PIM (in Earth masses) with effects of dust turbulent diffusion. A comparison between the results of our semi-analytical calculation (solid curves) and those of (Bitsch et al. 2018; dashed curves) for Σ ∝ r−0.5, uniform aspect ratios and two values of the turbulent viscosity of the disk: α = 10−2 (upper panel) and α = 5 × 10−4 (lower panel). The red stars indicate the PIM obtained from our 2D gas plus dust simulations (for h = 0.04).
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