Vacuum Structure of Cosmologically Viable Quadratic Modifications of Gravity that are Functions of the Gauss-Bonnet Invariant

TL;DR

This paper analyzes the stability of quadratic gravity theories involving the Gauss-Bonnet invariant, identifying conditions under which they are free of instabilities like ghosts and tachyons, crucial for their viability in cosmology and solar system tests.

Contribution

It provides a comprehensive stability analysis of quadratic Gauss-Bonnet gravity modifications, highlighting the unavoidable instabilities in many viable models.

Findings

Many cosmologically and solar system viable theories are ruled out due to instabilities.

Identification of conditions to avoid ghost and tachyonic modes.

First detailed stability study of quadratic Gauss-Bonnet modifications.

Abstract

We perform a thorough study of the theoretical consistency of recently proposed, viable, quadratic modifications of gravity that are functions of the the Gauss-Bonnet invariant, regarding the stability of their perturbations around vacuum, maximally symmetric spaces of constant curvature. We pay special attention, in particular, to the investigation of pathological instabilities associated with the occurrence of propagating spin-0 tachyon modes, and with the development of a graviton ghost. The latter effect is associated with the known "Ricci stability" issue, well studied in $f(R)$-theories. Within quadratic modifications of gravity it is discussed for the first time. Special attention is paid to the requirement of non-negativity of the effective gravitational coupling, which warrants that the graviton is not a negative-norm state. It is demonstrated that, several theories that pass the cosmological as well as the solar system tests, have to be rule out on the basis of the unavoidable character of these pathological instabilities.