Randall-Sundrum brane universe as a ground state for Chern-Simons gravity
Fabrizio Cordonier-Tello, Fernando Izaurieta, Patricio Mella, Eduardo, Rodr\'iguez

TL;DR
This paper demonstrates that a Randall-Sundrum brane universe can serve as a vacuum solution in five-dimensional Chern-Simons gravity, supporting linear gravitational perturbations and linking the solution to the algebraic structure of the spacetime.
Contribution
It introduces a novel interpretation of the Randall-Sundrum brane as a ground state in Chern-Simons gravity, incorporating non-zero torsion and group manifold properties.
Findings
Linear perturbations behave as standard gravitational waves.
The solution leads to a four-dimensional cosmological function depending on the Euler density.
The spacetime's group manifold structure is key to its role as a ground state.
Abstract
In stark contrast with the three-dimensional case, higher-dimensional Chern-Simons theories can have non-topological, propagating degrees of freedom. Finding those vacua that allow for the propagation of linear perturbations, however, proves to be surprisingly challenging. The simplest solutions are somehow "hyper-stable," preventing the construction of realistic, four-dimensional physical models. Here, we show that a Randall-Sundrum brane universe can be regarded as a vacuum solution of Chern-Simons gravity in five-dimensional spacetime, with non vanishing torsion along the dimension perpendicular to the brane. Linearized perturbations around this solution not only exist, but behave as standard gravitational waves on a four-dimensional Minkowski background. In the non-perturbative regime, the solution leads to a four-dimensional "cosmological function" …
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