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Constrained partition functions and the antisymmetric tensor field

Michael McGuigan

  • School of Natural Sciences, Institute for Advanced Study, Olden Lane, Princeton, New Jersey 08540

Phys. Rev. D 42, 2040 – Published 15 September, 1990

DOI: https://doi.org/10.1103/PhysRevD.42.2040

Abstract

We consider the case when the spatial topology of the Universe is that of a torus with metric gij. We form an expression for the density of states under the constraint that the total momentum and winding number are zero. To accomplish this we introduce nonzero values of g00, g0i, and B0i in the imaginary-time formalism and integrate over all such values.

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