Publications (21)
Tidal contributions to the full gravitational waveform to the second-and-a-half post-Newtonian order
Eve Dones, Quentin Henry, Laura Bernard
This paper describes the different steps to include the adiabatic tidal effects to the gravitational waveform amplitude for quasi-circular non-spinning compact binaries up to the s…
ESIGMAHM: An Eccentric, Spinning inspiral-merger-ringdown waveform model with Higher Modes for the detection and characterization of binary black holes
Kaushik Paul, Akash Maurya, Quentin Henry +5
We present a time-domain inspiral-merger-ringdowm (IMR) waveform model ESIGMAHM constructed within a framework we named ESIGMA for coalescing binaries of spinning black holes on mo…
Tidal effects in the gravitational-wave phase evolution of compact binary systems to next-to-next-to-leading post-Newtonian order
Quentin Henry, Guillaume Faye, Luc Blanchet
We compute the gravitational-wave (GW) energy flux up to the next-to-next-to-leading (NNL) order of tidal effects in a spinless compact binary system on quasi-circular orbits. Star…
Spin contributions to the gravitational-waveform modes for spin-aligned binaries at the 3.5PN order
Quentin Henry, Sylvain Marsat, Mohammed Khalil
We complete the post-Newtonian (PN) prediction at the 3.5PN order for the spin contributions to the gravitational waveforms emitted by inspiraling compact binaries, in the case of…
Tidal effects in the equations of motion of compact binary systems to next-to-next-to-leading post-Newtonian order
Quentin Henry, Guillaume Faye, Luc Blanchet
As a first step in the computation of the orbital phase evolution of spinless compact binaries including tidal effects up to the next-to-next-to-leading (NNL) order, we obtain the…
Conservative (failed)-tail effects at the fifth post-Newtonian order
Quentin Henry, François Larrouturou
This work deals with the tail and ``failed'' tail sectors of the conservative dynamics for compact binary systems at the 5PN order. We employ the Fokker Lagrangian method with dime…