Cosmological stability in $f(\phi,{\cal G})$ gravity

TL;DR

This paper investigates the stability of scalar and tensor perturbations in a class of modified gravity theories involving a scalar field coupled to the Gauss-Bonnet term, revealing conditions under which these theories remain stable during cosmological evolution.

Contribution

It demonstrates that nonlinear functions of the Gauss-Bonnet term lead to instabilities in scalar perturbations during decelerating epochs, and identifies stable linear couplings as viable alternatives.

Findings

Nonlinear Gauss-Bonnet functions cause scalar instabilities in decelerating epochs.

Pure $f( ext{GB})$ gravity is unstable during radiation and matter eras.

Linear coupling $\xi() ext{GB}$ can be stable if subdominant.

Abstract

In gravitational theories where a canonical scalar field $\phi$ with a potential $V(\phi)$ is coupled to a Gauss-Bonnet (GB) term ${\cal G}$ with the Lagrangian $f(\phi,{\cal G})$, we study the cosmological stability of tensor and scalar perturbations in the presence of a perfect fluid. We show that, in decelerating cosmological epochs with a positive tensor propagation speed squared, the existence of nonlinear functions of ${\cal G}$ in $f$ always induces Laplacian instability of a dynamical scalar perturbation associated with the GB term. This is also the case for $f({\cal G})$ gravity, where the presence of nonlinear GB functions $f({\cal G})$ is not allowed during the radiation- and matter-dominated epochs. A linearly coupled GB term with $\phi$ of the form $\xi (\phi){\cal G}$ can be consistent with all the stability conditions, provided that the scalar-GB coupling is subdominant to the background cosmological dynamics.