Top: Mass loss rates from Owen & Kollmeier (2019, Figure 6) due to radiation pressure, with the photoevaporative trap location and dust surface density evolution of our fiducial model plotted on top (dashed line). Bottom: Mass loss rates for the fiducial smooth disk model (solid), the disk model with uniform entrainment (ϵ_w = ϵ, dotted), and the estimated loss rates from the Owen & Kollmeier (2019) radiation pressure (dashed), given our fiducial model properties.