Comparison of dust fluxes and the fraction of total accreted dust mass in the full disk models for various planet masses and dust diffusivities. Top: dust flux through the planetary gap in models with different planet masses. The blue line is for a model without a planet. The dashed, dotted, and dash-dotted red lines show additional simulations with a Saturn-mass planet for different radial dust diffusivity parameters δ_r. Bottom: total fraction of outer dust mass accreted through the planetary gap.