Gravitational wave astronomy is rapidly maturing as a standard tool to study astrophysics, astronomy, and cosmology. However, to fully realize the promise of gravitational waves, accurate wave templates computed either numerically or using analytical approximations are essential, as exact solutions to the highly nonlinear Einstein field equations from which templates are derived are intractable for realistic systems. In this thesis, we present progress made in computing observables from an effective field theory framework of gravity applicable to the early stages of binary mergers. We first tackle next-to-leading order spin dependent contributions to the equations of motion in the post-Newtonian expansion, and use these results to derive...
We complete the post-Newtonian (PN) prediction at the 3.5PN order for thespin contributions to the g...
Motivated by the search for gravitational waves emitted by binary black holes, we investigate the gr...
We compute the spin-tidal couplings that affect the dynamics of two orbiting bodies at the leading o...
Gravitational wave astronomy is rapidly maturing as a standard tool to study astrophysics, astronomy...
International audienceWe implement the effective field theory for gravitating spinning objects in th...
We derive spin-orbit coupling effects on the gravitational field and equations of motion of compact ...
We report on recent results obtained in the post-Newtonian framework for the modelling of the gravit...
Gravitational waves provide us with a new window into our Universe, and have already been used to pl...
The linear- and quadratic-in-spin contributions to the binding potential and gravitational-wave flux...
Using the gravitational potential and source multipole moments bilinear in the spins, first computed...
International audienceTo be observed and analyzed by the network of gravitational wave detectors on ...
Gravitational waves contain tail effects which are due to the back-scattering of linear waves in the...
To be observed and analyzed by the network of gravitational wave detectors on ground (LIGO, VIRGO, e...
Compact binaries in hyperbolic orbits are plausible gravitational-wave (GW) sources for the upcoming...
We calculate the gravitational waveform for spinning, precessing compact binary inspirals through se...
We complete the post-Newtonian (PN) prediction at the 3.5PN order for thespin contributions to the g...
Motivated by the search for gravitational waves emitted by binary black holes, we investigate the gr...
We compute the spin-tidal couplings that affect the dynamics of two orbiting bodies at the leading o...
Gravitational wave astronomy is rapidly maturing as a standard tool to study astrophysics, astronomy...
International audienceWe implement the effective field theory for gravitating spinning objects in th...
We derive spin-orbit coupling effects on the gravitational field and equations of motion of compact ...
We report on recent results obtained in the post-Newtonian framework for the modelling of the gravit...
Gravitational waves provide us with a new window into our Universe, and have already been used to pl...
The linear- and quadratic-in-spin contributions to the binding potential and gravitational-wave flux...
Using the gravitational potential and source multipole moments bilinear in the spins, first computed...
International audienceTo be observed and analyzed by the network of gravitational wave detectors on ...
Gravitational waves contain tail effects which are due to the back-scattering of linear waves in the...
To be observed and analyzed by the network of gravitational wave detectors on ground (LIGO, VIRGO, e...
Compact binaries in hyperbolic orbits are plausible gravitational-wave (GW) sources for the upcoming...
We calculate the gravitational waveform for spinning, precessing compact binary inspirals through se...
We complete the post-Newtonian (PN) prediction at the 3.5PN order for thespin contributions to the g...
Motivated by the search for gravitational waves emitted by binary black holes, we investigate the gr...
We compute the spin-tidal couplings that affect the dynamics of two orbiting bodies at the leading o...