177 citations · 1.4k across the 21 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…
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…
Non-Gaussianity in the Cosmic Microwave Background Induced by Dipolar Dark Matter
Luc Blanchet, David Langlois, Alexandre Le Tiec +1
In previous work [L. Blanchet and A. Le Tiec, Phys. Rev. D 80, 023524 (2009)], motivated by the phenomenology of dark matter at galactic scales, a model of dipolar dark matter (DDM…
Relativistic MOND theory based on the Khronon scalar field
Luc Blanchet, Sylvain Marsat
We investigate a model of modified gravity recovering the modified Newtonian dynamics (MOND) in the non-relativistic limit, based on the introduction of a preferred time foliation…
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…