Solution
ID: past-exam-of-the-mathematics-course-of-the-university-of-cambridge/2002/iii/paper-75/2/a/solution
Past exam of the mathematics course of the University of Cambridge 2002 iii Paper 75 2 a Solution by
Codex 0 Created 2026-10-03 Updated 2026-10-14
Use physical momentum and conserved-background comoving momentum . At fixed , the homogeneous collisionless phase-space distribution function is , with no spatial or angular dependence and no explicit background time derivative. The printed relation cannot have this meaning: freely propagating physical momentum redshifts as , so it should read . Keeping the printed relation literally would give and a nonzero zeroth-order redshift, inconsistent with the target equation. The standard definition is positively confirmed by the phase-space convention in Ma and Bertschinger's perturbation treatment.
With this conserved , the orders of the factors are:
- is first order; the zeroth-order collisionless equation has already made .
- is first order, while has a zeroth-order free-streaming velocity and first-order corrections. Their product contributes at first order only through that background velocity.
- begins at zeroth order; begins at first order. Its leading product is .
- begins at first order, and begins at first order because background trajectories keep their direction. Their product is second order and drops out.
Thus the linear Collisionless Boltzmann equation isFor photons . For a particle of mass , . The order counting does not assume that the first-order angular deflection itself vanishes; only its multiplication by an already perturbed angular distribution makes it higher order.
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