Spacetime geometry from algebra: spin foam models for non-perturbative quantum gravity
Daniele Oriti
TL;DR
This work surveys spin foam models as a covariant, non-perturbative approach to quantum gravity, foregrounding the Barrett-Crane Euclidean 4D model. It connects BF theory and the Plebanski formulation to gravity via simplicity and closure constraints, yielding a finite, gauge-invariant state-sum that encodes quantum geometry through labeled 2-complexes. A key contribution is showing how spin foams act as histories of spin networks, with group-field theory providing a natural framework to sum over foams and triangulations and to define quantum gravity observables. The Lorentzian extension, finiteness results, and the links to group field theories illuminate a path toward a background-independent quantum theory of spacetime, while highlighting open issues in the classical limit, causality, and coupling to matter. The paper thus consolidates a coherent, algebraic picture of quantum spacetime and outlines avenues toward unification with broader non-perturbative programs and potential phenomenology.
Abstract
This is an introduction to spin foam models for non-perturbative quantum gravity, an approach that lies at the point of convergence of many different research areas, including loop quantum gravity, topological quantum field theories, path integral quantum gravity, lattice field theory, matrix models, category theory, statistical mechanics. We describe the general formalism and ideas of spin foam models, the picture of quantum geometry emerging from them, and give a review of the results obtained so far, in both the Euclidean and Lorentzian case. We focus in particular on the Barrett-Crane model for 4-dimensional quantum gravity.
