activity
20042008
most citedPhenomenological template family for black-hole coalescence waveforms

332 citations · 874 across the 7 of their papers we have counts for

collaborators

8 papers

gr-qc200834 cited

Constraint-preserving boundary treatment for a harmonic formulation of the Einstein equations

Jennifer Seiler, Bela Szilagyi, Denis Pollney +1

We present a set of well-posed constraint-preserving boundary conditions for a first-order in time, second-order in space, harmonic formulation of the Einstein equations. The bound…

gr-qc2007149 cited

Faithful Effective-One-Body waveforms of equal-mass coalescing black-hole binaries

Thibault Damour, Alessandro Nagar, Ernst Nils Dorband +2

We continue the program of constructing, within the Effective-One-Body (EOB) approach, high-accuracy analytic waveforms describing the signal emitted by inspiralling and coalescing…

gr-qc200759 cited

Implementation of standard testbeds for numerical relativity

M. C. Babiuc, S. Husa, D. Alic +8

We discuss results that have been obtained from the implementation of the initial round of testbeds for numerical relativity which was proposed in the first paper of the Apples wit…

gr-qc2007222 cited

Recoil velocities from equal-mass binary black-hole mergers: a systematic investigation of spin-orbit aligned configurations

Denis Pollney, Christian Reisswig, Luciano Rezzolla +8

Binary black-hole systems with spins aligned with the orbital angular momentum are of special interest, as studies indicate that this configuration is preferred in nature. If the s…

gr-qc200773 cited

Excision without excision: the relativistic turducken

David Brown, Olivier Sarbach, Erik Schnetter +4

to turducken (turduckens, turduckening, turduckened, turduckened) [math.]: To stuff a black hole. We analyze and apply an alternative to black hole excision based on smoothing the…

gr-qc2007332 cited

Phenomenological template family for black-hole coalescence waveforms

P. Ajith, S. Babak, Y. Chen +15

Recent progress in numerical relativity has enabled us to model the non-perturbative merger phase of the binary black-hole coalescence problem. Based on these results, we propose a…