Same as in Fig. 4, except for Model V. The corresponding temporal evolution of the five dust quantities is shown in Fig. 7. The gas surface density (panel b) is fixed to the input profile corresponding to the classical self-similar solution (Lynden-Bell & Pringle 1974), with a total disk gas mass M_disk = 0.05 M_⋆, and a critical radius R_c = 80 au. As a result, the gas is no longer in a steady-state MRI-driven accretion at t = 0 yr, unlike Model IV. Here we note that, in panel f, the dead zone outer edge coincides at t = 0 yr and t = 100 yr.