Ultraviolet divergences, repulsive forces and a spherical plasma shell

Abstract

We discuss the vacuum energy of the electromagnetic ¯eld interacting with a spherical plasma shell together with a model for the classical motion of the shell. We discuss the ultraviolet divergences in terms of the heat kernel coe±cients. Using these, we carry out the renormalization by rede¯ning the parameters of the classical model. It turns out that this is possible and that the resulting model has a vacuum energy which changes sign in dependence on the parameters of the plasma shell. In the limit of the plasma shell becoming an ideal conductor the vacuum energy found by Boyer in 1968 is reproduced

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