Impact of three years of data from the Wilkinson Microwave Anisotropy Probe on cosmological models with dynamical dark energy

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dc.creatorDoran, Michael
dc.creatorRobbers, Georg
dc.creatorWetterich, Christof
dc.date2006-09-29
dc.date2007-01-23
dc.date.accessioned2026-07-07T10:23:42Z
dc.date.available2026-07-07T10:23:42Z
dc.descriptionThe first three years of observation of the Wilkinson Microwave Anisotropy Probe (WMAP) have provided the most precise data on the anisotropies of the cosmic microwave background (CMB) to date. We investigate the impact of these results and their combination with data from other astrophysical probes on cosmological models with a dynamical dark energy component. By considering a wide range of such models, we find that the constraints on dynamical dark energy are significantly improved compared to the first year data.
dc.description5 pages, 2 figures; v2: more explanatory title, added references, minor clarifications, matches published version
dc.identifierhttps://arxiv.org/abs/astro-ph/0609814
dc.identifierhttp://arxiv.org/abs/astro-ph/0609814
dc.identifierPhys.Rev.D75:023003,2007
dc.identifierdoi:10.1103/PhysRevD.75.023003
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/175927
dc.subjectAstrophysics
dc.titleImpact of three years of data from the Wilkinson Microwave Anisotropy Probe on cosmological models with dynamical dark energy
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