Dark Energy: Is it Q or Lambda ?

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dc.creatorMelchiorri, Alessandro
dc.creatorOdman, Carolina
dc.date2002-12-30
dc.date.accessioned2026-07-07T02:07:02Z
dc.date.available2026-07-07T02:07:02Z
dc.descriptionNew observations of Cosmic Microwave Background Anisotropies, Supernovae luminosity distances and Galaxy Clustering are sharpening our knowledge about dark energy. Here we present the latest constraints.
dc.description4 pages, 2 figures, to appear in proceedings of the XVIIIth IAP Colloquium `On the Nature of Dark Energy', IAP, Paris
dc.identifierhttps://arxiv.org/abs/astro-ph/0212566
dc.identifierhttp://arxiv.org/abs/astro-ph/0212566
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/5564
dc.subjectAstrophysics
dc.titleDark Energy: Is it Q or Lambda ?
dc.typetext

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