Hydrodynamical Simulations of Resonant Breaking in Multi-Planet Systems via Rebound Migration During Disk Dispersal

arXiv:2606.11452 · astro-ph.EP · Submitted 2026-06-09 · Read on arXiv

Beibei Liu, Clément Baruteau, Zhaohuan Zhu, Ya-Ping Li, Sijme-Jan Paardekooper, Shigeru Ida

astro-ph.EP

Submitted: 2026-06-09

Comments: 10 pages, 9 figures, accepted for publication in A&A, animations on this link: https://github.com/bbliu-astro/movies/tree/main/hydrodynamic_rebound

Code: https://github.com/bbliu-astro/movies

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

Terminology

• Accuracy — 1× in this paper · explained in 1 episode

Sources

• Dynamical Excitation as a probe of planetary origins
• Capture and Stability of Resonant Planet Pairs in Turbulent Disk
• 3D MHD simulations of planet migration in cavities and inner discs of magnetized stars

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