Entanglement entropy in Loop Quantum Gravity and geometrical area law
Muxin Han
TL;DR
This work develops an algebraic framework for entanglement entropy in Loop Quantum Gravity, where gauge invariance prevents a simple factorization of the Hilbert space. By formulating entropy with non-factor von Neumann algebras and a renormalized trace, it derives a geometrical area law S ∝ Ar(𝒮) from fixed-area states and shows bulk entanglement can renormalize the area-law coefficient and produce logarithmic corrections. The analysis connects LQG microstate counting to black hole entropy and extends to infinite-dimensional settings, where edge modes and hidden sectors systematically account for boundary gauge freedoms. Overall, the paper provides a rigorous, gauge-consistent pathway from quantum geometry to horizon thermodynamics, clarifying how boundary and bulk degrees of freedom shape entanglement in quantum gravity.
Abstract
The non-factorizing nature of the Hilbert space in Loop Quantum Gravity (LQG) due to gauge invariance requires a generalized definition of entanglement entropy. This work employs the framework of von Neumann algebras to investigate the entanglement entropy in LQG. On a graph, the holonomy and flux operators within a region and on the boundary generate a non-factor type I von Neumann algebra, which is used to define the entanglement entropy for LQG states. This algebraic formalism is applied to ``fixed-area states''--superpositions of spin networks associated with a surface with a definite macroscopic area given by the LQG area spectrum. By maximizing the entropy, we derive a geometrical area law where the entanglement entropy is proportional to the area. In addition, we show that bulk entanglement can renormalize the area-law coefficient and produce logarithmic corrections. The results in this paper closely relate to LQG black hole entropy.
