Defect models of cosmic structure in light of the new CMB data

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dc.creatorAlbrecht, Andreas
dc.date2000-09-08
dc.date.accessioned2026-07-07T01:55:23Z
dc.date.available2026-07-07T01:55:23Z
dc.descriptionDefect models of cosmic structure formation have faced a number of difficult challenges over recent years. Yet interestingly, new CMB data does not show strong evidence for secondary oscillations in the anisotropy power. Here I review the current standing of the cosmic defect models of structure formation in light of the current data.
dc.description12 Pages including 4 figures. To appear in the proceedings of the XXXVth Rencontres de Moriond ``Energy Densities in the Universe''
dc.identifierhttps://arxiv.org/abs/astro-ph/0009129
dc.identifierhttp://arxiv.org/abs/astro-ph/0009129
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/1637
dc.subjectAstrophysics
dc.subjectHigh Energy Physics - Phenomenology
dc.titleDefect models of cosmic structure in light of the new CMB data
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