Testing Gaussianity, Homogeneity, and Isotropy with the Cosmic Microwave Background

We review the basic hypotheses which motivate the statistical framework used to analyze the cosmic microwave background, and how that framework can be enlarged as we relax those hypotheses. In particular, we try to separate as much as possible the questions of gaussianity, homogeneity, and isotropy...

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Main Authors: L. Raul Abramo, Thiago S. Pereira
Format: Article
Language:English
Published: Wiley 2010-01-01
Series:Advances in Astronomy
Online Access:http://dx.doi.org/10.1155/2010/378203
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author L. Raul Abramo
Thiago S. Pereira
author_facet L. Raul Abramo
Thiago S. Pereira
author_sort L. Raul Abramo
collection DOAJ
description We review the basic hypotheses which motivate the statistical framework used to analyze the cosmic microwave background, and how that framework can be enlarged as we relax those hypotheses. In particular, we try to separate as much as possible the questions of gaussianity, homogeneity, and isotropy from each other. We focus both on isotropic estimators of nongaussianity as well as statistically anisotropic estimators of gaussianity, giving particular emphasis on their signatures and the enhanced “cosmic variances” that become increasingly important as our putative Universe becomes less symmetric. After reviewing the formalism behind some simple model-independent tests, we discuss how these tests can be applied to CMB data when searching for large-scale “anomalies”.
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spelling doaj-art-53c785fa698c4d729d854c1bb79c7c872025-02-03T07:24:39ZengWileyAdvances in Astronomy1687-79691687-79772010-01-01201010.1155/2010/378203378203Testing Gaussianity, Homogeneity, and Isotropy with the Cosmic Microwave BackgroundL. Raul Abramo0Thiago S. Pereira1Instituto de Física, Universidade de São Paulo, CP 66318, CEP 05315-970 São Paulo, BrazilInstituto de Física Teórica, Universidade Estadual Paulista, CP 70532-2, CEP 01156-970 São Paulo, BrazilWe review the basic hypotheses which motivate the statistical framework used to analyze the cosmic microwave background, and how that framework can be enlarged as we relax those hypotheses. In particular, we try to separate as much as possible the questions of gaussianity, homogeneity, and isotropy from each other. We focus both on isotropic estimators of nongaussianity as well as statistically anisotropic estimators of gaussianity, giving particular emphasis on their signatures and the enhanced “cosmic variances” that become increasingly important as our putative Universe becomes less symmetric. After reviewing the formalism behind some simple model-independent tests, we discuss how these tests can be applied to CMB data when searching for large-scale “anomalies”.http://dx.doi.org/10.1155/2010/378203
spellingShingle L. Raul Abramo
Thiago S. Pereira
Testing Gaussianity, Homogeneity, and Isotropy with the Cosmic Microwave Background
Advances in Astronomy
title Testing Gaussianity, Homogeneity, and Isotropy with the Cosmic Microwave Background
title_full Testing Gaussianity, Homogeneity, and Isotropy with the Cosmic Microwave Background
title_fullStr Testing Gaussianity, Homogeneity, and Isotropy with the Cosmic Microwave Background
title_full_unstemmed Testing Gaussianity, Homogeneity, and Isotropy with the Cosmic Microwave Background
title_short Testing Gaussianity, Homogeneity, and Isotropy with the Cosmic Microwave Background
title_sort testing gaussianity homogeneity and isotropy with the cosmic microwave background
url http://dx.doi.org/10.1155/2010/378203
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AT thiagospereira testinggaussianityhomogeneityandisotropywiththecosmicmicrowavebackground