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Non-commutative Geometry from Perturbative Quantum Gravity

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arxiv 2207.03345 v3 pith:ZA2D7EGQ submitted 2022-07-06 gr-qc

classification gr-qc
keywords quantumgravityperturbativenon-commutativeeffectsnon-commutativityquestionaffirmative
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Trying to connect a fundamentally non-commutative spacetime with the conservative perturbative approach to quantum gravity, we are led to the natural question: are non-commutative geometrical effects already present in the regime where perturbative quantum gravity provides a predictive framework? Moreover, is it necessary to introduce non-commutativity by hand, or does it arise through quantum-gravitational effects? We show that the first question can be answered in the affirmative, and the second one in the negative: perturbative quantum gravity predicts non-commutativity at the Planck scale, once one clarifies the structure of observables in the quantum theory.

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Cited by 4 Pith papers

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

  1. Relational path integral, effective actions and quantum frame covariance in gravity

    hep-th 2026-07 conditional novelty 7.0 of 10

    The gravitational path integral is reformulated with dynamical reference frames, producing gauge-invariant correlators, frame-dependent vacua, and effective actions, with sharpness of events becoming frame-relative.

  2. Crossed products and quantum reference frames: on the observer-dependence of gravitational entropy

    hep-th 2024-12 accept novelty 6.0 of 10

    Gravitational subregion entropy is observer-dependent: different quantum clocks produce different von Neumann algebras and different entropy functionals for the same global state.

  3. Linearization (in)stabilities and crossed products

    hep-th 2024-11 conditional novelty 6.0 of 10

    Second-order Taub charge constraints are justified as linearization stability conditions in spatially closed spacetimes, while in boundary or no-isometry cases the justification is weaker and depends on interest in se...

  4. Modified Mukhanov-Sasaki equation and primordial perturbations in $\kappa$-deformed non-commutative space-time

    gr-qc 2026-07 reject novelty 5.0 of 10

    A κ-deformed star product modifies the inflationary perturbation equation, yielding a (ln k)^2 correction to the power spectrum and a claimed ACT DR6 bound on the deformation length.

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