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Modified teleparallel theories of gravity in symmetric spacetimes

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arxiv 1901.05472 v3 pith:FHHDCIJK submitted 2019-01-16 gr-qc hep-thmath-phmath.MP

classification gr-qchep-thmath-phmath.MP
keywords symmetrygravityteleparallelcosmologicalspintetradsconnectionequations
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abstract

Teleparallel gravity theories employ a tetrad and a Lorentz spin connection as independent variables in their covariant formulation. In order to solve their field equations, it is helpful to search for solutions which exhibit certain amounts of symmetry, such as spherical or cosmological symmetry. In this article we present how to apply the notion of spacetime symmetries known from Cartan geometry to teleparallel geometries. We explicitly derive the most general tetrads and spin connections which are compatible with axial, spherical, cosmological and maximal symmetry. For homogeneous and isotropic spacetime symmetry we find that the tetrads and spin connection found by the symmetry constraints are universal solutions to the anti-symmetric part of the field equations of any teleparallel theory of gravity. In other words, for cosmological symmetry we find what has become known as "good tetrads" in the context of $f(T)$ gravity.

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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. Degenerate and connection-dependent cosmological sectors in f(Q,C) gravity

    gr-qc 2026-07 conditional novelty 6.0 of 10

    Connection field equations force a degenerate f(R)-equivalent sector of f(Q,C) cosmology in which three geometric connections coincide, and only nonzero integration constants make the connections physically distinct.

  2. Quintessence dark energy model in non-linear $f(Q)$ theory with bulk-viscosity

    gr-qc 2025-06 reject novelty 4.0 of 10

    A quadratic f(Q) gravity model with bulk viscosity is fitted to expansion data, but the reported Hubble-law formula contradicts the paper's own scale-factor solution.

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