Structure of Convective-Reactive Zone in a Supernova Progenitor

arXiv:2610.01239 · astro-ph.SR, astro-ph.HE · Submitted 2026-10-01 · Read on arXiv

astro-ph.SR, astro-ph.HE

Submitted: 2026-10-01

Updated: 2026-10-01

Code: https://github.com/mmicromegas/ransX

Terminology

• Entrainment — 29× in this paper · explained in 2 episodes
• Abundance — 18× in this paper · explained in 1 episode
• Core — 4× in this paper · explained in 2 episodes
• Reynolds-Averaged Navier-Stokes — 3× in this paper
• Robustness — 2× in this paper · explained in 5 episodes
• Artificial Intelligence (AI) — 1× in this paper · explained in 2 episodes

Sources

• 3D Macro Physics and Light Odd-Z Element Production in O-C Shell Mergers: Implications for $^{40}\mathrm{K}$ production and radiogenic heating inventories of rocky exoplanets
• Compressible Hydrodynamic Mean-Field Equations in Spherical Geometry and their Application to Turbulent Stellar Convection Data
• Astrophysical Reaction Rates From Statistical Model Calculations
• Destratification in the Progenitor Interior of the Mg-rich Supernova Remnant N49B

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