$N$-body chaos, phase-space transport and relaxation in numerical simulations
Astrophysics of Galaxies
2020-03-18 v1
Abstract
Using direct -body simulations of self-gravitating systems we study the dependence of dynamical chaos on the system size . We find that the -body chaos quantified in terms of the largest Lyapunov exponent decreases with . The values of its inverse (the so-called Lyapunov time ) 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.
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"