Deformation Operators of Spin Networks and Coarse-Graining
Etera R. Livine
TL;DR
The paper develops a coarse-graining framework for spin networks in loop quantum gravity by gauge-fixing a bounded region to a single vertex, revealing a residual closure defect that encodes bulk curvature. It extends the SU(2) deformation/observables from a single vertex to boundary data of regions, preserving a universal U(N) structure on the boundary and introducing SL(2,C) boosts that map boundary data to closure-satisfying configurations. A Lorentz-invariant rest area emerges as a Casimir and potential observable with links to black hole physics, demonstrated concretely in a one-loop example. The work discusses the physical meaning of the closure defect, the tree-dependence of coarse-graining, and potential extensions to tagged/loopy spin networks and twistor formalisms, with implications for holography and quantum gravity dynamics.
Abstract
In the context of loop quantum gravity, quantum states of geometry are mathematically defined as spin networks living on graphs embedded in the canonical space-like hypersurface. In the effort to study the renormalisation flow of loop gravity, a necessary step is to understand the coarse-graining of these states in order to describe their relevant structure at various scales. Using the spinor network formalism to describe the phase space of loop gravity on a given graph, we focus on a bounded (connected) region of the graph and coarse-grain it to a single vertex using a gauge-fixing procedure. We discuss the ambiguities in the gauge-fixing procedure and their consequences for coarse-graining spin(or) networks. This allows to define the boundary deformations of that region in a gauge-invariant fashion and to identify the area preserving deformations as U(N) transformations similarly to the already well-studied case of a single intertwiner. The novelty is that the closure constraint is now relaxed and the closure defect interpreted as a local measure of the curvature inside the coarse-grained region. It is nevertheless possible to cancel the closure defect by a Lorentz boost. We further identify a Lorentz-invariant observable related to the area and closure defect, which we name "rest area". Its physical meaning remains an open issue.
