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Metric perturbations in Noncommutative Gravity

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arxiv 2310.06038 v2 pith:QIGYFHT4 submitted 2023-10-09 hep-th gr-qcmath-phmath.MP

classification hep-thgr-qcmath-phmath.MP
keywords noncommutativegeneralgravitymetricperturbationstheoryalgebrabackground
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We use the framework of Hopf algebra and noncommutative differential geometry to build a noncommutative (NC) theory of gravity in a bottom-up approach. Noncommutativity is introduced via deformed Hopf algebra of diffeomorphisms by means of a Drinfeld twist. The final result of the construction is a general formalism for obtaining NC corrections to the classical theory of gravity for a wide class of deformations and a general background. This also includes a novel proposal for noncommutative Einstein manifold. Moreover, the general construction is applied to the case of a linearized gravitational perturbation theory to describe a NC deformation of the metric perturbations. We specifically present an example for the Schwarzschild background and axial perturbations, which gives rise to a generalization of the work by Regge and Wheeler. All calculations are performed up to first order in perturbation of the metric and noncommutativity parameter. The main result is the noncommutative Regge-Wheeler potential. Finally, we comment on some differences in properties between the Regge-Wheeler potential and its noncommutative counterpart.

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Cited by 2 Pith papers

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

  1. Corrections to Kerr-Newman black hole from Noncommutative Einstein-Maxwell equation

    gr-qc 2025-02 reject novelty 6.0 of 10

    The author states that a specific deformed Kerr-Newman metric and Seiberg-Witten modified potential solve the noncommutative Einstein-Maxwell equations to first order in the noncommutativity parameter, without showing...

  2. Noncommutative black holes: Topological bulk-boundary correspondence and Binary Merger Bounds

    gr-qc 2026-07 reject novelty 4.0 of 10

    For noncommutative RN-AdS black holes, the paper claims bulk and boundary thermodynamic topological charges equal to zero and derives perturbative second-law corrections to the remnant-mass bound.

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