TRACE: a code for Time-Reversible Astrophysical Close Encounters
Tiger Lu, David M. Hernandez, Hanno Rein

TL;DR
TRACE is a novel, nearly time-reversible hybrid integrator for planetary N-body simulations that offers superior speed and accuracy in modeling close encounters and complex astrophysical systems.
Contribution
It introduces a new time-reversible switching method for hybrid integrators, improving performance over existing methods like MERCURIUS and IAS15.
Findings
TRACE matches or exceeds the accuracy of existing integrators.
TRACE achieves up to 41x speed-up in large N-body simulations.
TRACE performs well in systems with close encounters and violent scattering.
Abstract
We present TRACE, an almost time-reversible hybrid integrator for the planetary N-body problem. Like hybrid symplectic integrators, TRACE can resolve close encounters between particles while retaining many of the accuracy and speed advantages of a fixed time-step symplectic method such the Wisdom-Holman map. TRACE switches methods time-reversibly during close encounters following the prescription of Hernandez & Dehnen. In this paper we describe the derivation and implementation of TRACE and study its performance for a variety of astrophysical systems. In all our test cases, TRACE is at least as accurate and fast as the hybrid symplectic integrator MERCURIUS. In many cases, TRACE's performance is vastly superior to that of MERCURIUS. In test cases with planet-planet close encounters, TRACE is as accurate as MECURIUS with a 12x speed-up. If close encounters with the central star are…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
