For spherical fragments of common mass density , with between specified diameter cutoffs, mass normalization of a power-law size distribution and integration of the geometric cross-section give
Indeed and ; eliminating proves the formula. If both cutoff ratios raised to and are small, respectively, this reduces to . Approaching either endpoint requires the corresponding logarithmic integral.
Assume spherical fragments of the common mass density , and let count fragments per unit diameter. Mass normalization of a power-law size distribution gives
Their geometric cross-sections are , hence the cross-section of a power-law fragment population is exactly
For , large fragments dominate the mass integral and small fragments dominate the geometric cross-section integral. Neglecting the subdominant endpoints gives
The two actual error parameters are and . They must both be small; the approximation is not uniform as approaches either endpoint. At or the corresponding integral is logarithmic, so the endpoint-dominated formula must be replaced by that integral.
Assume spherical bodies of common mass density , a well-mixed belt, and that counts bodies in the entire belt rather than per unit volume. A body of diameter has mass . The mass normalization of a power-law size distribution is
Consequently
The thin-torus volume is circumference times radial width times full vertical height,
The local number-density distribution needed for a planetesimal collision rate is . Thus belt geometry does not enter this total-number but does enter collision rates. This approximation treats the stated height as uniform, independent of size.