English

A Simple Random-Walk Model Explains the Disruption Process of Hierarchical, Eccentric 3-Body Systems

Solar and Stellar Astrophysics 2020-09-08 v3 Earth and Planetary Astrophysics

Abstract

We study the disruption process of hierarchical 3-body systems with bodies of comparable mass. Such systems have long survival times that vary by orders of magnitude depending on the initial conditions. By comparing with 3-body numerical integrations, we show that the evolution and disruption of such systems can be statistically described as a simple random-walk process in the outer-orbit's energy, where the energy-exchange per pericenter passage (step-size) is calculated from the initial conditions. In our derivation of the step-size, we use previous analytic results for parabolic encounters, and average over the (Kozai-Lidov) oscillations in orbital parameters, which are faster then the energy diffusion timescale. While similar random-walk models were studied before, this work differs in two manners: (a) this is the first time that the Kozai-Lidov averaged step-size is derived from first principles and demonstrated to reproduce the statistical evolution of numerical ensembles without fitting parameters, and (b) it provides a characteristic life-time, instead of answering the binary question (stable/unstable), set by case-specific criteria.

Keywords

Cite

@article{arxiv.2005.03669,
  title  = {A Simple Random-Walk Model Explains the Disruption Process of Hierarchical, Eccentric 3-Body Systems},
  author = {Jonathan Mushkin and Boaz Katz},
  journal= {arXiv preprint arXiv:2005.03669},
  year   = {2020}
}

Comments

11 pages, 14 figures;

R2 v1 2026-06-23T15:23:27.719Z