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Non-commutative Geometry from Perturbative Quantum Gravity in de Sitter spacetime

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arxiv 2305.01517 v2 pith:CBS5NH25 submitted 2023-04-29 gr-qc

classification gr-qc
keywords non-commutativeapproachbackgroundcoordinatesdynamicalgravitynaturallyperturbative
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We show that a non-commutative structure arises naturally from perturbative quantum gravity in a de Sitter background metric. Our work builds on recent advances in the construction of observables in highly symmetric background spacetimes [Brunetti et al., JHEP 08, 032 (2016); Fr\"ob and Lima, Class. Quant. Grav. 35, 095010 (2018)], where the dynamical coordinates that are needed in the relational approach were established for such backgrounds to all orders in perturbation theory. We show that these dynamical coordinates that describe events in the perturbed spacetime are naturally non-commuting, and determine their commutator to leading order in the Planck length. Our result generalizes the causal non-commutative structure that was found using the same approach in Minkowski space [Fr\"ob, Much and Papadopoulos, Phys. Rev. D 107, 064041 (2023)].

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  1. 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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