Non-gaussianity Analysis
Non-Gaussianity Analysis is a statistical methodology in cosmology that characterizes deviations from Gaussianity in the temperature fluctuations of the Cosmic Microwave Background, distinguishing itself by quantifying primordial non-Gaussian signatures to constrain inflationary models and underlying physics of the early universe.
1.2K
Publications
73.9K
Citations
1.9K
Authors
720
Institutions
Publications per year
2017–2026
270
1.2K
1–5 of 1.2K
1.9K
33
h-index
Istituto Nazionale di Fisica Nucleare, Sezione di Padova, Italy
23 publications · 1.8K citations
21
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21
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Kavli Institute for Particle Astrophysics and Cosmology, United States
18 publications · 1.9K citations
17
h-index
17
h-index
1–5 of 1.9K
720
University of Cambridge
Cambridge, United Kingdom
41 h-index
149 publications
9.3K citations
Istituto Nazionale di Fisica Nucleare, Sezione di Padova
Padua, Italy
37 h-index
108 publications
7K citations
University of Portsmouth
Portsmouth, United Kingdom
36 h-index
113 publications
8.7K citations

University of Padua
Padua, Italy
35 h-index
97 publications
5.5K citations
The University of Tokyo
Tokyo, Japan
35 h-index
115 publications
6.4K citations

Centre National de la Recherche Scientifique
Paris, France
34 h-index
157 publications
7.8K citations
Princeton University
Princeton, United States
33 h-index
63 publications
9.3K citations

Kavli Institute for the Physics and Mathematics of the Universe
Kashiwa, Japan
30 h-index
62 publications
2.6K citations
1–8 of 720
JCAP · 275 publications · 18.2K citations
75
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158 publications · 12.2K citations
57
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147 publications · 6.4K citations
45
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ApJ · 69 publications · 5.6K citations
39
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PRD · 61 publications · 2.6K citations
30
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