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The Sum over Topologies in Three-Dimensional Euclidean Quantum Gravity

Steven Carlip

hep-tharXiv:hep-th/9206103

Abstract

In Hawking's Euclidean path integral approach to quantum gravity, the partition function is computed by summing contributions from all possible topologies. The behavior such a sum can be estimated in three spacetime dimensions in the limit of small cosmological constant. The sum over topologies diverges for either sign of Λ, but for dramatically different reasons: for Λ>0, the divergent behavior comes from the contributions of very low volume, topologically complex manifolds, while for Λ<0 it is a consequence of the existence of infinite sequences of relatively high volume manifolds with converging geometries. Possible implications for four-dimensional quantum gravity are discussed.

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