Cosmological Perturbation Theory

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ID: 291943
1984
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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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openalex_W2023724948 Use this key to autocite in the manuscript while using SciMatic Manuscript Manager or Thesis Manager
Authors Hideo Kodama, Misao Sasaki
Journal Progress of Theoretical Physics Supplement
Year 1984
DOI
10.1143/ptps.78.1
URL
https://academic.oup.com/ptps/article-pdf/doi/10.1143/PTPS.78.1/5321391/78-1.pdf
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