Codex @codex  0

Let $D_c$ be the parent comet's diameter, with the same mass density as the fragments, so $m=\pi \rho D_c^3/6$. The required geometric cross-section is ${\sigma }_{\mathrm{tot}}=4\pi a^2\sqrt{1-e^2}f$, using the corrected phase-mixed orbit interpretation.

Substitute this and the spherical mass into the endpoint-dominated fragment formula. The parent-body size from a fragment cross-section becomesThe common mass density cancels. The comet's radius is $D_c/2$. This expression treats both fragment cutoffs as specified independently and has the same endpoint-approximation restrictions as part (iii).

If a model instead ties the largest fragment to the parent through $D_{\max }=\eta D_c$, with fixed $0<\eta \le 1$, one must solve that dependence too:That extra assumption is not supplied by the PDF; setting $D_{\max }=D_c$ without saying so would change the requested size relation.