Forecasting cosmic doomsday from CMB-LSS cross-correlations.

dc.contributor.authorGarriga Torres, Jaumecat
dc.contributor.authorPogosian, Levoncat
dc.contributor.authorVachaspati, T. (Tanmay)cat
dc.date.accessioned2010-05-06T09:32:57Z
dc.date.available2010-05-06T09:32:57Z
dc.date.issued2004cat
dc.description.abstractA broad class of dark energy models, which have been proposed in attempts at solving the cosmological constant problems, predict a late time variation of the equation of state with redshift. The variation occurs as a scalar field picks up speed on its way to negative values of the potential. The negative potential energy eventually turns the expansion into contraction and the local universe undergoes a big crunch. In this paper we show that cross-correlations of the cosmic microwave background anisotropy and matter distribution, in combination with other cosmological data, can be used to forecast the imminence of such cosmic doomsday.eng
dc.format.extent11 p.cat
dc.format.mimetypeapplication/pdfeng
dc.identifier.idgrec520521cat
dc.identifier.issn0556-2821cat
dc.identifier.urihttps://hdl.handle.net/2445/12379
dc.language.isoengeng
dc.publisherThe American Physical Societyeng
dc.relation.isformatofReproducció digital del document publicat en format paper, proporcionada per PROLA i http://dx.doi.org/10.1103/PhysRevD.69.063511cat
dc.relation.ispartofPhysical Review D, 2004, vol. 69, núm. 6, p. 063511-1-063511-11cat
dc.relation.urihttp://dx.doi.org/10.1103/PhysRevD.69.063511
dc.rights(c) The American Physical Society, 2004eng
dc.rights.accessRightsinfo:eu-repo/semantics/openAccess
dc.sourceArticles publicats en revistes (Física de la Matèria Condensada)
dc.subject.classificationCosmologiacat
dc.subject.otherCosmologyeng
dc.titleForecasting cosmic doomsday from CMB-LSS cross-correlations.eng
dc.typeinfo:eu-repo/semantics/articleeng
dc.typeinfo:eu-repo/semantics/publishedVersion

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