On the derivation of the Kompaneets equation.

The relaxation of a photon bath to thermal equilibrium via Compton scattering with electrons is described in the Kompaneets equation (1956). The equation is mostly known from studies of astrophysical plasmas, for its convergence to the Planck distribution and for explaining the Sunyaev-Zeldovich effect changing the apparent brightness of the cosmic microwave background radiation. We revisit its derivation emphasizing its structure as a Kramers-Moyal diffusion approximation to the quantum Boltzmann equation or Master equation with stimulated emission. We do not assume that the Planck law is stationary in performing the continuum approximation but we emphasize the necessity of the flux or M{\o}ller factor to arrive at a continuity equation. On the other hand, the structure allows more general assumptions than originally envisioned by Kompaneets.