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 derive an analytic phenomenological expression that predicts the final mass of the black-hole rem...
We discuss the properties of the effective-one-body (EOB) multipolar gravitational waveform emitted ...
We adapt a method of matching post-Newtonian and black-hole-perturbation theories on a timelike surf...
Combining recent techniques giving non-perturbative re-summed estimates of the damping and conservat...
Using two recent techniques giving non-perturbative re-summed estimates of the damping and of the co...
We study the coalescence of non-spinning binary black holes from the innermost stable circular orbit...
We discuss the transition from quasi-circular inspiral to plunge of a system of two nonrotating blac...
We study the transition from inspiral to plunge in general relativity by computing gravitational wav...
31 pages, 7 tables, and 13 figuresWe investigate the non-adiabatic dynamics of spinning black hole b...
Binary black holes are the most promising candidate sources for the first generation of earth-based ...
We investigate the dynamics and gravitational-wave (GW) emission in the binary merger of equal-mass ...
We present preliminary results from self-consistent, high resolution direct N-body simulations of ma...
Spectacular breakthroughs in numerical relativity now make it possible to compute spacetime dynamic...
We map the general relativistic two-body problem onto that of a test particle moving in an effective...
Over the last few years enormous progress has been made in the numerical description of the inspiral...
We derive an analytic phenomenological expression that predicts the final mass of the black-hole rem...
We discuss the properties of the effective-one-body (EOB) multipolar gravitational waveform emitted ...
We adapt a method of matching post-Newtonian and black-hole-perturbation theories on a timelike surf...
Combining recent techniques giving non-perturbative re-summed estimates of the damping and conservat...
Using two recent techniques giving non-perturbative re-summed estimates of the damping and of the co...
We study the coalescence of non-spinning binary black holes from the innermost stable circular orbit...
We discuss the transition from quasi-circular inspiral to plunge of a system of two nonrotating blac...
We study the transition from inspiral to plunge in general relativity by computing gravitational wav...
31 pages, 7 tables, and 13 figuresWe investigate the non-adiabatic dynamics of spinning black hole b...
Binary black holes are the most promising candidate sources for the first generation of earth-based ...
We investigate the dynamics and gravitational-wave (GW) emission in the binary merger of equal-mass ...
We present preliminary results from self-consistent, high resolution direct N-body simulations of ma...
Spectacular breakthroughs in numerical relativity now make it possible to compute spacetime dynamic...
We map the general relativistic two-body problem onto that of a test particle moving in an effective...
Over the last few years enormous progress has been made in the numerical description of the inspiral...
We derive an analytic phenomenological expression that predicts the final mass of the black-hole rem...
We discuss the properties of the effective-one-body (EOB) multipolar gravitational waveform emitted ...
We adapt a method of matching post-Newtonian and black-hole-perturbation theories on a timelike surf...
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