Quasi-local holographic dualities in non-perturbative 3d quantum gravity
Bianca Dittrich, Christophe Goeller, Etera R. Livine, Aldo Riello
TL;DR
This paper investigates quasi-local holographic dualities in 3d quantum gravity using the $Ponzano-Regge$ state-sum to relate finite-region bulk quantum geometry to boundary 2d theories. It shows how boundary spin-network data induce 2d statistical models, exemplified by the isotropic $6$-vertex model at $j= frac{1}{2}$ on a square lattice, and derives a boundary action for a twisted torus that, in a stationary-phase regime, reproduces the expected semi-classical partition function and reveals a $BMS_3$-like structure in the $ abla$-to-zero limit. The study discusses two distinct large-scale limits and their interplay and highlights non-local topological insertions that encode bulk non-contractible cycles without summing over bulk topologies. Together these results provide a concrete, non-perturbative realization of holography in quasi-local regions and suggest avenues toward holographic renormalization in discrete gravity. The framework offers concrete tools for probing bulk-boundary correspondence in finite regions and for comparing non-perturbative gravity with perturbative AdS3/CFT2 insights.
Abstract
We present a line of research aimed at investigating holographic dualities in the context of three dimensional quantum gravity within finite bounded regions. The bulk quantum geometrodynamics is provided by the Ponzano-Regge state-sum model, which defines 3d quantum gravity as a discrete topological quantum field theory (TQFT). This formulation provides an explicit and detailed definition of the quantum boundary states, which allows a rich correspondence between quantum boundary conditions and boundary theories, thereby leading to holographic dualities between 3d quantum gravity and 2d statistical models as used in condensed matter. After presenting the general framework, we focus on the concrete example of the coherent twisted torus boundary, which allows for a direct comparison with other approaches to 3d/2d holography at asymptotic infinity. We conclude with the most interesting questions to pursue in this framework.
