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Dark coupling

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Dark coupling

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dc.contributor.author Gavela, María Belén
dc.contributor.author Hernández Díaz, Daniel
dc.contributor.author López Honórez, Laura
dc.contributor.author Mena Requejo, Olga
dc.contributor.author Rigolin, Stefano
dc.date.accessioned 2014-09-11T08:33:06Z
dc.date.available 2014-09-11T08:33:06Z
dc.date.issued 2009
dc.identifier.citation Gavela, M. B. Hernández, D. López Honórez, Laura Mena Requejo, Olga Rigolin, S. 2009 Dark coupling Journal Of Cosmology And Astroparticle Physics 2009 7 034
dc.identifier.uri http://hdl.handle.net/10550/37736
dc.description.abstract The two dark sectors of the universe-dark matter and dark energy - may interact with each other. Background and linear density perturbation evolution equations are developed for a generic coupling. We then establish the general conditions necessary to obtain models free from non-adiabatic instabilities. As an application, we consider a viable universe in which the interaction strength is proportional to the dark energy density. The scenario does not exhibit 'phantom crossing' and is free from instabilities, including early ones. A sizeable interaction strength is compatible with combined WMAP, HST, SN, LSS and H(z) data. Neutrino mass and/or cosmic curvature are allowed to be larger than in non-interacting models. Our analysis sheds light as well on unstable scenarios previously proposed.
dc.language.iso eng
dc.relation.ispartof Journal Of Cosmology And Astroparticle Physics, 2009, vol. 2009, num. 7, p. 034
dc.subject Astrofísica
dc.title Dark coupling
dc.type journal article es_ES
dc.date.updated 2014-09-11T08:33:06Z
dc.identifier.doi 10.1088/1475-7516/2009/07/034
dc.identifier.idgrec 097546
dc.rights.accessRights open access es_ES

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