Solution

ID: past-exam-of-the-mathematics-course-of-the-university-of-cambridge/2016/iii/paper-321/1/a/ii/solution

Let with . The derivatives of this similarity solution are
The first-derivative terms cancel in the dimensionless diffusion equation, leaving for . Thus
At the inner boundary , . Interpreting the named variable as vanishing there sets . Even if only the true viscous torque in an accretion disk is required to vanish, a nonzero would give infinite total mass near ; finite mass again selects . With nonnegative surface density, choose ; its value fixes the initial mass normalization. Therefore
The surface density vanishes exponentially at the origin and has an tail at infinity. Its peak occurs at , with . The peak moves inward and grows as time increases.
Figure 1.
Surface-density profiles of the printed similarity solution at two times, showing an inward-moving growing peak and the outer power-law tail
. Details.
The plot uses and shows the actual surface density, with logarithmic radius to resolve both peaks. The later profile is larger at every fixed radius. Its total mass is finite; its total angular momentum is not, as the next calculation establishes.

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