We consider a five-layer Casimir cavity, including a thin superconducting
film. We show that when the cavity is cooled below the critical temperature for
the onset of superconductivity, the sharp variation (in the microwave region)
of the reflection coefficient of the film produces a variation in the value of
the Casimir energy. Even though the relative variation in the Casimir energy is
very small, its magnitude can be comparable to the condensation energy of the
superconducting film, and thus causes a significant increase in the value of
the critical magnetic field, required to destroy the superconductivity of the
film. The proposed scheme might also help clarifying the current controversy
about the magnitude of the contribution to Casimir free energy from the TE zero
mode, as we find that alternative treatments of this mode strongly affect the
shift of critical field.Comment: RevTex 4, 15 pages, 8 figures. Revised version with improved
presentation, a brief description of the ALADIN experiment, and a few
references adde