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The response of a superconductor to a gravitational wave is shown to obey aLondon-like constituent equation. The Cooper pairs are described by theGinzburg-Landau free energy density embedded in curved spacetime. The latticeions are modeled by quantum harmonic oscillators characterized by quasi-energyeigenvalues. This formulation is shown to predict a dynamical Casimir effectsince the zero-point energy of the ionic lattice phonons is modulated by thegravitational wave. It is also shown that the response to a gravitational waveis far less for the Cooper pair density than for the ionic lattice. Thispredicts a "charge separation effect" which can be used to detect the passageof a gravitational wave.

A new approach to detecting gravitational waves via the coupling of gravity to the zero-point energy of the phonon modes of a superconductor