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The document presents a study on the buoyancy response of protoplanetary discs to embedded planets, highlighting a cross-code comparison between PLUTO/IDEFIX and FARGO3D through high-resolution numerical simulations. It reveals that PLUTO/IDEFIX struggles to resolve higher-order buoyancy-related oscillations, which weakens vortensity growth and associated torque, suggesting that high-resolution or high-order schemes are necessary for accurate modeling. The findings emphasize the importance of numerical meth
- Author
- elitegamerx1987
- Language
- EN