| Abstract: |
In classical Newtonian gravity, the three-body problem is known to be chaotic for general initial data. We investigate the existence of chaos for the three- body problem in general relativity using the first post-Newtonian approxima- tion. Our initial data consists of a third object entering a binary pair and is parameterized by an impact parameter and phase angle. The Hamiltonian equations of motion are integrated using adaptive methods and we extract gauge-independent quantities at infinity. We present results that characterize chaos in general relativity. |