Chaos in a 3-body Self-Gravitating Cosmological Spacetime
arXiv:astro-ph/0607070 · doi:10.1103/PhysRevD.76.104051
Abstract
We investigate the equal-mass 3-body system in general relativistic lineal gravity in the presence of a cosmological constant . The cosmological vacuum energy introduces features that do not have a non-relativistic counterpart, inducing a competing expansion/contraction of spacetime that competes with the gravitational self-attraction of the bodies. We derive a canonical expression for the Hamiltonian of the system and discuss the numerical solution of the resulting equations of motion. As for the system with , we find that the structure of the phase space yields a rich variety of interesting dynamics that can be divided into three distinct regions: annulus, pretzel, and chaotic; the first two being regions of quasi-periodicity while the latter is a region of chaos. However unlike the case, we find that a negative cosmological constant considerably diminishes the amount of chaos in the system, even beyond that of the non-relativistic system. By contrast, a positive cosmological constant considerably enhances the amount of chaos, typically leading to KAM breakdown.
arXiv comment40 pages, 16 figures, Latex
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