Past exam of the mathematics course of the University of Cambridge 2018 iii Paper 301 3 iii Solution Created 2026-10-03 Updated 2026-10-05
Use the Lorentz-invariant phase-space measure from the original PDF, including the and factors missing from the local TeX. In the center of mass frame put and , assuming . The spatial Dirac delta distribution sets , leavingSince , the radial integral givesThe invariant flux factor is , using the Källén function. Dividing the phase space by this flux yields , with the final-state labels retained as in the printed formula.
Let . Of the Mandelstam variables, isThe azimuthal integral contributes , and the angular endpoints are thereforeChanging variables gives the requested expression from the formula supplied in the paper:There is a normalization qualification: the displayed starting formula integrates over labeled final momenta and contains no . For the physical cross-section of two indistinguishable outgoing quanta of this real scalar field, the identical-particle factor in a final-state phase-space integral divides the full integral by two. With that convention ; equivalently, integrate only one representative of each exchanged pair. The boxed value follows the given formula exactly.