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Spacetime perturbations and quasi-teleparallel gravity

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arxiv 2503.03119 v2 pith:NPSBNZD7 submitted 2025-03-05 gr-qc astro-ph.COhep-th

classification gr-qcastro-ph.COhep-th
keywords perturbationspacetimegravitybackgroundnon-metricityriemannianteleparalleltorsion
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Gravity is identical to curved spacetime. It is manifested by the curvature of a Riemannian spacetime in general relativity but by torsion or non-metricity in teleparallel gravity models. In this paper, we apply these multiple options to the spacetime perturbation theory and seek the possibilities of representing the gravitation of the background and that of the perturbation in separate ways. We show that the perturbation around a Riemannian background can be described by torsion or non-metricity, so that we have teleparallel like actions for the perturbation.

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  1. Correlated parity violation in gravity and electromagnetism from five-dimensional spacetime

    gr-qc 2026-08 conditional novelty 7.0 of 10

    A five-dimensional teleparallel Kaluza-Klein action produces a single parameter-free prediction: the electromagnetic helicity dispersion shift is exactly six times the gravitational one.

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