Chern–Simons gravity in four dimensions

dc.contributor.authorMorales, Ivan
dc.contributor.authorNeves, Bruno
dc.contributor.authorOporto, Zui
dc.contributor.authorPiguet, Olivier
dc.date.accessioned2019-01-21T13:45:43Z
dc.date.available2019-01-21T13:45:43Z
dc.date.issued2017-02
dc.description.abstractFive-dimensional Chern–Simons theory with (anti-)de Sitter SO(1,5) or SO(2,4) gauge invariance presents an alternative to general relativity with cosmological constant. We consider the zero modes of its Kaluza–Klein compactification to four dimensions. Solutions with vanishing torsion are obtained in the cases of a spherically symmetric 3-space and of a homogeneous and isotropic 3-space, which reproduce the Schwarzshild–de Sitter and ΛΛ CDM cosmological solutions of general relativity. We also check that vanishing torsion is a stable feature of the solutions.en
dc.formatpdfpt-BR
dc.identifier.issn1434-6052
dc.identifier.urihttps://doi.org/10.1140/epjc/s10052-017-4653-8
dc.identifier.urihttp://www.locus.ufv.br/handle/123456789/23113
dc.language.isoengpt-BR
dc.publisherThe European Physical Journal Cpt-BR
dc.relation.ispartofseriesVolume 77, Issue 87, February 2017pt-BR
dc.rightsOpen Accesspt-BR
dc.subjectGauge grouppt-BR
dc.subjectField equationpt-BR
dc.subjectCosmological constantpt-BR
dc.subjectCosmological solutionpt-BR
dc.subjectSimons theorypt-BR
dc.titleChern–Simons gravity in four dimensionsen
dc.typeArtigopt-BR

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