A von Neumann algebraic approach to Quantum Theory on curved spacetime
Louis E Labuschagne, W Adam Majewski
TL;DR
The paper develops a von Neumann algebraic formulation of AQFT on curved spacetime, replacing a global Hilbert space with local standard-forms to obtain a locally covariant, tensorial framework. It demonstrates how Killing local flows lift to automorphisms of local algebras and establishes conditions for quantum Lie derivatives, while constructing representations via Araki–Woods factors from quasi-free, particularly Hadamard, states. The work also integrates Orlicz-space techniques to accommodate unbounded field observables and discusses implications for semiclassical gravity through well-defined stress-energy expectations. Collectively, the results provide a robust, entanglement-capable, locally covariant AQFT on globally hyperbolic spacetimes, with a clear path toward including broader observables and applications to curved-background dynamics.
Abstract
By extending the method developed in our recent paper \cite{LM} we present the AQFT framework in terms of von Neumann algebras. In particular, this approach allows for a locally covariant categorical description of AQFT which moreover satisfies the additivity property and provides a natural and intrinsic framework for a description of entanglement. Turning to dynamical aspects of QFT we show that Killing local flows may be lifted to the algebraic setting in curved space-time. Furthermore, conditions under which quantum Lie derivatives of such local flows exist are provided. The central question that then emerges is how such quantum local flows might be described in interesting representations. We show that quasi-free representations of Weyl algebras fit the presented framework perfectly. Finally, the problem of enlarging the set of observables is discussed. We point out the usefulness of Orlicz space techniques to encompass unbounded field operators. In particular, a well-defined framework within which one can manipulate such operators is necessary for the correct presentation of (semiclassical) Einstein's equation.
