activity
20012008
most citedAccurate evolutions of inspiralling neutron-star binaries: prompt and delayed collapse to black hole

378 citations · 2k across the 14 of their papers we have counts for

collaborators

17 papers

gr-qc2008117 cited

On the ergoregion instability in rotating gravastars

Cecilia B. M. H. Chirenti, Luciano Rezzolla

The ergoregion instability is known to affect very compact objects that rotate very rapidly and do not possess a horizon. We present here a detailed analysis on the relevance of th…

gr-qc2008378 cited

Accurate evolutions of inspiralling neutron-star binaries: prompt and delayed collapse to black hole

Luca Baiotti, Bruno Giacomazzo, Luciano Rezzolla

Binary neutron-star (BNS) systems represent primary sources for the gravitational-wave (GW) detectors. We present a systematic investigation in full GR of the dynamics and GW emiss…

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-qc2007225 cited

On the final spin from the coalescence of two black holes

Luciano Rezzolla, Enrico Barausse, Ernst Nils Dorband +4

We provide a compact analytic formula to compute the spin of the black hole produced by the coalescence of two black holes. The expression, which uses an analytic fit of numerical-…

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-qc2007121 cited

The influence of the hydrodynamic drag from an accretion torus on extreme mass-ratio inspirals

E. Barausse, L. Rezzolla

We have studied extreme mass-ratio inspirals (EMRIs) in spacetimes containing a rotating black hole and a non self-gravitating torus with constant specific angular momentum. We hav…