Spin Foam Models for Quantum Gravity
Alejandro Perez
TL;DR
<3-5 sentence high-level summary> The paper surveys spin foam formulations as a background-independent, covariant approach to quantum gravity, connecting Loop Quantum Gravity to a path-integral-like sum over histories of quantum geometry. It analyzes how 4D gravity can be modeled as constrained BF theory, with Barrett–Crane as a central example and a comprehensive group-field-theory (GFT) reformulation that yields a discretization-independent description. Finite results and integral representations for both Riemannian and Lorentzian versions are presented, alongside asymptotic analyses of vertex amplitudes and discussions of discretization, gauge issues, and the continuum limit. The work clarifies the landscape of spin foams, highlights key achievements in finiteness and GFT connections, and identifies open problems in achieving a viable low-energy limit and a robust renormalization framework for quantum gravity.
Abstract
In this article we review the present status of the spin foam formulation of non-perturbative (background independent) quantum gravity. The article is divided in two parts. In the first part we present a general introduction to the main ideas emphasizing their motivations from various perspectives. Riemannian 3-dimensional gravity is used as a simple example to illustrate conceptual issues and the main goals of the approach. The main features of the various existing models for 4-dimensional gravity are also presented here. We conclude with a discussion of important questions to be addressed in four dimensions (gauge invariance, discretization independence, etc.). In the second part we concentrate on the definition of the Barrett-Crane model. We present the main results obtained in this framework from a critical perspective. Finally we review the combinatorial formulation of spin foam models based on the dual group field theory technology. We present the Barrett-Crane model in this framework and review the finiteness results obtained for both its Riemannian as well as its Lorentzian variants.
