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Holographic dark energy and the universe expansion acceleration

dc.contributor.authorAlmeida, JPB
dc.contributor.authorPereira, J. G.
dc.contributor.institutionUniversidade Estadual Paulista (Unesp)
dc.date.accessioned2014-05-20T14:07:46Z
dc.date.available2014-05-20T14:07:46Z
dc.date.issued2006-05-04
dc.description.abstractBy incorporating the holographic principle in a time-depending Lambda-term cosmology, new physical bounds on the arbitrary parameters of the model can be obtained. Considering then the dark energy as a purely geometric entity, for which no equation of state has to be introduced, it is shown that the resulting range of allowed values for the parameters may explain both the coincidence problem and the universe accelerated expansion, without resorting to any kind of additional structures. (C) 2006 Elsevier B.V. All rights reserved.en
dc.description.affiliationUniv Estadual Paulista, Inst Fis Teor, BR-01405900 São Paulo, Brazil
dc.description.affiliationUnespUniv Estadual Paulista, Inst Fis Teor, BR-01405900 São Paulo, Brazil
dc.format.extent75-79
dc.identifierhttp://dx.doi.org/10.1016/j.physletb.2006.02.069
dc.identifier.citationPhysics Letters B. Amsterdam: Elsevier B.V., v. 636, n. 2, p. 75-79, 2006.
dc.identifier.doi10.1016/j.physletb.2006.02.069
dc.identifier.issn0370-2693
dc.identifier.lattes1599966126072450
dc.identifier.urihttp://hdl.handle.net/11449/23805
dc.identifier.wosWOS:000237397800001
dc.language.isoeng
dc.publisherElsevier B.V.
dc.relation.ispartofPhysics Letters B
dc.relation.ispartofjcr4.254
dc.relation.ispartofsjr2,336
dc.rights.accessRightsAcesso restrito
dc.sourceWeb of Science
dc.titleHolographic dark energy and the universe expansion accelerationen
dc.typeArtigo
dcterms.licensehttp://www.elsevier.com/about/open-access/open-access-policies/article-posting-policy
dcterms.rightsHolderElsevier B.V.
dspace.entity.typePublication
unesp.author.lattes1599966126072450
unesp.campusUniversidade Estadual Paulista (UNESP), Instituto de Física Teórica (IFT), São Paulopt

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