Ponzano-Regge model revisited III: Feynman diagrams and Effective field theory
Laurent Freidel, Etera R. Livine
TL;DR
This work connects 3D quantum gravity spin foams (Ponzano–Regge and Turaev–Viro) with conventional quantum field theory by focusing on matter couplings and the no-gravity limit. It shows that Feynman amplitudes emerge as abelian spin-foam evaluations in the $G_N o0$ limit, while finite gravity yields a non-commutative, braided effective field theory governed by a κ-Poincaré symmetry and a star-product on Lie algebra variables. The paper develops a rigorous framework for particle propagation in quantum geometry, including explicit Feynman rules, braiding, and a causal (Lorentzian) extension, and demonstrates how different cosmological constants lead to distinct state-sum limits (PR, TV, hyperbolic) with corresponding propagators. Together, these results provide a principled path from quantum gravity to an effective non-commutative field theory, highlighting the role of doubly special relativity and non-trivial spacetime braiding in 3D. The findings have potential implications for understanding matter dynamics in quantum spacetime and guiding extensions to higher-dimensional models.
Abstract
We study the no gravity limit G_{N}-> 0 of the Ponzano-Regge amplitudes with massive particles and show that we recover in this limit Feynman graph amplitudes (with Hadamard propagator) expressed as an abelian spin foam model. We show how the G_{N} expansion of the Ponzano-Regge amplitudes can be resummed. This leads to the conclusion that the dynamics of quantum particles coupled to quantum 3d gravity can be expressed in terms of an effective new non commutative field theory which respects the principles of doubly special relativity. We discuss the construction of Lorentzian spin foam models including Feynman propagators
