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Please use this identifier to cite or link to this item: http://acervodigital.unesp.br/handle/11449/24147
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dc.contributor.authorBeltran Almeida, J. P.-
dc.contributor.authorMayor, C. S. O.-
dc.contributor.authorPereira, J. G.-
dc.date.accessioned2013-09-30T18:53:22Z-
dc.date.accessioned2014-05-20T14:09:22Z-
dc.date.accessioned2016-10-25T17:16:49Z-
dc.date.available2013-09-30T18:53:22Z-
dc.date.available2014-05-20T14:09:22Z-
dc.date.available2016-10-25T17:16:49Z-
dc.date.issued2012-07-01-
dc.identifierhttp://dx.doi.org/10.1134/S0202289312030012-
dc.identifier.citationGravitation & Cosmology. New York: Springer, v. 18, n. 3, p. 181-187, 2012.-
dc.identifier.issn0202-2893-
dc.identifier.urihttp://hdl.handle.net/11449/24147-
dc.identifier.urihttp://acervodigital.unesp.br/handle/11449/24147-
dc.description.abstractIn de Sitter special relativity, spacetime translations are replaced by a combination of translations and proper conformal transformations. As a consequence, the energy-momentum current is replaced by a combination of ordinary energy-momentum and proper conformal currents. Whereas the ordinary energy-momentumtensor remains to be a dynamic source of the spacetime curvature, the proper conformal current appears as a kinematic source of I >. The de Sitter special relativity, therefore, allows for a new interpretation of dark energy as an entity encoded in the kinematic group of spacetime. Furthermore, since ordinary energy is allowed to transform into dark energy and vice versa, it provides a natural scenario for an evolving cosmological term. A qualitative discussion on how a I >-evolving universe would behave is presented.en
dc.description.sponsorshipFundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)-
dc.description.sponsorshipCoordenação de Aperfeiçoamento de Pessoal de Nível Superior (CAPES)-
dc.description.sponsorshipConselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq)-
dc.format.extent181-187-
dc.language.isoeng-
dc.publisherSpringer-
dc.sourceWeb of Science-
dc.titleDe sitter relativity: a natural scenario for an evolving Lambdaen
dc.typeoutro-
dc.contributor.institutionUniv Antonio Narino-
dc.contributor.institutionUniversidade Estadual Paulista (UNESP)-
dc.description.affiliationUniv Antonio Narino, Dept Fis, Fac Ciencias Basicas, Bogota, Colombia-
dc.description.affiliationUNESP Univ Estadual Paulista, Inst Fis Teor, BR-01156970 São Paulo, Brazil-
dc.description.affiliationUnespUNESP Univ Estadual Paulista, Inst Fis Teor, BR-01156970 São Paulo, Brazil-
dc.identifier.doi10.1134/S0202289312030012-
dc.identifier.wosWOS:000307973900004-
dc.rights.accessRightsAcesso restrito-
dc.relation.ispartofGravitation & Cosmology-
Appears in Collections:Artigos, TCCs, Teses e Dissertações da Unesp

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