Cosmological teleparallel perturbations
Lavinia Heisenberg, Manuel Hohmann, Simon Kuhn

TL;DR
This paper investigates cosmological perturbations in various teleparallel gravity theories, revealing the presence of multiple degrees of freedom, ghost instabilities, and strong coupling issues, thus highlighting challenges in these models.
Contribution
It provides a comprehensive analysis of perturbations in $f(G)$, $f(T)$, and $f(Q)$ gravity, including connection degrees of freedom, and identifies stability issues in these theories.
Findings
Up to seven degrees of freedom in $f(Q)$ backgrounds.
Only two tensor modes propagate in $f(G)$ and $f(T)$ gravity.
Presence of ghost degrees of freedom and strong coupling problems.
Abstract
There has been growing interest in gravity, which has led to significant advancements in the field. However, it is important to note that most studies in this area were based on the coincident gauge, thus overlooking the impact of the connection degrees of freedom. In this work, we pay special attention to the connection when studying perturbations in general teleparallel, metric teleparallel, and symmetric teleparallel theories of gravity. We do not just examine perturbations in the metric, but also in the affine connection. To illustrate this, we investigate cosmological perturbations in , , and gravity with and without matter in form of an additional scalar field for spatially flat and curved FLRW geometries. Our perturbative analysis reveals that for general backgrounds, there are up to seven degrees of freedom, depending on the background…
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Taxonomy
TopicsCosmology and Gravitation Theories · Astrophysics and Cosmic Phenomena · Solar and Space Plasma Dynamics
