Common Envelope Evolution: Too stochastic to be deterministic

arXiv:2609.37718 · astro-ph.SR · Submitted 2026-09-29 · Read on arXiv

astro-ph.SR

Submitted: 2026-09-29

Updated: 2026-09-29

Terminology

Core — 5× in this paper · explained in 2 episodes
Population Synthesis — 3× in this paper · explained in 2 episodes

Sources

A Framework for Linking Pre- and Post-Common Envelope Binary Properties with Star Clusters: The First Demonstration with a Massive White Dwarf+M Dwarf Binary in Alessi 12
Effect of Neutron Star Jets on Common Envelope Evolution
Simulating the convection in red super-giant stars: wobbling jets in common envelope evolution
Post-red-giant-branch Planetary Nebulae
Three-dimensional simulations of accretion disks in pre-CE systems -- II. Accretion efficiency and angular momentum transport
Disc-mediated angular momentum transport resolves the mass-gain problem in rotating binaries
AREPO-RSG: Aspherical Circumstellar Material and Winds from Pulsating Dusty Red Supergiants in Global 3D Radiation Hydrodynamic Simulations
Dust Formation in Common Envelope Binary Interactions -- III. Lightcurves
High-Speed Outflows and Dusty Disks during the AGB to PN Transition: The PANORAMA survey
Building three-dimensional giant stellar models for common envelope simulations
The Best Guess: Testing new and old formalisms for the common envelope against observations
A giant magnetic eruption from the asymptotic giant branch star Mira A
Population demographics of post-interaction WDMS binaries: From common envelope evolution to stable mass transfer
The Common Envelope Evolution Outcome. III. the Improvement of Stellar Binding Energy with the Envelope Residual

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