Casimir energy of confining large N gauge theories

Abstract

Four-dimensional asymptotically-free large N gauge theories compactified on S3R × R have a weakly-coupled confining regime when R is small compared to the strong scale. We compute the vacuum energy of a variety of confining large N non-supersymmetric gauge theories in this calculable regime, where the vacuum energy can be thought of as the S3 Casimir energy. The N=∞ renormalized vacuum energy turns out to vanish in all of the large N gauge theories we have examined, confirming a striking prediction of temperature-reflection symmetry.

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