Solution

ID: past-exam-of-the-kinetic-theory-course-of-the-university-of-oxford/2025/3/c/solution

Let denote . Average the Collisionless Boltzmann equation to second order. All first-order angle derivatives average to zero, leaving
An angle integration by parts shows that
Thus the angle-averaged galactic distribution function obeys an action-space continuity equation,
This sign also follows from Hamilton's equations, : the flux is .
Reality gives and . Orthogonality of the Fourier series implies
Insert b to obtain
Although individual terms are complex, pairing with makes the flux real.
Now take the marginalization specified by . Assume vanishing radial-action flux at and : the first boundary does not permit negative radial action, and the second has no escaping flux in this calculation. Then
with
If radial-action boundary flux were present, its explicit boundary term would have to be retained.

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