On the Degree of Generality of Inflation in Friedmann Cosmological Models with a Massive Scalar Field : Astrophysics and Relativity
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概要
- 論文の詳細を見る
Friedmann cosmological models with a massive minimally coupled scalar field are investigated by numerical methods. It is indicated that the majority of the solutions undergo the inflationary stage in flat and open models. In a closed model the ratio of the number of solutions without adequate inflation to the number of the total solutions are obtained numerically.
- 理論物理学刊行会の論文
- 1988-03-25
著者
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Sato Humitaka
Department Of Nuclear Science Kyoto University
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Ishihara Hideki
Department Of Mathematics And Physics Graduate School Of Science Osaka City University
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Ishihara Hideki
Department Of Physics Kyoto University
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BELINSKY V.A.
Department of Physics, Kyoto University
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KHALATNIKOV I.M.
Department of Physics, Kyoto University
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Belinsky V.a.
Department Of Physics Kyoto University:(present Address)l. D. Landau Institute Of Theoretical Physic
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Khalatnikov I.m.
Department Of Physics Kyoto University:(present Address)l. D. Landau Institute Of Theoretical Physic
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BELINSKY V.A.
Department of Physics, Kyoto University:(Present address)L. D. Landau Institute of Theoretical Physics, USSR Academy of Sciences
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KHALATNIKOV I.M.
Department of Physics, Kyoto University:(Present address)L. D. Landau Institute of Theoretical Physics, USSR Academy of Sciences
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SATO Humitaka
Department of Physics, Kyoto University
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ISHIHARA Hideki
Department of Physics, Kyoto University
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