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PrefaceZeta regularization is a method to treat the divergent quantities appearing in several areas of mathematics and physics; these are managed by introducing a complex parameter, with the role of a regulator, and defining their "renormalized versions" in terms of the analytic continuation with respect to the regulator. The standard textbook example of this procedure deals with the divergent series +∞
=1(1) which, in the zeta approach, is interpreted as the analytic continuation at s = −1 of the regularized series ζ(s) := +∞ =1 −s . The latter series only converges for s > 1 but the function s → ζ(s) defined in this way, the well-known Riemann zeta function, possesses a unique analytic extension to C \ {1} and ζ(−1) = −1/12; in this sense, the sum (1) "equals" −1/12. In a more pictorial language, one could say that −1/12 is the "renormalized" value of the series (1).The application of zeta regularization to the divergences of quantum field theory was first proposed by Dowker and Critchley [46], Hawking [84] and Wald [146] to renormalize local observables, especially the vacuum expectation value (VEV) of the stress-energy tensor. The ultimate purpose was the semiclassical treatment of quantum effects in general relativity, e.g. using the stress-energy VEV as a source term in Einstein's equations. Due to the attention to vacuum states, the zeta approach was connected from its very beginning to Casimir physics. However, the above mentioned pioneers focused their investigations on the conceptual validity of the method, rather than on its implementation for actual computations in specific configurations. For example, the elegant formula of Dowker-Critchley-Hawking, which gives the VEV of the stress-energy tensor as the functional derivative of the (renormalized) effective field action with respect to the space-time metric is not useful for actual computations in a given geometry, apart from very special cases. This is due to the fact that its use would require computing the effective action for all spacetime metrics close the one under consideration. For this reason, Birrel and Davies have described the application of this formula as "impossibly difficult" (see [18], page 190).Moreover, papers [46,84, 146] deal with a quantized field on the whole spacetime manifold and do not consider the possibility of confining the field to a given space ...