Noise-Induced Phase Space Transport in Two-Dimensional Hamiltonian Systems
arXiv:astro-ph/9902092 · doi:10.1103/PhysRevE.60.1567
Abstract
First passage time experiments were used to explore the effects of low amplitude noise as a source of accelerated phase space diffusion in two-dimensional Hamiltonian systems, and these effects were then compared with the effects of periodic driving. The objective was to quantify and understand the manner in which ``sticky'' chaotic orbits that, in the absence of perturbations, are confined near regular islands for very long times, can become ``unstuck'' much more quickly when subjected to even very weak perturbations. For both noise and periodic driving, the typical escape time scales logarithmically with the amplitude of the perturbation. For white noise, the details seem unimportant: Additive and multiplicative noise typically have very similar effects, and the presence or absence of a friction related to the noise by a Fluctuation-Dissipation Theorem is also largely irrelevant. Allowing for colored noise can significantly decrease the efficacy of the perturbation, but only when the autocorrelation time becomes so large that there is little power at frequencies comparable to the natural frequencies of the unperturbed orbit. Similarly, periodic driving is relatively inefficient when the driving frequency is not comparable to these natural frequencies. This suggests strongly that noise-induced extrinsic diffusion, like modulational diffusion associated with periodic driving, is a resonance phenomenon. The logarithmic dependence of the escape time on amplitude reflects the fact that the time required for perturbed and unperturbed orbits to diverge a given distance scales logarithmically in the amplitude of the perturbation.
15 pages, including 13 Figures and 1 Table, uses Phys. Rev. macros
References in corpus (6)
Cited by in corpus (17)
- A new Monte Carlo method for dynamical evolution of non-spherical stellar systems
- Chaos and chaotic phase mixing in cuspy triaxial potentials
- Fluctuations Do Matter: Large Noise-Enhanced Halos in Charged-Particle Beams
- Chaotic mixing in noisy Hamiltonian systems
- Chaos and the continuum limit in the gravitational N-body problem. I. Integrable potentials
- Chaos and the continuum limit in the gravitational N-body problem II. Nonintegrable potentials
- Chaos, ergodicity, and the thermodynamics of lower-dimensional Hamiltonian systems
- Production of Enhanced Beam Halos via Collective Modes and Colored Noise
- Chaos and the continuum limit in nonneutral plasmas and charged particle beams
- Effect of noise in open chaotic billiards
- Noise-Enhanced Parametric Resonance in Perturbed Galaxies
- Gibbs attractor: a chaotic nearly Hamiltonian system, driven by external harmonic force
- On the influence of noise on chaos in nearly Hamiltonian systems
- Energy relaxation in galaxies induced by an external environment and/or incoherent internal pulsations
- A disturbance in the force. How force fluctuations hinder dynamical friction and induce core stalling
- Noise, friction and the radial-orbit instability in anisotropic stellar systems: stochastic N-body simulations
- Taking apart the dynamical clock. Fat-tailed dynamical kicks shape the blue-straggler star bimodality