TWO-POP-PY runs a two-population dust evolution model that follows the upper end of the dust size distribution and the evolution of the dust surface density profile and treats dust surface density, maximum particle size, small and large grain velocity, and fragmentation. It derives profiles that describe the dust-to-gas ratios and the dust surface density profiles well in protoplanetary disks, in addition to the radial flux by solid material rain out.
https://ui.adsabs.harvard.edu/abs/2012A%26A...539A.148B and, if you use the size distribution reconstruction, also https://ui.adsabs.harvard.edu/abs/2015ApJ...813L..14B