activity
20042024
most citedRelativistic tidal properties of neutron stars

851 citations · 9.6k across the 106 of their papers we have counts for

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Showing 2007Show all

6 papers · 1 filter

gr-qc2007★ 177 cited

Comparing Effective-One-Body gravitational waveforms to accurate numerical data

Thibault Damour, Alessandro Nagar

We continue the program of constructing, within the Effective-One-Body (EOB) approach, high accuracy, faithful analytic waveforms describing the gravitational wave signal emitted b…

gr-qc2007★ 149 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-qc2007★ 4 cited

Analytic approximations, perturbation methods, and their applications

P. Jaranowski, K. G. Arun, L. Barack +33

The paper summarizes the parallel session B3 {\em Analytic approximations, perturbation methods, and their applications} of the GR18 conference. The talks in the session reported n…

gr-qc2007★ 241 cited

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

Thibault Damour, Alessandro Nagar

We address the problem of constructing high-accuracy, faithful analytic waveforms describing the gravitational wave signal emitted by inspiralling and coalescing binary black holes…

gr-qc2007★ 73 cited

Final spin of a coalescing black-hole binary: an Effective-One-Body approach

Thibault Damour, Alessandro Nagar

We update the analytical estimate of the final spin of a coalescing black-hole binary derived within the Effective-One-Body (EOB) approach. We consider unequal-mass non-spinning bl…

gr-qc2007★ 79 cited

Gravitational Waves from Nonlinear Couplings of Radial and Polar Nonradial Modes in Relativistic Stars

Andrea Passamonti, Nikolaos Stergioulas, Alessandro Nagar

The post-bounce oscillations of newly-born relativistic stars are expected to lead to gravitational-wave emission through the excitation of nonradial oscillation modes. At the same…