Non-Gaussianity and the Cosmic Microwave Background Anisotropies

We review in a pedagogical way the present status of the impact of non-Gaussianity (NG) on the cosmic microwave background (CMB) anisotropies. We first show how to set the initial conditions at second order for the CMB anisotropies when some primordial NG is present. However, there are many sources...

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Main Authors: N. Bartolo, S. Matarrese, A. Riotto
Format: Article
Language:English
Published: Wiley 2010-01-01
Series:Advances in Astronomy
Online Access:http://dx.doi.org/10.1155/2010/157079
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author N. Bartolo
S. Matarrese
A. Riotto
author_facet N. Bartolo
S. Matarrese
A. Riotto
author_sort N. Bartolo
collection DOAJ
description We review in a pedagogical way the present status of the impact of non-Gaussianity (NG) on the cosmic microwave background (CMB) anisotropies. We first show how to set the initial conditions at second order for the CMB anisotropies when some primordial NG is present. However, there are many sources of NG in CMB anisotropies, beyond the primordial one, which can contaminate the primordial signal. We mainly focus on the NG generated from the post inflationary evolution of the CMB anisotropies at second order in perturbation theory at large and small angular scales, such as the ones generated at the recombination epoch. We show how to derive the equations to study the second-order CMB anisotropies and provide analytical computations to evaluate their contamination to primordial NG (complemented with numerical examples). We also offer a brief summary of other secondary effects. This paper requires basic knowledge of the theory of cosmological perturbations at the linear level.
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spelling doaj-art-9e961b36b7784e4abe3f30a883e18fad2025-02-03T05:59:08ZengWileyAdvances in Astronomy1687-79691687-79772010-01-01201010.1155/2010/157079157079Non-Gaussianity and the Cosmic Microwave Background AnisotropiesN. Bartolo0S. Matarrese1A. Riotto2Dipartimento di Fisica “G. Galilei”, Università di Padova, via Marzolo 8, 131 Padova, ItalyDipartimento di Fisica “G. Galilei”, Università di Padova, via Marzolo 8, 131 Padova, ItalyINFN, Sezione di Padova, via Marzolo 8, 35131 Padova, ItalyWe review in a pedagogical way the present status of the impact of non-Gaussianity (NG) on the cosmic microwave background (CMB) anisotropies. We first show how to set the initial conditions at second order for the CMB anisotropies when some primordial NG is present. However, there are many sources of NG in CMB anisotropies, beyond the primordial one, which can contaminate the primordial signal. We mainly focus on the NG generated from the post inflationary evolution of the CMB anisotropies at second order in perturbation theory at large and small angular scales, such as the ones generated at the recombination epoch. We show how to derive the equations to study the second-order CMB anisotropies and provide analytical computations to evaluate their contamination to primordial NG (complemented with numerical examples). We also offer a brief summary of other secondary effects. This paper requires basic knowledge of the theory of cosmological perturbations at the linear level.http://dx.doi.org/10.1155/2010/157079
spellingShingle N. Bartolo
S. Matarrese
A. Riotto
Non-Gaussianity and the Cosmic Microwave Background Anisotropies
Advances in Astronomy
title Non-Gaussianity and the Cosmic Microwave Background Anisotropies
title_full Non-Gaussianity and the Cosmic Microwave Background Anisotropies
title_fullStr Non-Gaussianity and the Cosmic Microwave Background Anisotropies
title_full_unstemmed Non-Gaussianity and the Cosmic Microwave Background Anisotropies
title_short Non-Gaussianity and the Cosmic Microwave Background Anisotropies
title_sort non gaussianity and the cosmic microwave background anisotropies
url http://dx.doi.org/10.1155/2010/157079
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