  We calculate the first relativistic corrections to the Kompaneets equation
for the evolution of the photon frequency distribution brought about by Compton
scattering. The Lorentz invariant Boltzmann equation for electron-photon
scattering is first specialized to isotropic electron and photon distributions,
the squared scattering amplitude and the energy-momentum conserving delta
function are each expanded to order v^/c^4, averages over the directions of the
electron and photon momenta are then carried out, and finally an integration
over the photon energy yields our Fokker- Planck equation. The Kompaneets
equation, which involves only first- and second-order derivatives with respect
to the photon energy, results from the order v^2/c^2 terms, while the first
relativistic corrections of order v^4/c^4 introduce third- and fourth-order
derivatives. We emphasize that our result holds when neither the electrons nor
the photons are in thermal equilibrium; two effective temperatures characterize
a general, non-thermal electron distribution. When the electrons are in thermal
equilibrium our relativistic Fokker-Planck equation is in complete agreement
with the most recent published results, but we both disagree with older work.
