English

Split invariant curves in rotating bar potentials

Chaotic Dynamics 2021-11-17 v2 Astrophysics of Galaxies

Abstract

Invariant curves are generally closed curves in the Poincare's surface of section. Here we study an interesting dynamical phenomenon, first discovered by Binney et al. (1985) in a rotating Kepler potential, where an invariant curve of the surface of section can split into two disconnected line segments under certain conditions, which is distinctively different from the islands of resonant orbits. We first demonstrate the existence of split invariant curves in the Freeman bar model, where all orbits can be described analytically. We find that the split phenomenon occurs when orbits are nearly tangent to the minor/major axis of the bar potential. Moreover, the split phenomenon seems necessary to avoid invariant curves intersecting with each other. Such a phenomenon appears only in rotating potentials, and we demonstrate its universal existence in other general rotating bar potentials. It also implies that actions are no longer proportional to the area bounded by an invariant curve if the split occurs, but they can still be computed by other means.

Keywords

Cite

@article{arxiv.2109.06744,
  title  = {Split invariant curves in rotating bar potentials},
  author = {Tian-Ye Xia and Juntai Shen},
  journal= {arXiv preprint arXiv:2109.06744},
  year   = {2021}
}

Comments

Accepted to publish on ApJ. 8 pages, 6 figures. The animated version of Figure 1 is at this link: http://astro.sjtu.edu.cn/~jtshen/split_ic/3Dps.mp4

R2 v1 2026-06-24T05:57:28.492Z