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Phys. Rev. D 55, 3337–3345 (1997)

Inhomogeneity of spatial curvature for inflation

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Osamu Iguchi and Hideki Ishihara
Department of Physics, Tokyo Institute of Technology, Meguroku, Tokyo 152, Japan

Jiro Soda
Department of Physics, University of Alberta, Edmonton, Canada T6G 2J1
Department of Fundamental Sciences, FIHS, Kyoto University, Kyoto 606, Japan

Received 7 June 1996; published in the issue dated 15 March 1997

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 nonsmall 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.

© 1997 The American Physical Society

URL:
http://link.aps.org/doi/10.1103/PhysRevD.55.3337
DOI:
10.1103/PhysRevD.55.3337
PACS:
98.80.Cq, 98.80.Hw