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Quantum corrected equations of motion in the interior and exterior Schwarzschild spacetime

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arxiv 2007.05416 v1 pith:4JPZ7DYJ submitted 2020-07-10 hep-th

Xavier Calmet , Roberto Casadio , Folkert Kuipers This is my paper · ORCID
classification hep-th
keywords quantumcorrectionsdensityequationsgravitymotionspacetimeadditional
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In this paper we derive the leading quantum gravitational corrections to the geodesics and the equations of motion for a scalar field in the spacetime containing a constant density star. It is shown that these corrections can be calculated in quantum gravity reliably and in a model independent way. Furthermore, we find that quantum gravity gives rise to an additional redshift that results from the gradient instead of the amplitude of the density profile.

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Cited by 1 Pith paper

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

  1. Properties of compact objects in quadratic non-metricity gravity

    gr-qc 2025-07 reject novelty 4.0 of 10

    Quadratic non-metricity gravity with a fitted coupling ξ can match PSR J0740+6620 while keeping the radial sound speed below c²/3, according to the paper's chosen metric ansatz.

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