Planet formation at the inner edge of the dead zone I. the interplay between accretion outbursts and dust growth

arXiv:2602.20283 · astro-ph.EP, astro-ph.SR · Submitted 2026-02-23 · Read on arXiv

astro-ph.EP, astro-ph.SR

Submitted: 2026-02-23

Updated: 2026-08-26

Code: https://github.com/alexziab/growpacity

Terminology

• Streaming Instability — 5× in this paper · explained in 2 episodes
• Angular Momentum Transport — 4× in this paper · explained in 3 episodes
• Metallicity — 4× in this paper · explained in 3 episodes
• Abundance — 3× in this paper · explained in 1 episode
• Accuracy — 2× in this paper · explained in 1 episode
• Dynamic Modeling — 2× in this paper · explained in 3 episodes
• Activation Function — 1× in this paper · explained in 1 episode
• Adaptation — 1× in this paper · explained in 1 episode
• Trace — 1× in this paper · explained in 2 episodes
• Verification — 1× in this paper · explained in 2 episodes
• alpha — 1× in this paper · explained in 1 episode

Sources

• TriPoDPy: 1D Tri-Population size distributions forDust evolution in protoplanetary disks

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