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Primordial non-Gaussianity in the large scale structure of the Universe


Desjacques, V; Seljak, U (2010). Primordial non-Gaussianity in the large scale structure of the Universe. Advances in Astronomy, 2010:908640.

Abstract

Primordial non-Gaussianity is a potentially powerful discriminant of the physical mechanisms that generate the cosmological fluctuations observed today. Any detection of non-Gaussianity would have profound implications for our understanding of cosmic structure formation. In this paper, we review past and current efforts in the search for primordial non-Gaussianity in the large-scale structure of the Universe.

Abstract

Primordial non-Gaussianity is a potentially powerful discriminant of the physical mechanisms that generate the cosmological fluctuations observed today. Any detection of non-Gaussianity would have profound implications for our understanding of cosmic structure formation. In this paper, we review past and current efforts in the search for primordial non-Gaussianity in the large-scale structure of the Universe.

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Additional indexing

Other titles:Primordial non-Gaussianity from the large scale structure
Item Type:Journal Article, refereed, further contribution
Communities & Collections:07 Faculty of Science > Institute for Computational Science
Dewey Decimal Classification:530 Physics
Language:English
Date:2010
Deposited On:03 Mar 2011 07:51
Last Modified:07 Dec 2017 05:27
Publisher:Hindawi
ISSN:1687-7969
Publisher DOI:https://doi.org/10.1155/2010/908640
Related URLs:http://arxiv.org/abs/1006.4763

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