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No further gravitational wave modes in $F(T)$ gravity

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arxiv 1309.2698 v2 pith:YB76IKOH submitted 2013-09-11 gr-qc astro-ph.COhep-th

Kazuharu Bamba , Salvatore Capozziello , Mariafelicia De Laurentis , Shin'ichi Nojiri , Diego Sáez-Gómez This is my paper · ORCID
classification gr-qcastro-ph.COhep-th
keywords gravitygravitationalmodeswavefurtherlimitachievedanalysis
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abstract

We explore the possibility of further gravitational wave modes in $F(T)$ gravity, where $T$ is the torsion scalar in teleparallelism. It is explicitly demonstrated that gravitational wave modes in $F(T)$ gravity are equivalent to those in General Relativity. This result is achieved by calculating the Minkowskian limit for a class of analytic function of $F(T)$. This consequence is also confirmed by the preservative analysis around the flat background in the weak field limit with the scalar-tensor representation of $F(T)$ gravity.

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Cited by 2 Pith papers

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  1. Conformal Gravity and Transformations in the Symmetric Teleparallel Framework

    gr-qc 2019-08 conditional novelty 6.0 of 10

    A conformally invariant gravity action built from the square of a non-metricity scalar gives second-order field equations in symmetric teleparallel gravity.

  2. ACT-DR6 consistent inflation in generalised entropic cosmology and $f(Q)$ gravity

    gr-qc 2026-07 conditional novelty 4.0 of 10

    Reconstruction produces explicit f(Q) and generalised-entropic inflation models (and scalar-coupled versions) whose slow-roll parameters match ACT-DR6 + Planck-BAO constraints on n_s and r.

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