N-Body Dynamics as a Mechanism for Mean Motion Resonance Formation in the Post-Gas Era

arXiv:2609.31244 · astro-ph.EP · Submitted 2026-09-25 · Read on arXiv

astro-ph.EP

Submitted: 2026-09-25

Updated: 2026-09-25

Comments: 18 pages, 3 figures; accepted for publication in Research in Astronomy and Astrophysics

License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/

Terminology

• N-body simulations — 7× in this paper · explained in 2 episodes
• Robustness — 3× in this paper · explained in 5 episodes
• Trace — 2× in this paper · explained in 2 episodes
• Benchmark — 1× in this paper · explained in 2 episodes
• Clustering — 1× in this paper · explained in 2 episodes

Sources

• Terrestrial planet formation in the era of GPU computing

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