Strong interactions and exact solutions in non-linear massive gravity

TL;DR

This paper studies strong coupling effects and exact solutions in a covariant non-linear massive gravity model, exploring conditions for recovering general relativity and potential cosmological implications of graviton mass.

Contribution

It provides a detailed analysis of strong coupling regimes, identifies conditions for the Vainshtein mechanism, and presents new exact vacuum solutions with cosmological relevance.

Findings

Vainshtein mechanism can recover GR in certain parameter regimes

Three main cases of non-linear behavior depending on parameters

Exact vacuum solutions asymptoting to de Sitter or anti de Sitter space

Abstract

We investigate strong coupling effects in a covariant massive gravity model, which is a candidate for a ghost free non-linear completion of Fierz-Pauli. We analyse the conditions to recover general relativity via Vainshtein mechanism in the weak field limit, and find three main cases depending on the choice of parameters. In the first case, the potential is such that all non-linearities disappear and the vDVZ discontinuity cannot be avoided. In the second case, the Vainshtein mechanism allows to recover general relativity within a macroscopic radius from a source. In the last case, the strong coupling of the scalar graviton completely shields the massless graviton, and weakens gravity when approaching the source. In the second part of the paper, we explore new exact vacuum solutions, that asymptote de Sitter or anti de Sitter space depending on the parameter choice. The curvature of the space is proportional to the mass of the graviton, thus providing a cosmological background which may explain the present day acceleration in terms of the graviton mass. Moreover, by expressing the potential for non-linear massive gravity in a convenient form, we also suggest possible connections with a higher dimensional framework.