activity
19972009
most citedOn the determination of the last stable orbit for circular general relativistic binaries at the third post-Newtonian approximation

478 citations · 792 across the 8 of their papers we have counts for

collaborators

8 papers

gr-qc2009★ 7 cited

Post-Newtonian methods: Analytic results on the binary problem

Gerhard Schäfer

A detailed account is given on approximation schemes to the Einstein theory of general relativity where the iteration starts from the Newton theory of gravity. Two different coordi…

gr-qc2008★ 6 cited

Binary Black Hole Coalescence in Semi-Analytic Puncture Evolution

Achamveedu Gopakumar, Gerhard Schaefer

Binary black-hole coalescence is treated semi-analytically by a novel approach. Our prescription employs the conservative Skeleton Hamiltonian that describes orbiting Brill-Lindqui…

gr-qc2007

Post-Newtonian Approximations, Compact Binaries, and Strong-Field Tests of Gravity

Luc Blanchet, L P Grishchuk, Gerhard Schaefer

This is an extended summary of the two parallel sessions held at MG11: PPN1 ``Strong Gravity and Binaries'' (chaired by L.B. and L.G.) and PPN2 ``Post-Newtonian Dynamics in Binary…

gr-qc2003★ 18 cited

A skeleton approximate solution of the Einstein field equations for multiple black-hole systems

G. Faye, P. Jaranowski, G. Schaefer

An approximate analytical and non-linear solution of the Einstein field equations is derived for a system of multiple non-rotating black holes. The associated space-time has the sa…

gr-qc2003★ 12 cited

Optimizing the third-and-a-half post-Newtonian gravitational radiation-reaction force for numerical simulations

Guillaume Faye, Gerhard Schaefer

The gravitational radiation-reaction force acting on perfect fluids at 3.5 post-Newtonian order is cast into a form which is directly applicable to numerical simulations. Extensive…

gr-qc2001★ 3 cited

Can Schwarzschildean gravitational fields suppress gravitational waves?

Edward Malec, Gerhard Schaefer

Gravitational waves in the linear approximation propagate in the Schwarzschild spacetime similarly as electromagnetic waves. A fraction of the radiation scatters off the curvature…