Abstract
Using the first law of binary black-hole mechanics, we compute the binding energy and total angular momentum of two nonspinning compact objects moving on circular orbits with frequency , at leading order beyond the test-particle approximation. By minimizing 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 to those recently obtained from numerical simulations of comparable-mass nonspinning 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.
- Received 23 November 2011
DOI:https://doi.org/10.1103/PhysRevLett.108.131103
© 2012 American Physical Society