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...
Main Authors: | N. Bartolo, S. Matarrese, A. Riotto |
---|---|
Format: | Article |
Language: | English |
Published: |
Hindawi Limited
2010-01-01
|
Series: | Advances in Astronomy |
Online Access: | http://dx.doi.org/10.1155/2010/157079 |
Similar Items
-
Non-Gaussianity and Statistical Anisotropy from Vector Field Populated Inflationary Models
by: Emanuela Dimastrogiovanni, et al.
Published: (2010-01-01) -
Non-Gaussianity in the cosmic microwave background
by: Smith, Sarah Jane
Published: (2006) -
Primordial Non-Gaussianity in the Cosmic Microwave Background
by: Amit P. S. Yadav, et al.
Published: (2010-01-01) -
Cosmic Strings and Their Induced Non-Gaussianities in the Cosmic Microwave Background
by: Christophe Ringeval
Published: (2010-01-01) -
Non-Gaussianity and extragalactic foregrounds to the Cosmic Microwave Background
by: Lacasa, Fabien
Published: (2013)