Logotipo do repositório

De sitter relativity: a natural scenario for an evolving Lambda

dc.contributor.authorBeltran Almeida, J. P.
dc.contributor.authorMayor, C. S. O. [UNESP]
dc.contributor.authorPereira, J. G. [UNESP]
dc.contributor.institutionUniv Antonio Narino
dc.contributor.institutionUniversidade Estadual Paulista (Unesp)
dc.date.accessioned2013-09-30T18:53:22Z
dc.date.accessioned2014-05-20T14:09:22Z
dc.date.available2013-09-30T18:53:22Z
dc.date.available2014-05-20T14:09:22Z
dc.date.issued2012-07-01
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.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.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.identifierhttp://dx.doi.org/10.1134/S0202289312030012
dc.identifier.citationGravitation & Cosmology. New York: Springer, v. 18, n. 3, p. 181-187, 2012.
dc.identifier.dimensionspub.1045969401
dc.identifier.doi10.1134/S0202289312030012
dc.identifier.issn0202-2893
dc.identifier.issn1995-0721
dc.identifier.lattes1599966126072450
dc.identifier.orcid0000-0002-5324-0679
dc.identifier.orcid0000-0002-5616-8414
dc.identifier.urihttp://hdl.handle.net/11449/24147
dc.identifier.wosWOS:000307973900004
dc.language.isoeng
dc.publisherSpringer
dc.publisherPleiades Publishing
dc.relation.ispartofGravitation & Cosmology
dc.relation.ispartofjcr0.870
dc.relation.ispartofsjr0,397
dc.rights.accessRightsAcesso restritopt
dc.sourceWeb of Science
dc.sourceDimensions
dc.titleDe sitter relativity: a natural scenario for an evolving Lambdaen
dc.typeArtigopt
dcterms.licensehttp://www.maik.rssi.ru/cgi-perl/contents.pl?catalog=4&page=1&lang=eng
dcterms.rightsHolderSpringer
dspace.entity.typePublication
relation.isOrgUnitOfPublication41d94a5b-139b-457c-90a7-77b71f4e94df
relation.isOrgUnitOfPublication.latestForDiscovery41d94a5b-139b-457c-90a7-77b71f4e94df
unesp.author.lattes1599966126072450
unesp.author.orcid0000-0002-5616-8414[3]
unesp.author.orcid0000-0002-5324-0679[1]
unesp.campusUniversidade Estadual Paulista (UNESP), Instituto de Física Teórica (IFT), São Paulopt

Arquivos