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 ${ 4\pi^2\over k^2} +O(k^{ -4})$, where $q^{ 2k}=1$. We also discuss the relation to the Euclidean Chern-Simons-Witten gravity in 3-dimension.

Categories: hep-th

3-dimensional Gravity from the Turaev-Viro Invariant