Pith. sign in

REVIEW 3 cited by

Covariant path integrals for quantum fields back-reacting on classical space-time

Not yet reviewed by Pith; the record is open.

This paper has not been read by Pith yet. Machine review is queued; the pith claim, tier, and objections will appear here once it completes.

SPECIMEN: schema-true, not a live event

T0 review · schema-true

One-sentence machine reading of the paper's core claim.

pith:XXXXXXXX · record.json · timestamp

arxiv 2302.07283 v3 pith:NWNA2RMB submitted 2023-02-14 gr-qc hep-thquant-ph

classification gr-qchep-thquant-ph
keywords pathquantumclassicaltheoryfieldsintegralintegralsspace-time
verification ladder T0 review T1 audit T2 compute T3 formal
0 comments
read the original abstract

We introduce configuration space path integrals for quantum fields interacting with classical fields. We show that this can be done consistently by proving that the dynamics are completely positive directly, without resorting to master equation methods. These path integrals allow one to readily impose space-time symmetries, including Lorentz invariance or diffeomorphism invariance. They generalize and combine the Feynman-Vernon path integral of open quantum systems and the stochastic path integral of classical stochastic dynamics while respecting symmetry principles. We introduce a path integral formulation of general relativity where the space-time metric is treated classically. The theory is a candidate for a fundamental theory that reconciles general relativity with quantum mechanics. The theory is manifestly covariant, and may be inequivalent to the theory derived using master-equation methods. We prove that entanglement cannot be created via the classical field, reinforcing proposals to test the quantum nature of gravity via entanglement generation.

Discussion (0). Continue with ORCID to comment.

Forward citations

Cited by 3 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Classical theories of gravity produce entanglement

    quant-ph 2025-10 conditional novelty 7.0 of 10

    In quantum field theory, a classical gravitational potential can entangle two superposed masses through virtual matter exchange, so gravitationally induced entanglement is not by itself proof of quantum gravity.

  2. Testing classical-quantum gravity with geodesic deviation

    gr-qc 2026-03 conditional novelty 6.0 of 10

    Analytic strain spectra of geodesic deviation in Oppenheim CQ gravity are testable by current GW detectors and, combined with prior bounds, can exclude the original white-noise model.

  3. A Spin-Based Pathway to Testing the Quantum Nature of Gravity

    quant-ph 2025-09 unverdicted novelty 3.0 of 10

    A review and roadmap for using spin-based Stern-Gerlach superpositions of NV-center diamonds to test the quantum nature of gravity via gravitationally induced entanglement.

Pith tools