Add to ORKGUsing the NRGR effective field theory formalism we calculate the remaining source multipole moments necessary to obtain the spin contributions to the gravitational wave amplitude to 2.5 Post-Newtonian (PN) order. We also reproduce the tail contribution to the waveform linear in spin at 2.5PN arising from the nonlinear interaction between the current quadrupole and the mass monopole
includes the correction of an erratum to be published in Phys. Rev. DInternational audienceMotivated...
International audienceThis paper is motivated by the need to improve the post-Newtonian (PN) amplitu...
includes the correction of an erratum to be published in Phys. Rev. DInternational audienceMotivated...
Using the NRGR effective field theory formalism we calculate the remaining source multipole moments ...
Using effective field theory techniques we calculate the source multipole moments needed to obtain t...
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...
Motivated by the search for gravitational waves emitted by binary black holes, we investigate the gr...
includes the correction of an erratum to be published in Phys. Rev. DInternational audienceMotivated...
Open Access - IOP selectThis paper is motivated by the need to improve the post-Newtonian (PN) ampli...
includes the correction of an erratum to be published in Phys. Rev. DInternational audienceMotivated...
The linear- and quadratic-in-spin contributions to the binding potential and gravitational-wave flux...
We calculate the gravitational waveform for spinning, precessing compact binary inspirals through se...
includes the correction of an erratum to be published in Phys. Rev. DInternational audienceMotivated...
International audienceWe compute the next-to-next-to-leading order spin-orbit contributions in the t...
includes the correction of an erratum to be published in Phys. Rev. DInternational audienceMotivated...
International audienceThis paper is motivated by the need to improve the post-Newtonian (PN) amplitu...
includes the correction of an erratum to be published in Phys. Rev. DInternational audienceMotivated...
Using the NRGR effective field theory formalism we calculate the remaining source multipole moments ...
Using effective field theory techniques we calculate the source multipole moments needed to obtain t...
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...
Motivated by the search for gravitational waves emitted by binary black holes, we investigate the gr...
includes the correction of an erratum to be published in Phys. Rev. DInternational audienceMotivated...
Open Access - IOP selectThis paper is motivated by the need to improve the post-Newtonian (PN) ampli...
includes the correction of an erratum to be published in Phys. Rev. DInternational audienceMotivated...
The linear- and quadratic-in-spin contributions to the binding potential and gravitational-wave flux...
We calculate the gravitational waveform for spinning, precessing compact binary inspirals through se...
includes the correction of an erratum to be published in Phys. Rev. DInternational audienceMotivated...
International audienceWe compute the next-to-next-to-leading order spin-orbit contributions in the t...
includes the correction of an erratum to be published in Phys. Rev. DInternational audienceMotivated...
International audienceThis paper is motivated by the need to improve the post-Newtonian (PN) amplitu...
includes the correction of an erratum to be published in Phys. Rev. DInternational audienceMotivated...