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Dark coupling and gauge invariance

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Dark coupling and gauge invariance

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dc.contributor.author Gavela, María Belén
dc.contributor.author López Honórez, Laura
dc.contributor.author Mena Requejo, Olga
dc.contributor.author Rigolin, Stefano
dc.date.accessioned 2014-09-11T08:05:50Z
dc.date.available 2014-09-11T08:05:50Z
dc.date.issued 2010
dc.identifier.citation Gavela, M. B. López Honórez, L. Mena Requejo, Olga Rigolin, S. 2010 Dark coupling and gauge invariance Journal Of Cosmology And Astroparticle Physics 10 11 044
dc.identifier.uri http://hdl.handle.net/10550/37723
dc.description.abstract We study a coupled dark energy-dark matter model in which the energy-momentum exchange is proportional to the Hubble expansion rate. The inclusion of its perturbation is required by gauge invariance. We derive the linear perturbation equations for the gauge invariant energy density contrast and velocity of the coupled fluids, and we determine the initial conditions. The latter turn out to be adiabatic for dark energy, when assuming adiabatic initial conditions for all the standard fluids. We perform a full Monte Carlo Markov Chain likelihood analysis of the model, using WMAP 7-year data.
dc.language.iso eng
dc.relation.ispartof Journal Of Cosmology And Astroparticle Physics, 2010, vol. 10, num. 11, p. 044
dc.subject Física
dc.subject Astrofísica
dc.title Dark coupling and gauge invariance
dc.type journal article es_ES
dc.date.updated 2014-09-11T08:05:50Z
dc.identifier.doi 10.1088/1475-7516/2010/11/044
dc.identifier.idgrec 097554
dc.rights.accessRights open access es_ES

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