Relativistic Effects on Circumbinary Orbit Stability

Abstract With n -body simulations and analytic approximations, we study the dynamics and stability of low-eccentricity misaligned test particles around binary systems with varying mass fraction and eccentricity. General relativity (GR) plays a primary role in determining the motion of an outer particle, since it drives apsidal precession of the binary orbit. The effects of GR can drive particle instability close to the binary orbit, depending upon the binary parameters and the initial inclination of the particle. For the binary parameters we consider, we find instability up to a semimajor axis of about 8 a b , where a b is the binary semimajor axis. In particular, we identify and analyze three different regions of instability that are driven by GR in the phase plane of the initial semimajor axis and the initial inclination of the particle. The results have implications for circumbinary orbits and circumbinary disks on all scales, but are particularly important around supermassive black hole binaries where the effects of GR can be strong.