Acceleration of a relativistic plasma by radiation pressure

The greatly enhanced radiation pressure force felt by a relativistic plasma is accompanied by catastrophic Compton cooling and only in extreme conditions can it lead to acceleration to relativistic bulk velocities. The equations of motion are solved in the optimal case and it is found that the efficiency of acceleration is typically < 1 per cent (the energy lost being given to the scattered photons). The complicating effects of expansion of the plasma, finite source size and scattering above the Klein-Nishina limit are described. The paper ends with a short list of situations in which the phenomenon may nevertheless be of importance. (author)