Effects of Radiative Diffusion on Dynamical Corotation Torque in Three-dimensional Protoplanetary Disks

The dynamical corotation torque arising from the deformation of horseshoe orbits, along with the vortensity gradient in the background disk, is important for determining the orbital migration rate and direction of low-mass planets. Previous two-dimensional studies have predicted that the dynamical c...

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Bibliographic Details
Published in:The Astrophysical journal 2022-10, Vol.938 (2), p.102
Main Authors: Yun, Han-Gyeol, Kim, Woong-Tae, Bae, Jaehan, Han, Cheongho
Format: Article
Language:English
Subjects:
Accretion disks
Adiabatic flow
Astrophysics
Buoyancy
Corotation
Deceleration
Deposition
Diffusion
Diffusion effects
High altitude
Irradiation
Planet formation
Planetary evolution
Planetary migration
Planetary-disk interactions
Planets
Protoplanetary disks
Radiative transfer
Resonance
Torque
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Summary:The dynamical corotation torque arising from the deformation of horseshoe orbits, along with the vortensity gradient in the background disk, is important for determining the orbital migration rate and direction of low-mass planets. Previous two-dimensional studies have predicted that the dynamical corotation torque is positive, decelerating inward planet migration. In contrast, recent three-dimensional studies have shown that buoyancy resonance makes the dynamical corotation torque negative, accelerating inward migration. In this paper, we study the dependence of the dynamical corotation torque on thermal transport, using three-dimensional simulations. We first show that our results are consistent with previous three-dimensional studies when the disk is fully adiabatic. In more realistic radiative disks, however, radiative diffusion suppresses buoyancy resonance significantly, especially in high-altitude regions, and yields a positive dynamical corotation torque. This alleviates the issue of rapid migration being caused by the negative dynamical corotation torque in adiabatic disks. Our results suggest that radiative diffusion, together with stellar irradiation and accretion heating, are needed to accurately describe the migration of low-mass planets.
ISSN:0004-637X
1538-4357
DOI:10.3847/1538-4357/ac9185