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Please use this identifier to cite or link to this item: http://acervodigital.unesp.br/handle/11449/24477
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dc.contributor.authorAbramo, L. R.-
dc.contributor.authorBatista, R. C.-
dc.contributor.authorLiberato, L.-
dc.contributor.authorRosenfeld, Rogério-
dc.date.accessioned2013-09-30T18:58:03Z-
dc.date.accessioned2014-05-20T14:11:41Z-
dc.date.available2013-09-30T18:58:03Z-
dc.date.available2014-05-20T14:11:41Z-
dc.date.issued2008-03-01-
dc.identifierhttp://dx.doi.org/10.1103/PhysRevD.77.067301-
dc.identifier.citationPhysical Review D. College Pk: Amer Physical Soc, v. 77, n. 6, p. 4, 2008.-
dc.identifier.issn1550-7998-
dc.identifier.urihttp://hdl.handle.net/11449/24477-
dc.description.abstractWe discuss the intriguing possibility that dark energy may change its equation of state in situations where large dark energy fluctuations are present. We show indications of this dynamical mutation in some generic models of dark energy.en
dc.format.extent4-
dc.language.isoeng-
dc.publisherAmer Physical Soc-
dc.sourceWeb of Science-
dc.titleDynamical mutation of dark energyen
dc.typeoutro-
dc.contributor.institutionUniversidade de São Paulo (USP)-
dc.contributor.institutionUniversidade Estadual Paulista (UNESP)-
dc.description.affiliationUniv São Paulo, Inst Fis, BR-05315970 São Paulo, Brazil-
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.identifier.doi10.1103/PhysRevD.77.067301-
dc.identifier.wosWOS:000254544500133-
dc.rights.accessRightsAcesso restrito-
dc.identifier.fileWOS000254544500133.pdf-
dc.relation.ispartofPhysical Review D-
Appears in Collections:Artigos, TCCs, Teses e Dissertações da Unesp

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