Using two recent techniques giving non-perturbative re-summed estimates of the damping and of the conservative part of the dynamics of two-body systems, we describe the transition between adiabatic inspiral and plunge in binary non-spinning black holes moving along quasi-circular orbits
We present a multipolar analysis of the gravitational recoil computed in recent numerical simulation...
The end state of a coalescing binary of compact objects depends strongly on the final total mass M a...
Gravitational waves emitted during the inspiral, plunge and merger of a black hole binary carry line...
Using two recent techniques giving non-perturbative re-summed estimates of the damping and of the co...
Combining recent techniques giving non-perturbative re-summed estimates of the damping and conservat...
31 pages, 7 tables, and 13 figuresWe investigate the non-adiabatic dynamics of spinning black hole b...
We study the coalescence of non-spinning binary black holes from the innermost stable circular orbit...
We study the transition from inspiral to plunge in general relativity by computing gravitational wav...
We study the fully nonlinear dynamical evolution of binary black hole data, whose orbital parameters...
We discuss the transition from quasi-circular inspiral to plunge of a system of two nonrotating blac...
Over the last few years enormous progress has been made in the numerical description of the inspiral...
International audienceThe merger phase of binary black hole coalescences is a transient between an i...
We present a multipolar analysis of the gravitational recoil computed in recent numerical simulation...
The end state of a coalescing binary of compact objects depends strongly on the final total mass M a...
Gravitational waves emitted during the inspiral, plunge and merger of a black hole binary carry line...
Using two recent techniques giving non-perturbative re-summed estimates of the damping and of the co...
Combining recent techniques giving non-perturbative re-summed estimates of the damping and conservat...
31 pages, 7 tables, and 13 figuresWe investigate the non-adiabatic dynamics of spinning black hole b...
We study the coalescence of non-spinning binary black holes from the innermost stable circular orbit...
We study the transition from inspiral to plunge in general relativity by computing gravitational wav...
We study the fully nonlinear dynamical evolution of binary black hole data, whose orbital parameters...
We discuss the transition from quasi-circular inspiral to plunge of a system of two nonrotating blac...
Over the last few years enormous progress has been made in the numerical description of the inspiral...
International audienceThe merger phase of binary black hole coalescences is a transient between an i...
We present a multipolar analysis of the gravitational recoil computed in recent numerical simulation...
The end state of a coalescing binary of compact objects depends strongly on the final total mass M a...
Gravitational waves emitted during the inspiral, plunge and merger of a black hole binary carry line...
DOI
Add to ORKG