3.5PN computation of the (2,2) mode of the gravitational wave amplitude emitted by compact binaries, on quasi-circular orbits and in the absence of spins. We use the…
Third post-Newtonian spin-orbit effect in the gravitational radiation flux of compact binaries
Luc Blanchet, Alessandra Buonanno, Guillaume Faye
Gravitational waves contain tail effects that are due to the backscattering of linear waves in the curved space-time geometry around the source. The knowledge as well as the accura…
Next-to-next-to-leading order spin-orbit effects in the equations of motion of compact binary systems
Sylvain Marsat, Alejandro Bohe, Guillaume Faye +1
We compute next-to-next-to-leading order spin contributions to the post-Newtonian equations of motion for binaries of compact objects, such as black holes or neutron stars. For max…
Spin effects on gravitational waves from inspiraling compact binaries at second post-Newtonian order
Alessandra Buonanno, Guillaume Faye, Tanja Hinderer
We calculate the gravitational waveform for spinning, precessing compact binary inspirals through second post-Newtonian order in the amplitude. When spins are collinear with the or…
The third and a half post-Newtonian gravitational wave quadrupole mode for quasi-circular inspiralling compact binaries
Guillaume Faye, Sylvain Marsat, Luc Blanchet +1
We compute the quadrupole mode of the gravitational waveform of inspiralling compact binaries at the third and a half post-Newtonian (3.5PN) approximation of general relativity. Th…
Effective action approach to higher-order relativistic tidal interactions in binary systems and their effective one body description
Donato Bini, Thibault Damour, Guillaume Faye
The gravitational-wave signal from inspiralling neutron-star--neutron-star (or black-hole--neutron-star) binaries will be influenced by tidal coupling in the system. An important s…