We apply the background field method and the effective action formalism to
describe the four-dimensional dynamical Casimir effect. Our picture corresp
onds to the consideration of quantum cosmology for an expanding FRW univers
e (the boundary conditions act as a moving mirror) filled by a quantum mass
less GUT which is conformally invariant. We consider cases in which the sta
tic Casimir energy is attractive and repulsive. Inserting the simplest poss
ible inertial term, we find, in the adiabatic (and semiclassical) approxima
tion, the dynamical evolution of the scale factor and the dynamical Casimir
stress analytically and numerically [for SU(2) super Yang-Mills theory]. A
lternative kinetic energy terms are explored in the appendix.