Cosmic Microwave Background Anisotropies from Scaling Seeds: Generic Properties of the Correlation Functions

dc.creatorDurrer, Ruth
dc.creatorKunz, Martin
dc.date1997-11-12
dc.date.accessioned2026-07-07T11:34:07Z
dc.date.available2026-07-07T11:34:07Z
dc.descriptionIn this work we present a partially new method to analyze fluctuations which are induced by causal scaling seeds. We show that the power spectra due to this kind of seed perturbations are determined by five analytic functions, which we determine numerically for a special example. We put forward the view that, even if recent work disfavors the models with cosmic strings and global O(4) texture, causal scaling seed perturbations merit a more thorough and general analysis, which we initiate in this paper.
dc.descriptionLaTeX file with RevTex, 6 pages, 6 PS figs., submitted to Phys. Rev. D. A version with higher quality images can be found at http://mykonos.unige.ch/~kunz/
dc.identifierhttps://arxiv.org/abs/astro-ph/9711133
dc.identifierhttp://arxiv.org/abs/astro-ph/9711133
dc.identifierPhys.Rev.D57:R3199-R3203,1998
dc.identifierdoi:10.1103/PhysRevD.57.3199
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/198133
dc.subjectAstrophysics
dc.titleCosmic Microwave Background Anisotropies from Scaling Seeds: Generic Properties of the Correlation Functions
dc.typetext

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