3-dimensional Gravity from the Turaev-Viro Invariant

TL;DR

In the semiclassical continuum limit the Turaev-Viro invariant obtained recently defines a naturally regularized path integral {ital a} {ital la} Ponzano and Regge, in which a contribution from the cosmological term is effectively included.

Abstract

We study the $q$-deformed su(2) spin network as a 3-dimensional quantum gravity model. We show that in the semiclassical continuum limit the Turaev-Viro invariant obtained recently defines naturally regularized path-integral $\grave{\rm a}$ la Ponzano-Regge, In which a contribution from the cosmological term is effectively included. The regularization dependent cosmological constant is found to be ${4π^2\over k^2} +O(k^{-4})$, where $q^{2k}=1$. We also discuss the relation to the Euclidean Chern-Simons-Witten gravity in 3-dimension.