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19942008
most citedWormholes as Black Hole Foils

249 citations · 1.8k across the 20 of their papers we have counts for

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gr-qc2008205 cited

Effective one body approach to the dynamics of two spinning black holes with next-to-leading order spin-orbit coupling

Thibault Damour, Piotr Jaranowski, Gerhard Schäfer

Using a recent, novel Hamiltonian formulation of the gravitational interaction of spinning binaries, we extend the Effective One Body (EOB) description of the dynamics of two spinn…

gr-qc2008171 cited

Accurate Effective-One-Body waveforms of inspiralling and coalescing black-hole binaries

Thibault Damour, Alessandro Nagar, Mark Hannam +2

The Effective-One-Body (EOB) formalism contains several flexibility parameters, notably , $\vp$ and $\a$. We show here how to jointly constrain the values of these parameters…

gr-qc200857 cited

Introductory lectures on the Effective One Body formalism

Thibault Damour

The Effective One Body (EOB) formalism is an analytical approach which aims at providing an accurate description of the motion and radiation of coalescing binary black holes. We pr…

gr-qc2007177 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-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-qc2007210 cited

Hamiltonian of two spinning compact bodies with next-to-leading order gravitational spin-orbit coupling

Thibault Damour, Piotr Jaranowski, Gerhard Schäfer

A Hamiltonian formulation is given for the gravitational dynamics of two spinning compact bodies to next-to-leading order ( and ) in the spin-orbit interaction. We…