Curvature in spinfoams
Elena Magliaro and Claudio Perini
Institute for Gravitation and the Cosmos, Physics Department,
Penn State, University Park, PA 16802-6300, USA
(Dated: June 10, 2018)
We consider spinfoam quantum gravity. We show in a simple case that the amplitude projects over a nontrivial (curved) classical geometry. This suggests that, at least for spinfoams without bubbles and for large values of the boundary spins, the amplitude takes the form of a path integral over Regge metrics, thus enforcing discrete Einstein equations in the classical limit. The result relies crucially on a new interpretation of the semiclassical limit for the amplitudes truncated to a fixed 2-complex.
The physical picture emerging from the spinfoam gravity is that of a discrete, combinatorial spacetime structure (a quantum foam of virtual geometries), where the Plank scale plays the role of a
natural minimal length. Spinfoams are the result of the quantization of general relativity formulated as a constrained BF theory.