Cosmological Strucure Formation with Topological Defects

Simple item page
dc.creatorDurrer, Ruth
dc.date2000-03-23
dc.date.accessioned2026-07-07T01:52:51Z
dc.date.available2026-07-07T01:52:51Z
dc.descriptionStructure formation with topological defects is described. The main differences from inflationary models are highlighted. The results are compared with recent observations. It is concluded that all the defect models studied so far are in disagreement with recent observations of CMB anisotropies. Furthermore, present observations do not support 'decoherence', a generic feature of structure formation from topological defects.
dc.description9 pages, 5 figures, moriond.sty
dc.identifierhttps://arxiv.org/abs/astro-ph/0003363
dc.identifierhttp://arxiv.org/abs/astro-ph/0003363
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/766
dc.subjectAstrophysics
dc.subjectHigh Energy Physics - Phenomenology
dc.titleCosmological Strucure Formation with Topological Defects
dc.typetext

Files

Collections

arXiv