Steady State by Recycling prevents Premature Collapse of Protoplanetary Atmospheres
T. W. Moldenhauer, R. Kuiper, W. Kley, C. W. Ormel

TL;DR
This paper demonstrates through 3D simulations that atmosphere-disk recycling can establish a steady state, preventing premature collapse of protoplanetary atmospheres and explaining the existence of mini-Neptunes.
Contribution
It provides the first detailed simulation evidence that recycling halts cooling and contraction, maintaining atmospheres in a steady state and avoiding runaway gas accretion.
Findings
Recycling leads to a steady state in planetary atmospheres.
Recycling prevents atmospheres from collapsing into gas giants.
Steady state is achieved where radiative cooling is balanced by gas recycling.
Abstract
In recent years, space missions such as Kepler and TESS have discovered many close-in planets with significant atmospheres consisting of hydrogen and helium: mini-Neptunes. This indicates that these planets formed early in gas-rich disks while avoiding the runaway gas accretion that would otherwise have turned them into hot-Jupiters. A solution is to invoke a long Kelvin-Helmholtz contraction (or cooling) timescale, but it has also been suggested that thermodynamical cooling can be prevented by hydrodynamical planet atmosphere-disk recycling. We investigate the efficacy of the recycling hypothesis in preventing the collapse of the atmosphere, check for the existence of a steady state configuration, and determine the final atmospheric mass to core mass ratio. We use three-dimensional radiation-hydrodynamic simulations to model the formation of planetary proto-atmospheres. Equations are…
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