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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 |