Quantum Holonomy Theory
Johannes Aastrup, Jesper M. Grimstrup

TL;DR
Quantum holonomy theory offers a non-perturbative framework for quantum gravity coupled with fermions, deriving classical constraints and fermionic dynamics from a novel algebraic and geometric approach.
Contribution
It introduces a new non-perturbative quantum gravity model based on holonomy-diffeomorphisms and Dirac operators, linking quantum gravity with fermionic fields.
Findings
Classical Hamiltonian constraint emerges in semi-classical limit
Operator constraint algebra reproduces classical relations
States connect Dirac operator expectation to fermionic Hamiltonian
Abstract
We present quantum holonomy theory, which is a non-perturbative theory of quantum gravity coupled to fermionic degrees of freedom. The theory is based on a C*-algebra that involves holonomy-diffeomorphisms on a 3-dimensional manifold and which encodes the canonical commutation relations of canonical quantum gravity formulated in terms of Ashtekar variables. Employing a Dirac type operator on the configuration space of Ashtekar connections we obtain a semi-classical state and a kinematical Hilbert space via its GNS construction. We use the Dirac type operator, which provides a metric structure over the space of Ashtekar connections, to define a scalar curvature operator, from which we obtain a candidate for a Hamilton operator. We show that the classical Hamilton constraint of general relativity emerges from this in a semi-classical limit and we then compute the operator constraint…
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