Dark energy effects in the Cosmic Microwave Background Radiation

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dc.creatorCorasaniti, P. S.
dc.date2002-10-11
dc.date.accessioned2026-07-07T02:05:40Z
dc.date.available2026-07-07T02:05:40Z
dc.descriptionUnderstanding the nature of the dark energy is one of the most important task in cosmology. In principle several cosmological observations can be used to discriminate amid a static cosmological constant contribution and a dynamical quintessence component. In view of the upcoming high resolution CMB experiments, using a model independent approach we study the dark energy imprint in the CMB anisotropy power spectrum and the degeneracy with other cosmological parameters.
dc.description4 pages, 3 figures, to appear in the Proceedings of the XVIII IAP Colloquium `On the nature of dark energy', Paris, 1-5 July 2002
dc.identifierhttps://arxiv.org/abs/astro-ph/0210257
dc.identifierhttp://arxiv.org/abs/astro-ph/0210257
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/5169
dc.subjectAstrophysics
dc.titleDark energy effects in the Cosmic Microwave Background Radiation
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