Gravitational Ionization: A Chaotic Net in the Kepler System
arXiv:gr-qc/9608054 · doi:10.1088/0264-9381/14/3/013
Abstract
The long term nonlinear dynamics of a Keplerian binary system under the combined influences of gravitational radiation damping and external tidal perturbations is analyzed. Gravitational radiation reaction leads the binary system towards eventual collapse, while the external periodic perturbations could lead to the ionization of the system via Arnold diffusion. When these two opposing tendencies nearly balance each other, interesting chaotic behavior occurs that is briefly studied in this paper. It is possible to show that periodic orbits can exist in this system for sufficiently small damping. Moreover, we employ the method of averaging to investigate the phenomenon of capture into resonance.
REVTEX Style, Submitted
References in corpus (2)
Cited by in corpus (16)
- Detecting stochastic gravitational waves with binary resonance
- Chaos in pp-wave spacetimes
- Delay Equations and Radiation Damping
- Dynamical Friction and Resonance Trapping in Planetary Systems
- Chaotic motion in pp-wave spacetimes
- Gravitational Radiation Damping and the Three-Body Problem
- Evolutionary Dynamics While Trapped in Resonance: A Keplerian Binary System Perturbed by Gravitational Radiation
- Chaos in the Kepler System
- Sustained resonance: a binary system perturbed by gravitational radiation
- Chaos in the Hill system
- Energy-momentum and asymptotic geometry
- Homoclinic crossing in open systems: Chaos in periodically perturbed monopole plus quadrupolelike potentials
- Chaotic motion in Kundt spacetimes
- Partial Averaging Near a Resonance in Planetary Dynamics
- Partial Averaging and Resonance Trapping in a Restricted Three-Body System
- Resonant Locking Between Binary Systems Induced by Gravitational Waves