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A moving pellicle superconducting mirror, which is driven by radiationpressure on its one side, and by the Coulomb force on its other side, canbecome a parametric oscillator that can generate microwaves when placed withina high-Q superconducting Fabry-Perot resonator system. A paraxial-wave analysisshows that the fundamental resonator eigenmode needed for parametricoscillation is the TM011 mode. A double Fabry-Perot structure is introduced toresonate the pump and the idler modes, but to reject the parasitic anti-Stokesmode. The threshold for oscillation is estimated based on theradiation-pressure coupling of the pump to the signal and idler modes, andindicates that the experiment is feasible to perform.

Parametric Oscillation of a Moving Mirror Driven by Radiation Pressure in a Superconducting Fabry-Perot Resonating System