Abstract
Use of the surrogate zeta-function method was crucial in calculating the Casimir energy in non-Abelian Kaluza–Klein theories. We establish the validity of this method for the case where the background metric is (Euclidean space) × (N sphere). Our techniques do not apply to the case where the background is (Minkowski space) × (N sphere).
Publisher
Canadian Science Publishing
Subject
General Physics and Astronomy
Cited by
6 articles.
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