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Cosmological Perturbation Theory

Kodama, Hideo, Sasaki, Misao·1984·Progress of Theoretical Physics Supplement

Abstract

The linear perturbation theory of spatially homogeneous and isotropic universes is reviewed and reformulated extensively. In the first half of the article, a gauge-invariant formulation of the theory is carried out with special attention paid to the geometrical meaning of the perturbation. In the second half of the article, the application of the theory to some important cosmological models is discussed.

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Metadata

Authors
Kodama, H., & Sasaki, M.
Venue
Progress of Theoretical Physics Supplement
Published
1984
Volume
78
Pages
1-166
ISSN
0375-9687 (ISSN-L)
OpenAlex
W2023724948
Cited by
1,671
References
0
FWCI
5.21
Type
journal article
Language
en
Open access
closed

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CoChat. (2026). Citation check: Cosmological Perturbation Theory. https://app.cochat.ai/papers/10.1143/ptps.78.1
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Kodama, H., & Sasaki, M. (1984). Cosmological Perturbation Theory. Progress of Theoretical Physics Supplement. https://doi.org/10.1143/ptps.78.1

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Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).

Semantic Scholar’s data is described in: Kinney, R., et al. (2023). The Semantic Scholar Open Data Platform. arXiv:2301.10140.