Linear Perturbation Theory
Linear Perturbation Theory is a theoretical framework within cosmological perturbation theory that describes the evolution of small-amplitude fluctuations in the early universe by linearizing the Einstein and fluid equations around a homogeneous and isotropic background spacetime.
757
Publications
58.6K
Citations
1.5K
Authors
684
Institutions
Publications per year
2017–2026
137
757
Large-scale structure of the Universe and cosmological perturbation theory
Francis Bernardeau, S. Colombi, E. Gaztañaga et al. · Physics Reports · 2002 · 1.9K citations · Full text
Natural Sciences, Astronomy, Physics +14
Cosmological Perturbation Theory
Hideo Kodama, Misao Sasaki · Progress of Theoretical Physics Supplement · 1984 · 1.7K citations
Natural Sciences, Physics, Cosmology +16
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684

Kyoto University
Kyoto, Japan
22 h-index
57 publications
4.8K citations

Centre National de la Recherche Scientifique
Paris, France
21 h-index
60 publications
5.8K citations
The University of Tokyo
Tokyo, Japan
21 h-index
57 publications
5K citations
University of Cambridge
Cambridge, United Kingdom
19 h-index
30 publications
3.3K citations
Princeton University
Princeton, United States
16 h-index
31 publications
10.9K citations
University of Portsmouth
Portsmouth, United Kingdom
14 h-index
30 publications
2.2K citations

Kavli Institute for the Physics and Mathematics of the Universe
Kashiwa, Japan
14 h-index
24 publications
1.2K citations
The University of Texas at Austin
Austin, United States
13 h-index
25 publications
1.2K citations
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65 publications · 6.1K citations
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72 publications · 5K citations
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ApJ · 60 publications · 11K citations
30
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JCAP · 64 publications · 4.8K citations
28
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36 publications · 6.3K citations
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