Renormalization of 3d quantum gravity from matrix models
J. Ambjorn (NBI, Copenhagen), J. Jurkiewicz (U. Krakow), R. Loll, (Spinoza Inst., U. Utrecht)

TL;DR
This paper demonstrates how a 3D Lorentzian quantum gravity model, mapped to a two-matrix model, exhibits additive renormalizations of key constants, providing insights into its non-perturbative structure.
Contribution
It introduces a mapping of 3D Lorentzian quantum gravity to a two-matrix model, revealing renormalization behavior of gravitational constants.
Findings
Cosmological constant undergoes additive renormalization.
Gravitational coupling constant is renormalized consistently with canonical quantization.
Model provides a non-perturbative framework for 3D quantum gravity.
Abstract
Lorentzian simplicial quantum gravity is a non-perturbatively defined theory of quantum gravity which predicts a positive cosmological constant. Since the approach is based on a sum over space-time histories, it is perturbatively non-renormalizable even in three dimensions. By mapping the three-dimensional theory to a two-matrix model with ABAB interaction we show that both the cosmological and the (perturbatively) non-renormalizable gravitational coupling constant undergo additive renormalizations consistent with canonical quantization.
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