On propagation in Loop Quantum Gravity
Thomas Thiemann, Madhavan Varadarajan

TL;DR
This paper demonstrates that in a simplified U(1)^3 model of Loop Quantum Gravity, solutions to the Hamiltonian constraint exhibit propagation, challenging previous criticisms of locality in the theory.
Contribution
The paper provides an analytical study of the U(1)^3 model, showing the existence of propagating solutions and addressing previous limitations in understanding LQG dynamics.
Findings
Existence of infinite solutions in the U(1)^3 model
Solutions are generally non-normalisable
Solutions exhibit propagation phenomena
Abstract
A rigorous implementation of the Wheeler-Dewitt equations was derived in the context of Loop Quantum Gravity (LQG) and was coined Quantum Spin Dynamics (QSD). The Hamiltonian constraint of QSD was criticised as being too local and to prevent "propagation" in canonical LQG. That criticism was based on an algorithm developed for QSD for generating solutions to the Wheeler-DeWitt equations. The fine details of that algorithm could not be worked out because the QSD Hamiltonian constraint makes crucial use of the volume operator which cannot be diagonalised analytically. In this paper, we consider the U(1) model for Euclidean vacuum LQG which consists in replacing the structure group SU(2) by U(1) and otherwise keeps all properties of the SU(2) theory intact. This enables analytical calculations and the fine details of the algorithm {\it can} be worked out. By considering one of…
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