dc.creatorChimento, Luis Pascual
dc.creatorForte, Mónica
dc.creatorRicharte, Martín Gustavo
dc.date.accessioned2018-09-11T17:24:54Z
dc.date.accessioned2018-11-06T12:56:50Z
dc.date.available2018-09-11T17:24:54Z
dc.date.available2018-11-06T12:56:50Z
dc.date.created2018-09-11T17:24:54Z
dc.date.issued2010-06
dc.identifierChimento, Luis Pascual; Forte, Mónica; Richarte, Martín Gustavo; Crossing the phantom divide with k-essence in braneworlds; World Scientific; Modern Physics Letters A: Particles and Fields; Gravitation; Cosmology and Nuclear Physics; 25; 29; 6-2010; 2469-2481
dc.identifier0217-7323
dc.identifierhttp://hdl.handle.net/11336/59104
dc.identifierCONICET Digital
dc.identifierCONICET
dc.identifier.urihttp://repositorioslatinoamericanos.uchile.cl/handle/2250/1871491
dc.description.abstractWe study a flat three-brane in the presence of a linear k field with nonzero cosmological constant Λ4. In this model the crossing of the phantom divide (PD) occurs when the k-essence energy density becomes negative. We show that in the high energy regime the effective equation of state has a resemblance of a modified Chaplygin gas while in the low energy regime it becomes linear. We find a scale factor that begins from a singularity and evolves to a de Sitter stable stage while other solutions have a super-accelerated regime and end with a big rip. We use the energy conditions to show when the effective equation of state of the brane-universe crosses the PD. © 2010 World Scientific Publishing Company.
dc.languageeng
dc.publisherWorld Scientific
dc.relationinfo:eu-repo/semantics/altIdentifier/doi/http://dx.doi.org/10.1142/S0217732310033797
dc.rightshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/
dc.rightsinfo:eu-repo/semantics/restrictedAccess
dc.subjectBRANEWORLDS
dc.subjectK-ESSENCE
dc.subjectPHANTOM DIVIDE
dc.titleCrossing the phantom divide with k-essence in braneworlds
dc.typeArtículos de revistas
dc.typeArtículos de revistas
dc.typeArtículos de revistas


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