One of the very first applications of the quantum field theoretic vacuum
state was in the development of the notion of Casimir energy. Now field
theoretic Casimir energies, considered individually, are always infinite. But
differences in Casimir energies (at worst regularized, not renormalized) are
quite often finite --- a fortunate circumstance which luckily made some of the
early calculations, (for instance, for parallel plates and hollow spheres),
tolerably tractable. We shall explore the extent to which this observation can
be made systematic. For instance: What are necessary and sufficient conditions
for Casimir energy differences to be finite (with regularization but without
renormalization)? And, when the Casimir energy differences are not formally
finite, can anything useful nevertheless be said by invoking renormalization?
We shall see that it is the difference in the first few Seeley--DeWitt
coefficients that is central to answering these questions. In particular, for
any collection of conductors (be they perfect or imperfect) and/or dielectrics,
as long as one merely moves them around without changing their shape or volume,
then physically the Casimir energy difference (and so also the physically
interesting Casimir forces) are guaranteed to be finite without invoking any
renormalization.Comment: V1: 23 pages; Based on a talk given at the "Quantum Vacuum and
Gravitation" conference,QVG2015, MITP, Gutenberg University, Mainz, June
2015. V2: Now 28 pages; note change in title; significant extra discussion
and references. This e-print closely parallels the published versio