The structure of phase space close to fixed points in a 4D symplectic map
arXiv:1205.4575 · doi:10.1142/S0218127413300231
Abstract
We study the dynamics in the neighborhood of fixed points in a 4D symplectic map by means of the color and rotation method. We compare the results with the corresponding cases encountered in galactic type potentials and we find that they are in good agreement. The fact that the 4D phase space close to fixed points is similar to the 4D representations of the surfaces of section close to periodic orbits, indicates an archetypical 4D pattern for each kind of (in)stability, not only in 3D autonomous Hamiltonian systems with galactic type potentials but for a larger class of dynamical systems. This pattern is successfully visualized with the method we use in the paper.
7 pages,6 figures
References in corpus (5)
- Probing the local dynamics of periodic orbits by the generalized alignment index (GALI) method
- The structure of invariant tori in a 3D galactic potential
- The structure and evolution of confined tori near a Hamiltonian Hopf Bifurcation
- Instabilities and stickiness in a 3D rotating galactic potential
- Chains of rotational tori and filamentary structures close to high multiplicity periodic orbits in a 3D galactic potential
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