Thermally Regulated Viscoelastic Tidal Migration of Eccentric Planets

arXiv:2606.14983 · astro-ph.EP · Submitted 2026-06-12 · Read on arXiv

Cristobal Petrovich, Hareesh Gautham Bhaskar

astro-ph.EP

Submitted: 2026-06-12

Comments: 16 pages, 8 figures, submitted to AAS Journals; comments welcome

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

Terminology

• Core — 39× in this paper · explained in 2 episodes
• Consistency — 1× in this paper · explained in 3 episodes
• Regularization — 1× in this paper · explained in 3 episodes

Sources

• Coupled orbital and interior structure evolution of lava planets
• Planetesimal-Driven Instabilities in Resonant Chains of Cold Neptunes and Their Dynamical Outcomes
• POSEIDON I: The Dynamical Origins of Transiting Neptunes
• A Homogeneous Catalog of Rossiter-McLaughlin Systems: Distinct e - lambda Trends in Three Gas-Giant Mass Regimes

Related papers

• PDS 70 c and SR 12 c: Observational Constraints on Giant-Planet and Satellite Formation
• Two-stage disruption of resonant chains
• Detectability of resolved hydrogen lines from the accretion shock at gas giants and their CPDs
• Binary-lens Microlensing Degeneracy: Impact on Planetary Sensitivity and Mass-ratio Function
• Atmospheric escape fractionates secondary but not primary atmospheres
• The Occurrence Rate of Nearby Planetary Companions to Hot Jupiters