Two-Dimensional Study of the Propagation of Planetary Wake and the Indication to Gap Opening in an Inviscid Protoplanetary Disk
Takayuki Muto, Takeru K. Suzuki, Shu-ichiro Inutsuka

TL;DR
This study investigates how planetary wakes influence gap formation in inviscid protoplanetary disks, revealing new criteria for gap opening that depend on wave shock dissipation and migration dynamics.
Contribution
It introduces a combined analytical and numerical approach to identify conditions for gap formation, emphasizing the role of shock-induced vorticity and migration halts.
Findings
Gap can form around low-mass planets due to shock dissipation.
Minimum planetary mass for gap opening is lower than previously estimated.
Gap formation criteria depend on migration timescales and wave dynamics.
Abstract
We analyze the physical processes of gap formation in an inviscid protoplanetary disk with an embedded protoplanet using two-dimensional local shearing-sheet model. Spiral density wave launched by the planet shocks and the angular momentum carried by the wave is transferred to the background flow. The exchange of the angular momentum can affect the mass flux in the vicinity of the planet to form an underdense region, or gap, around the planetary orbit. We first perform weakly non-linear analyses to show that the specific vorticity formed by shock dissipation of density wave can be a source of mass flux in the vicinity of the planet, and that the gap can be opened even for low-mass planets unless the migration of the planet is substantial. We then perform high resolution numerical simulations to check analytic consideration. By comparing the gap opening timescale and type I migration…
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