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  • Open Access

Structure of the continuum limit of spin foams

Matteo Bruno*

Eugenia Colafranceschi†

Fabio M. Mele‡

Carlo Rovelli§

  • *Contact author: bruno@cpt.univ-mrs.fr
  • †Contact author: ecolafra@ucm.es
  • ‡Contact author: fmele1@lsu.edu
  • §Contact author: crovelli@uwo.ca

Phys. Rev. D 114, 066005 – Published 8 September, 2026

DOI: https://doi.org/10.1103/7493-9nb7

Abstract

The spin foam approach to quantum gravity aims at providing a covariant path-integral formulation of canonical loop quantum gravity. Since spin foam amplitudes are defined through discretizations of spacetime, understanding the continuum limit of the theory remains a central open problem. In this work, we investigate the structural aspects of this limit in a model-independent manner. We introduce an axiomatic framework for spin foam amplitudes inspired by Atiyah’s formulation of topological quantum field theories (TQFTs). In this setting, Hilbert spaces and amplitudes are assigned to combinatorial and topological data associated with triangulated manifolds. By equipping the set of triangulations with suitable orders, this framework provides a precise notion of continuum limit and allows us to analyse its properties independently of any specific model. We systematically investigate how the specifics of the limit procedure allow to go beyond TQFT in the continuum. Under natural assumptions on the convergence of spin foam amplitudes, we establish a no-go result: sufficiently strong notions of convergence necessarily lead to a topological theory. Motivated by this obstruction, we weaken the notion of convergence and consider the continuum limit of spin foam amplitudes in a distributional sense, in the spirit of refined algebraic quantization. Under this assumption, the amplitude associated with the cylinder defines a rigging map, yielding a canonical construction of the physical Hilbert space. The resulting continuum amplitudes act as well-defined distributions on this space of physical states, characterizing this formulation of the gravitational path integral as physical in a precise sense.

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