Cosmic microwave background anisotropies seeded by coherent topological defects : a semi-analytic approach

dc.creatorUzan, Jean-Philippe
dc.creatorDeruelle, Nathalie
dc.creatorRiazuelo, Alain
dc.date1998-10-20
dc.date1999-10-25
dc.date.accessioned2026-07-07T02:28:30Z
dc.date.available2026-07-07T02:28:30Z
dc.descriptionWe consider a perfectly homogeneous, isotropic and spatially flat universe which undergoes a sudden phase transition producing topological defects. We assume that these defects form a coherent network which scales like the background density during the radiation and matter dominated eras, and describe them in terms of a few free functions. We carefully model the loss of scaling invariance during the transition from radiation to matter dominated era. We choose a simple set for the free functions, compute the microwave background temperature anisotropies generated by such a network, and compare our results to previous calculations.
dc.description30 pages, submitted to Phys. Rev. D. On CDROM of the Proceedings of the XIXth Texas Symposium (04/26)
dc.identifierhttps://arxiv.org/abs/astro-ph/9810313
dc.identifierhttp://arxiv.org/abs/astro-ph/9810313
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/13147
dc.subjectAstrophysics
dc.titleCosmic microwave background anisotropies seeded by coherent topological defects : a semi-analytic approach
dc.typetext

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