Five-dimensional Einstein-Chern-Simons cosmology
Fernando G\'omez, Samuel Lepe, Cristian Quinzacara, Patricio, Salgado

TL;DR
This paper explores a five-dimensional cosmological model based on Einstein-Chern-Simons gravity, derived from gauged Lie algebras, and compares its field equations with four-dimensional cosmology.
Contribution
It introduces a novel five-dimensional Einstein-Chern-Simons cosmological model using S-expansion of Lie algebras, extending previous four-dimensional frameworks.
Findings
Derivation of field equations from Anti-de Sitter and de Sitter algebras.
Identification of analogies with four-dimensional cosmological models.
Analysis of matter and gravitational sectors in five dimensions.
Abstract
We consider a five-dimensional Einstein-Chern-Simons action which is composed of a gravitational sector and a sector of matter, where the gravitational sector is given by a Chern-Simons gravity action instead of the Einstein-Hilbert action, and where the matter sector is given by a perfect fluid. The gravitational lagrangian is obtained gauging some Lie-algebras, which in turn, were obtained by S-expansion procedure of Anti-de Sitter and de Sitter algebras. On the cosmological plane, we discuss the field equations resulting from the Anti-de Sitter and de Sitter frameworks and we show analogies with four-dimensional cosmological schemes.
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