Matrix model formulation of four dimensional gravity
R. De Pietri
TL;DR
The paper investigates extending the successful $2$-D matrix-model description of quantum gravity to $4$-D by using $n$-tensor models whose Feynman diagrams encode $n$-simplicial complexes. It develops a formalism where fat graphs correspond to the dual $2$-skeletons of triangulations, and derives manifold conditions (Cycl, Surf) needed for the resulting space to be a $4$-manifold, while highlighting that not all fat graphs satisfy these conditions. Recognizing this limitation, the authors advocate moving to group field theories on homogeneous spaces to weight diagrams by topological invariants such as the Ooguri–Crane–Yetter ($OCY$) and Barrett–Crane invariants, thereby discriminating admissible space-times and connecting to spin-foam approaches. The work thus links dynamical triangulations, tensor models, and group-field theory in an effort to construct a viable $4D$ quantum gravity framework with manifest combinatorial and topological control.
Abstract
The attempt of extending to higher dimensions the matrix model formulation of two-dimensional quantum gravity leads to the consideration of higher rank tensor models. We discuss how these models relate to four dimensional quantum gravity and the precise conditions allowing to associate a four-dimensional simplicial manifold to Feynman diagrams of a rank-four tensor model.
