Cmb Bispectrum
The CMB Bispectrum is the three-point correlation function of temperature anisotropies in the cosmic microwave background, serving as a statistical measure of non-Gaussianity that distinguishes primordial density fluctuations from those generated by linear evolution in the early universe.
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3.5K
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736
Institutions
Publications per year
2017–2026
255
Variants
Cosmic Microwave Background Bispectrum
Parents
1.1K
A line of sight integration approach to cosmic microwave background anisotropies
1996 · 1.3K citations
Natural Sciences, Astronomy, Physics +16
THE TEMPERATURE OF THE COSMIC MICROWAVE BACKGROUND
The Astrophysical Journal · 2009 · 1.1K citations · Full text
Natural Sciences, Astronomy, Physics +11
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Centre National de la Recherche Scientifique
Paris, France
49 h-index
564 publications
132.5K citations
Princeton University
Princeton, United States
45 h-index
172 publications
32.4K citations
University of California, Berkeley
Berkeley, United States
44 h-index
253 publications
25.4K citations
University of Cambridge
Cambridge, United Kingdom
43 h-index
194 publications
30.9K citations
California Institute of Technology
Pasadena, United States
41 h-index
223 publications
39.4K citations

Lawrence Berkeley National Laboratory
Berkeley, United States
38 h-index
123 publications
14.7K citations
University of Chicago
Chicago, United States
37 h-index
394 publications
43.4K citations
Institut d'Astrophysique de Paris
Paris, France
37 h-index
172 publications
28.3K citations
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ApJ · 138 publications · 13.3K citations
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144 publications · 9.1K citations
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JCAP · 177 publications · 8.9K citations
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171 publications · 7.9K citations
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PRD · 65 publications · 3.1K citations
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