A transition from a decelerated to an accelerated phase of the universe expansion from the simplest non-trivial polynomial function of T in the f(R, T) formalism

dc.contributor.authorMoraes, P. H.R.S.
dc.contributor.authorRibeiro, G.
dc.contributor.authorCorrea, R. A.C.
dc.contributor.institutionITA – Instituto Tecnológico de Aeronáutica
dc.contributor.institutionFEG – Faculdade de Engenharia de Guaratinguetá
dc.contributor.institutionUniversidade Federal do ABC (UFABC)
dc.date.accessioned2022-04-29T08:45:00Z
dc.date.available2022-04-29T08:45:00Z
dc.date.issued2016-07-01
dc.description.abstractIn this work we present cosmological solutions from the simplest non-trivial polynomial function of T in f(R, T) theory of gravity, with R and T standing for the Ricci scalar and trace of the energy-momentum tensor, respectively. Although such an approach yields a highly non-linear differential equation for the scale factor, we show that it is possible to obtain analytical solutions for the cosmological parameters. For some values of the free parameters, the model is able to predict a transition from a decelerated to an accelerated expansion of the universe and the values of the deceleration parameter agree with observation.en
dc.description.affiliationDepartamento de Física ITA – Instituto Tecnológico de Aeronáutica
dc.description.affiliationDepartamento de Física e Química FEG – Faculdade de Engenharia de Guaratinguetá
dc.description.affiliationCCNH Universidade Federal do ABC
dc.identifierhttp://dx.doi.org/10.1007/s10509-016-2788-y
dc.identifier.citationAstrophysics and Space Science, v. 361, n. 7, 2016.
dc.identifier.doi10.1007/s10509-016-2788-y
dc.identifier.issn1572-946X
dc.identifier.issn0004-640X
dc.identifier.scopus2-s2.0-84975853476
dc.identifier.urihttp://hdl.handle.net/11449/231377
dc.language.isoeng
dc.relation.ispartofAstrophysics and Space Science
dc.sourceScopus
dc.subjectCosmic acceleration
dc.subjectCosmological models
dc.subjectf(R, T) gravity
dc.titleA transition from a decelerated to an accelerated phase of the universe expansion from the simplest non-trivial polynomial function of T in the f(R, T) formalismen
dc.typeArtigo

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