A Coordinate System for Dynamical Instabilities in Hierarchical Systems in REBOUND
Tiger Lu, Garett Brown
astro-ph.EP, astro-ph.IM
Submitted: 2026-05-01
Comments: Submitted to AAS Journals, comments welcome
License: http://creativecommons.org/licenses/by/4.0/
The gist: We implement coordinates suitable for studying wide binary systems in TRACE, a hybrid integrator in the widely used open-source N-body integration package REBOUND.
Terminology
Abstract
We implement coordinates suitable for studying wide binary systems in TRACE, a hybrid integrator in the widely used open-source N-body integration package REBOUND. This is a regime in which traditional hybrid integrators perform poorly. The coordinate system supports close encounters between any pair of bodies in the system. We describe the implementation of this coordinate system and benchmark its performance against other integrators in the REBOUND ecosystem. In tests of planet-planet scattering, stellar flybys, and ZLK oscillations. TRACE in wide binary coordinates is qualitatively correct when other hybrid methods fail, and in many cases returns statistically similar results to the high-precision IAS15 integrator with up to 9x speedups. We also provide some guidelines for when use of these coordinates are appropriate.
Sources
- Gravitational Scattering
- Artificial precession and instability in solar system and planetary simulations: analytic and numerical results
- Democratic heliocentric coordinates underestimate the rate of instabilities in long-term integrations of the Solar System
- Planetary Architectures of Kepler Compact Multis with Binary Star Companions
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