On the relationship between instability and Lyapunov times for the 3-body problem
arXiv:0810.5461 · doi:10.1111/j.1365-2966.2008.14149.x
Abstract
In this study we consider the relationship between the survival time and the Lyapunov time for 3-body systems. It is shown that the Sitnikov problem exhibits a two-part power law relationship as demonstrated previously for the general 3-body problem. Using an approximate Poincare map on an appropriate surface of section, we delineate escape regions in a domain of initial conditions and use these regions to analytically obtain a new functional relationship between the Lyapunov time and the survival time for the 3-body problem. The marginal probability distributions of the Lyapunov and survival times are discussed and we show that the probability density function of Lyapunov times for the Sitnikov problem is similar to that for the general 3-body problem.
arXiv comment9 pages, 19 figures, accepted for publication in MNRAS
References in corpus (2)
Cited by in corpus (9)
- Three Body Resonance Overlap in Closely Spaced Multiple Planet Systems
- On the minimal accuracy required for simulating self-gravitating systems by means of direct N-body methods
- Hamiltonian intermittency and Lévy flights in the three-body problem
- The Kepler map in the three-body problem
- Chaos in self-gravitating many-body systems: Lyapunov time dependence of and the influence of general relativity
- Disruption of the three-body gravitational systems: Lifetime statistics
- Isles of regularity in a sea of chaos amid the gravitational three-body problem
- On the inherent self-excited macroscopic randomness of chaotic three-body system
- Shadowing unstable orbits of the Sitnikov elliptic 3-body problem