Using the radial-drift expression already derived, the factor cancels and gives
For , and , so
The instantaneous flow is inward for and outward for . Nevertheless outward motion need not prevent eventual accretion. The trajectories in accretion trajectories in a compact viscous similarity disk satisfy
Multiplication by and integration give
A parcel at at time has . It reaches the origin at
Before arrival, decreases monotonically. Even a parcel initially moving outward eventually crosses , turns inward, and is accreted. Only , the outer-edge trajectory, never arrives; its surface density of a disk is zero. Thus almost every mass-carrying parcel is accreted in finite time.
For , the coefficient vanishes, leaving
The trajectories are , so each parcel keeps a fixed ratio . This is an expanding nonaccreting similarity disk supplied by an inner torque, not an inward accretion solution.