arXiv · gr-qc/9606012
Inhomogeneity of Spatial Curvature for Inflation
Abstract
We study how the initial inhomogeneities of the spatial curvature affect the onset of inflation in the closed universe. We consider a cosmological model which contains a radiation and a cosmological constant. In order to treat the inhomogeneities in the closed universe, we improve the long wavelength approximation such that the non-small spatial curvature is tractable in the lowest order. Using the improved scheme, we show how large inhomogeneities of the spatial curvature prevent the occurrence of inflation.
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O. Iguchi, H. Ishihara, J. Soda. 1996-06-07. Inhomogeneity of Spatial Curvature for Inflation. https://doi.org/10.1103/physrevd.55.3337
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