Using the first law of binary black-hole mechanics, we compute the binding energy E and total angular momentum J of two non-spinning compact objects moving on circular orbits with frequency Omega, at leading order beyond the test-particle approximation. By minimizing E(Omega) we recover the exact frequency shift of the Schwarzschild innermost stable circular orbit induced by the conservative piece of the gravitational self-force. Comparing our results for the coordinate invariant relation E(J) to those recently obtained from numerical simulations of comparable-mass non-spinning black-hole binaries, we find a remarkably good agreement, even in the strong-field regime. Our findings confirm that the domain of validity of perturbative calculations may extend well beyond the extreme mass-ratio limit.
@article{arxiv.1111.5609,
title = {Gravitational Self-Force Correction to the Binding Energy of Compact Binary Systems},
author = {Alexandre Le Tiec and Enrico Barausse and Alessandra Buonanno},
journal= {arXiv preprint arXiv:1111.5609},
year = {2012}
}