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Ghost and Laplacian Instabilities in the Teleparallel Horndeski Gravity

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arxiv 2301.04457 v2 pith:CYGXWMXK submitted 2023-01-11 gr-qc astro-ph.COhep-th

classification gr-qcastro-ph.COhep-th
keywords gravityteleparallelhorndeskimodelsclassgeometryghostinstabilities
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Teleparallel geometry offers a platform on which to build up theories of gravity where torsion rather than curvature mediates gravitational interaction. The teleparallel analogue of Horndeski gravity is an approach to teleparallel geometry where scalar-tensor theories are considered in this torsional framework. Being teleparallel gravity of lower order in dynamics, this turns out to be more general than metric Horndeski gravity. In other words, the class of teleparallel Horndeski gravity models is much broader than the standard metric one. In this work, we explore constraints on this wide range of models coming from ghost and Laplacian instabilities. The aim is to limit pathological branches of the theory by fundamental considerations. It is possible to conclude that a very large class of models results physically viable.

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  1. Propagating Gravitational Waves in Teleparallel Gauss-Bonnet Gravity

    gr-qc 2025-05 conditional novelty 6.0 of 10

    Tensor perturbations in F(T,T_G) teleparallel gravity produce gravitational waves that propagate at the speed of light, with a modified amplitude.

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