Scalar Perturbations
Scalar Perturbations is a type of primordial density fluctuation in the early universe that belongs to the class of cosmological perturbations characterized by spatial variations in the energy density and gravitational potential, distinguished from vector and tensor perturbations by its invariance under spatial rotations and its role in seeding large-scale structure formation through gravitational instability.
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Dark Matter as a Topological Vacuum Condensate
arXiv (Cornell University) · 2018 · 3.7K citations · Full text
Natural Sciences, Astronomy, Physics +16
Theory of cosmological perturbations
Viatcheslav Mukhanov · Physics Reports · 1992 · 3.6K citations · Full text
Natural Sciences, Astronomy, Physics +12
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Centre National de la Recherche Scientifique
Paris, France
41 h-index
135 publications
8.7K citations
The University of Tokyo
Tokyo, Japan
39 h-index
121 publications
9.8K citations

Kyoto University
Kyoto, Japan
39 h-index
111 publications
9.2K citations
University of Cambridge
Cambridge, United Kingdom
34 h-index
74 publications
5K citations

European Organization for Nuclear Research
Geneva, Switzerland
31 h-index
53 publications
4.3K citations

Kavli Institute for the Physics and Mathematics of the Universe
Kashiwa, Japan
31 h-index
72 publications
6.5K citations

Chinese Academy of Sciences
Beijing, China
28 h-index
92 publications
6.2K citations
Institute of Theoretical Physics
Beijing, China
28 h-index
88 publications
6K citations
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249 publications · 16.4K citations
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JCAP · 292 publications · 17.4K citations
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140 publications · 18.4K citations
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PRD · 195 publications · 7.6K citations
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87 publications · 6.1K citations
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