Dynamical mutation of dark energy

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dc.contributor.authorAbramo, L. R.
dc.contributor.authorBatista, R. C.
dc.contributor.authorLiberato, L. [UNESP]
dc.contributor.authorRosenfeld, R. [UNESP]
dc.contributor.institutionUniversidade de São Paulo (USP)
dc.contributor.institutionUniversidade Estadual Paulista (UNESP)
dc.date.accessioned2022-04-28T20:39:00Z
dc.date.available2022-04-28T20:39:00Z
dc.date.issued2008-03-10
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. © 2008 The American Physical Society.en
dc.description.affiliationInstituto de Física Universidade de São Paulo, CP 66318, 05315-970, São Paulo
dc.description.affiliationInstituto de Física Teórica Universidade Estadual Paulista, R. Pamplona 145, 01405-900, São Paulo
dc.description.affiliationUnespInstituto de Física Teórica Universidade Estadual Paulista, R. Pamplona 145, 01405-900, São Paulo
dc.identifierhttp://dx.doi.org/10.1103/PhysRevD.77.067301
dc.identifier.citationPhysical Review D - Particles, Fields, Gravitation and Cosmology, v. 77, n. 6, 2008.
dc.identifier.doi10.1103/PhysRevD.77.067301
dc.identifier.issn1550-7998
dc.identifier.issn1550-2368
dc.identifier.scopus2-s2.0-41449084266
dc.identifier.urihttp://hdl.handle.net/11449/225087
dc.language.isoeng
dc.relation.ispartofPhysical Review D - Particles, Fields, Gravitation and Cosmology
dc.sourceScopus
dc.titleDynamical mutation of dark energyen
dc.typeArtigo

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