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Black holes, gravitational waves and fundamental physics: a roadmap
AIM, UMR 7158, CEA/DRF, CNRS, Université Paris Diderot, Irfu/Service d'Astrophysique,
Centre de Saclay, FR-91191 Gif-sur-Yvette, France
Centre de Saclay, FR-91191 Gif-sur-Yvette, France
Self-force and radiation reaction in general relativity
L Barack, A Pound - Reports on Progress in Physics, 2018 - iopscience.iop.org
The detection of gravitational waves from binary black-hole mergers by the LIGO–Virgo
Collaboration marks the dawn of an era when general-relativistic dynamics in its most …
Collaboration marks the dawn of an era when general-relativistic dynamics in its most …
Scattering in black hole backgrounds and higher-spin amplitudes. Part II
A bstract We continue to investigate correspondences between, on the one hand, scattering
amplitudes for massive higher-spin particles and gravitons in appropriate quantum-to …
amplitudes for massive higher-spin particles and gravitons in appropriate quantum-to …
High-energy gravitational scattering and the general relativistic two-body problem
T Damour - Physical Review D, 2018 - APS
A technique for translating the classical scattering function of two gravitationally interacting
bodies into a corresponding (effective one-body) Hamiltonian description has been recently …
bodies into a corresponding (effective one-body) Hamiltonian description has been recently …
The effective field theorist's approach to gravitational dynamics
We review the effective field theory (EFT) approach to gravitational dynamics. We focus on
extended objects in long-wavelength backgrounds and gravitational wave emission from …
extended objects in long-wavelength backgrounds and gravitational wave emission from …
Post-Newtonian theory for gravitational waves
To be observed and analyzed by the network of current gravitational-wave detectors (LIGO,
Virgo, KAGRA), and in anticipation of future third generation ground-based (Einstein …
Virgo, KAGRA), and in anticipation of future third generation ground-based (Einstein …
Effective field theory for extreme mass ratio binaries
We derive an effective field theory describing a pair of gravitationally interacting point
particles in an expansion in their mass ratio, also known as the self-force (SF) expansion …
particles in an expansion in their mass ratio, also known as the self-force (SF) expansion …
Enhancing the SEOBNRv5 effective-one-body waveform model with second-order gravitational self-force fluxes
We leverage recent breakthrough calculations using second-order gravitational self-force
(2GSF) theory to improve both the gravitational-mode amplitudes and radiation-reaction …
(2GSF) theory to improve both the gravitational-mode amplitudes and radiation-reaction …
Energetics and scattering of gravitational two-body systems at fourth post-Minkowskian order
Upcoming observational runs of the LIGO-Virgo-KAGRA Collaboration and future
gravitational-wave (GW) detectors on the ground and in space require waveform models …
gravitational-wave (GW) detectors on the ground and in space require waveform models …
Black hole perturbation theory and gravitational self-force
Much of the success of gravitational-wave astronomy rests on perturbation theory.
Historically, perturbative analysis of gravitational-wave sources has largely focused on post …
Historically, perturbative analysis of gravitational-wave sources has largely focused on post …