Modified gravity, the Cascading DGP model and its critical tension

TL;DR

This paper analyzes the stability of the Cascading DGP modified gravity model, identifying a critical tension scale linked to ghost instabilities, which impacts the model's viability for explaining cosmic acceleration.

Contribution

It introduces a detailed perturbation analysis of the Cascading DGP model, revealing a critical tension scale that influences ghost instabilities and clarifies discrepancies with previous studies.

Findings

Identification of a critical tension scale affecting stability

Derivation of a master equation governing scalar perturbations

Numerical validation of the analytical results

Abstract

We investigate the presence of instabilities in the Cascading DGP model. We start by discussing the problem of the cosmological late time acceleration, and we introduce the modified gravity approach. We then focus on brane induced gravity models and in particular on the Cascading DGP model. We consider configurations of the latter model where the source term is given simply by vacuum energy (pure tension), and we study perturbations at first order around these configurations. We perform a four-dimensional scalar-vector-tensor decomposition of the perturbations, and show that, regarding the scalar sector, the dynamics in a suitable limit can be described by a master equation. This master equation contains an energy scale (critical tension) which is related in a non-trivial way to the parameters of the model. We give a geometrical interpretation of why this scale emerges, and explain its relevance for the presence of ghost instabilities in the theory. We comment on the difference between our result and the one present in the literature, and stress its importance regarding the phenomenological viability of the model. We finally provide a numerical check which confirms the validity of our analysis.