Abstract
The innermost stable circular orbit (ISCO) of a test particle around a Schwarzschild black hole of mass has (areal) radius . If the particle is endowed with mass , it experiences a gravitational self-force whose conservative piece alters the location of the ISCO. Here we calculate the resulting shifts and in the ISCO’s radius and frequency, at leading order in the mass ratio . We obtain, in the Lorenz gauge, and . We discuss the implications of our result within the context of the extreme-mass-ratio binary inspiral problem.
- Received 3 February 2009
DOI:https://doi.org/10.1103/PhysRevLett.102.191101
©2009 American Physical Society