dc.creatorUniversidad San Sebastián
dc.creatorUniversidad San Sebastián
dc.creatorUniversidad San Sebastián
dc.creatorUniversidad San Sebastián
dc.creatorGómez, F.
dc.creatorLepe, S.
dc.creatorQuinzacara, C.
dc.creatorSalgado, P.
dc.date.accessioned2023-05-24T04:57:53Z
dc.date.available2023-05-24T04:57:53Z
dc.date.created2023-05-24T04:57:53Z
dc.date.issued2021-05-15
dc.identifier2470-0010
dc.identifierhttps://repositorio.uss.cl/handle/uss/6948
dc.identifier10.1103/PhysRevD.103.104058
dc.description.abstractWe 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.
dc.languageeng
dc.relationPhysical Review D
dc.titleFive-dimensional Einstein-Chern-Simons cosmology
dc.typeArtículo


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