Textures and Cosmic Microwave Background non-Gaussian Signatures

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dc.creatorGangui, Alejandro
dc.date1997-11-27
dc.date.accessioned2026-07-07T02:25:25Z
dc.date.available2026-07-07T02:25:25Z
dc.descriptionWe report briefly on a recent analysis of the texture-induced CMB radiation three-point correlation function of temperature anisotropies as predicted by an analytical model. We specialize our analysis to both large-scales (e.g., for COBE-DMR, where we compare our prediction with the actual four-year data) and intermediate-scales. We show how the latter case puts strong constraints on the model parameters.
dc.descriptionTwo references updated, otherwise matches exactly the published version
dc.identifierhttps://arxiv.org/abs/astro-ph/9711343
dc.identifierhttp://arxiv.org/abs/astro-ph/9711343
dc.identifierHelv.Phys.Acta 69 (1996) 215-218
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/11869
dc.subjectAstrophysics
dc.titleTextures and Cosmic Microwave Background non-Gaussian Signatures
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