A map for eccentric orbits in triaxial potentials
Astrophysics
2015-06-24 v1
Abstract
We construct a simple symplectic map to study the dynamics of eccentric orbits in non-spherical potentials. The map offers a dramatic improvement in speed over traditional integration methods, while accurately representing the qualitative details of the dynamics. We focus attention on planar, non-axisymmetric power-law potentials, in particular the logarithmic potential. We confirm the presence of resonant orbit families (``boxlets'') in this potential and uncover new dynamics such as the emergence of a stochastic web in nearly axisymmetric logarithmic potentials. The map can also be applied to triaxial, lopsided, non-power-law and rotating potentials.
Cite
@article{arxiv.astro-ph/9706046,
title = {A map for eccentric orbits in triaxial potentials},
author = {J. Touma and S. Tremaine},
journal= {arXiv preprint arXiv:astro-ph/9706046},
year = {2015}
}
Comments
29 pages, 9 figures, Latex, submitted to MNRAS