English

$N$-body chaos, phase-space transport and relaxation in numerical simulations

Astrophysics of Galaxies 2020-03-18 v1

Abstract

Using direct NN-body simulations of self-gravitating systems we study the dependence of dynamical chaos on the system size NN. We find that the NN-body chaos quantified in terms of the largest Lyapunov exponent Λmax\Lambda_{\rm max} decreases with NN. The values of its inverse (the so-called Lyapunov time tλt_\lambda) are found to be smaller than the two-body collisional relaxation time but larger than the typical violent relaxation time, thus suggesting the existence of another collective time scale connected to many-body chaos.

Keywords

Cite

@article{arxiv.1907.12774,
  title  = {$N$-body chaos, phase-space transport and relaxation in numerical simulations},
  author = {Pierfrancesco Di Cintio and Lapo Casetti},
  journal= {arXiv preprint arXiv:1907.12774},
  year   = {2020}
}

Comments

4 pages, 2 figures. To appear in the proceedings of the 351 IAU Symposium "Star Clusters: from the Milky Way to the Early Universe"