On the regularization of the constraints algebra of Quantum Gravity in 2+1 dimensions with non-vanishing cosmological constant
Alejandro Perez, Daniele Pranzetti
TL;DR
The paper investigates the canonical quantization of 2+1 dimensional Riemannian gravity with a positive cosmological constant within loop quantum gravity. Using a holonomy-flux regularization on a cellular discretization, it shows that while the Gauss constraint algebra remains anomaly-free, the regulated curvature constraint algebra develops a genuine quantum anomaly proportional to $\Lambda$ and the local curvature term $\operatorname{tr}[W]-2$, persisting in the continuum limit. This deformation indicates a deformation of the diffeomorphism-related symmetry, posing a major challenge for Dirac-type quantization and suggesting links to quantum-group structures that arise in gravity with $\Lambda>0$. The results highlight a fundamental obstacle to extending the LQG program to nonzero cosmological constant in 2+1 dimensions and motivate exploring alternative quantization schemes like master constraint methods.
Abstract
We use the mathematical framework of loop quantum gravity (LQG) to study the quantization of three dimensional (Riemannian) gravity with positive cosmological constant (Lambda>0). We show that the usual regularization techniques (successful in the Lambda=0 case and widely applied in four dimensional LQG) lead to a deformation of the classical constraint algebra (or anomaly) proportional to the local strength of the curvature squared. We argue that this is an unavoidable consequence of the non-local nature of generalized connections.
