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Primordial Non-Gaussianity in the Large-Scale Structure of the Universe
Joint Authors
Desjacques, Vincent
Seljak, Uroš
Source
Issue
Vol. 2010, Issue 2010 (31 Dec. 2010), pp.1-23, 23 p.
Publisher
Hindawi Publishing Corporation
Publication Date
2010-08-04
Country of Publication
Egypt
No. of Pages
23
Main Subjects
Abstract EN
Primordial non-Gaussianity is a potentially powerful discriminant of the physical mechanisms that generated the cosmological fluctuations observed today.
Any detection of significant non-Gaussianity would thus have profound implications for our understanding of cosmic structure formation.
The large-scale mass distribution in the Universe is a sensitive probe of the nature of initial conditions.
Recent theoretical progress together with rapid developments in observational techniques will enable us to critically confront predictions of inflationary scenarios and set constraints as competitive as those from the Cosmic Microwave Background.
In this paper, we review past and current efforts in the search for primordial non-Gaussianity in the large-scale structure of the Universe.
American Psychological Association (APA)
Desjacques, Vincent& Seljak, Uroš. 2010. Primordial Non-Gaussianity in the Large-Scale Structure of the Universe. Advances in Astronomy،Vol. 2010, no. 2010, pp.1-23.
https://search.emarefa.net/detail/BIM-507252
Modern Language Association (MLA)
Desjacques, Vincent& Seljak, Uroš. Primordial Non-Gaussianity in the Large-Scale Structure of the Universe. Advances in Astronomy No. 2010 (2010), pp.1-23.
https://search.emarefa.net/detail/BIM-507252
American Medical Association (AMA)
Desjacques, Vincent& Seljak, Uroš. Primordial Non-Gaussianity in the Large-Scale Structure of the Universe. Advances in Astronomy. 2010. Vol. 2010, no. 2010, pp.1-23.
https://search.emarefa.net/detail/BIM-507252
Data Type
Journal Articles
Language
English
Notes
Includes bibliographical references
Record ID
BIM-507252