Gravitational radiation from post-Newtonian sources and inspiralling compact binaries
L Blanchet - Living reviews in relativity, 2014 - Springer
To be observed and analyzed by the network of gravitational wave detectors on ground
(LIGO, VIRGO, etc.) and by the future detectors in space (e LISA, etc.), inspiralling compact …
(LIGO, VIRGO, etc.) and by the future detectors in space (e LISA, etc.), inspiralling compact …
Black-hole binaries, gravitational waves, and numerical relativity
Understanding the predictions of general relativity for the dynamical interactions of two black
holes has been a long-standing unsolved problem in theoretical physics. Black-hole …
holes has been a long-standing unsolved problem in theoretical physics. Black-hole …
The Einstein Toolkit: a community computational infrastructure for relativistic astrophysics
Abstract We describe the Einstein Toolkit, a community-driven, freely accessible
computational infrastructure intended for use in numerical relativity, relativistic astrophysics …
computational infrastructure intended for use in numerical relativity, relativistic astrophysics …
Matching post-Newtonian and numerical relativity waveforms: Systematic errors and a new phenomenological model for nonprecessing black hole binaries
L Santamaria, F Ohme, P Ajith, B Brügmann… - Physical Review D …, 2010 - APS
We present a new phenomenological gravitational waveform model for the inspiral and
coalescence of nonprecessing spinning black hole binaries. Our approach is based on a …
coalescence of nonprecessing spinning black hole binaries. Our approach is based on a …
Template bank for gravitational waveforms from coalescing binary black holes:<? format?> Nonspinning binaries
Gravitational waveforms from the inspiral and ring-down stages of the binary black-hole
coalescences can be modeled accurately by approximation/perturbation techniques in …
coalescences can be modeled accurately by approximation/perturbation techniques in …
Higher-order spin effects in the amplitude and phase of gravitational waveforms emitted<? format?> by inspiraling compact binaries: Ready-to-use gravitational …
We provide ready-to-use time-domain gravitational waveforms for spinning compact binaries
with precession effects through 1.5 post-Newtonian (PN) order in amplitude, and compute …
with precession effects through 1.5 post-Newtonian (PN) order in amplitude, and compute …
Closed-form tidal approximants for binary neutron star gravitational waveforms constructed from high-resolution numerical relativity simulations
We construct closed-form gravitational waveforms (GWs) with tidal effects for the
coalescence of binary neutron stars. The method relies on a new set of eccentricity-reduced …
coalescence of binary neutron stars. The method relies on a new set of eccentricity-reduced …
The third post-Newtonian gravitational wave polarizations and associated spherical harmonic modes for inspiralling compact binaries in quasi-circular orbits
The gravitational waveform (GWF) generated by inspiralling compact binaries moving in
quasi-circular orbits is computed at the third post-Newtonian (3PN) approximation to general …
quasi-circular orbits is computed at the third post-Newtonian (3PN) approximation to general …
Tracking the precession of compact binaries from their gravitational-wave signal
We present a simple method to track the precession of a black-hole-binary system during the
inspiral, using only information from the gravitational-wave (GW) signal. Our method consists …
inspiral, using only information from the gravitational-wave (GW) signal. Our method consists …
The RIT binary black hole simulations catalog
The RIT numerical relativity group is releasing a public catalog of black-hole-binary
waveforms. The initial release of the catalog consists of 126 recent simulations that include …
waveforms. The initial release of the catalog consists of 126 recent simulations that include …