Evolution of the dust mass loss over time for a photoevaporating disk with F_UV = 10³ G₀. Top: evolution of the dust loss rate with and without dust traps (solid vs. dotted lines). The figure shows the distinction between the dust loss rate due to drift into the star (red), and due to entrainment with the photoevaporative wind (blue). Bottom: cumulative fraction of dust lost (relative to the initial dust mass) due to winds and drift.