Cosmic Microwave Background Anisotropies: Inflation versus Topological Defects

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dc.creatorSakellariadou, Mairi
dc.date1999-11-29
dc.date.accessioned2026-07-07T02:34:41Z
dc.date.available2026-07-07T02:34:41Z
dc.descriptionI present a briefly summary of the current status of inflationary models versus topological defects scenarios, as the mechanisms which could have induced the initial density perturbations, which left an imprint on the cosmic microwave backgound radiation anisotropies.
dc.descriptionLaTeX file (9 pages) To be published in the Proceedings of the Spanish Relativity Meeting, Bilbao 1999
dc.identifierhttps://arxiv.org/abs/astro-ph/9911497
dc.identifierhttp://arxiv.org/abs/astro-ph/9911497
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/15343
dc.subjectAstrophysics
dc.titleCosmic Microwave Background Anisotropies: Inflation versus Topological Defects
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