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A fully QED/relativistic theory of light pressure of CMB radiation andFokker-Planck equation for electron distribution combined with cosmologicrelation for CMB temperature, T, yields analytic results for the evolution ofthe distribution over large span of time and energies. A strong imprint of CMBon electrons transpires via formation of "frozen non-equilibrium" state ofelectrons in current epoch, and possible existence of cutoff and narrowspectral lines as remnants of high-T sources.

Compton light pressure and spectral imprint of relic radiation on cosmic electrons