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 giveIndeed 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.
Past exam of the mathematics course of the University of Cambridge 2017 iii Paper 316 1 iii Solution Created 2026-10-03 Updated 2026-10-06
Assume spherical fragments of the common mass density , and let count fragments per unit diameter. Mass normalization of a power-law size distribution givesTheir geometric cross-sections are , hence the cross-section of a power-law fragment population is exactlyFor , large fragments dominate the mass integral and small fragments dominate the geometric cross-section integral. Neglecting the subdominant endpoints givesThe 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.
Past exam of the mathematics course of the University of Cambridge 2019 iii Paper 316 2 i Solution Created 2026-10-03 Updated 2026-10-05
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 isConsequentlyThe 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.