On disc protoplanet interactions in a non-barotropic disc with thermal diffusion
S.-J. Paardekooper, J. C. B. Papaloizou

TL;DR
This paper investigates how the radial entropy gradient and thermal diffusion in a non-barotropic disc influence the migration of low-mass protoplanets, revealing non-linear effects that can reverse migration direction.
Contribution
It extends standard planet migration theory by incorporating non-barotropic effects and thermal diffusion, highlighting the importance of entropy gradients on migration behavior.
Findings
Entropy gradients significantly alter corotation torques.
Non-linear effects can cause outward migration.
Thermal diffusion influences torque saturation.
Abstract
We study the disc planet interactions of low-mass protoplanets embedded in a circumstellar disc. We extend the standard theory of planet migration from the usual locally isothermal assumption to include non-barotropic effects, focusing on the validity of linear theory. We compared solutions of the linear equations with results from non-linear hydrodynamic simulations, where in both cases we adopted a background entropy gradient and solved the energy equation. We show that the migration behavior of embedded planets depends critically on the background radial entropy gradient in the disc. The presence of such a gradient not only changes the corotation torque on the planet, but also always guarantees a departure from linear behavior, which gives a singular density response at corotation, in the absence of thermal or viscous diffusion. A negative entropy gradient tends to give rise to…
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