Rational Conformal Field Theory and Multi-Wormhole Partition Function in 3-dimensional Gravity

preprint1992arXivOpen access

Abstract

We study the Turaev-Viro invariant as the Euclidean Chern-Simons-Witten gravity partition function with positive cosmological constant. After explaining why it can be identified as the partition function of 3-dimensional gravity, we show that the initial data of the TV invariant can be constructed from the duality data of a certain class of rational conformal field theories, and that, in particular, the original Turaev-Viro's initial data is associated with the Ak+1A_{k+1} modular invariant WZW model. As a corollary we then show that the partition function Z(M)Z(M) is bounded from above by Z((S2×S1)♯g)=(S00)−2g+2∼Λ−3g−32Z((S^2\times S^1)^{\sharp g}) =(S_{00})^{-2g+2}\sim Λ^{-\frac{3g-3}{2}}, where gg is the smallest genus of handlebodies with which MM can be presented by Hegaard splitting. Z(M)Z(M) is generically very large near Λ∼+0Λ\sim +0if MM is neither S3S^3 nor a lens space, and many-wormholeconfigurations dominate near Λ∼+0Λ\sim +0 in the sense that Z(M)Z(M) generically tends to diverge faster as the ``number of wormholes'' gg becomes larger.

Explore this paper’s authors, topics and related work.

Building this map preview

BZPEER is loading the nearby papers, people, topics and institutions for this page.

Reviews 0

Write a reviewWrite

No reviews yet.

Discussion 0

Add a commentWrite

No comments yet.