Expanding Shell around a Void and Universe Model : Astrophysics and Relativity

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概要

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• Under the thin-shell approximation, we study the expansion of the shell formed around a single spherical void in the dust universe. We find that the peculiar velocity of the shell is determined mostly by the density parameter Ω_0. It also depends on the interior dust energy density, but is not so sensitive to a cosmological constant. This feature may open a possibility of determining the universe model from the surface motion of voids.

• 理論物理学刊行会の論文
• 1993-06-25

著者

• Sato Humitaka

  Department Of Physics Kyoto Univesity

• Sato Humitaka

  Department Of Nuclear Science Kyoto University

• MAEDA Keiichi

  Department of Earth Science and Astronomy, College of Arts and Science, University of Tokyo

• SAKAI NOBUYUKI

  Department of Chemical Engineering, Faculty of Engineering, Niigata University

• Maeda K

  Department Of Earth Science And Astronomy College Of Arts And Science University Of Tokyo

• Maeda Keiichi

  Research Institute For Fundamental Physics Kyoto University

• Sakai Nobuyuki

  Department Of Chemical Engineering Faculty Of Engineering Niigata University

• Maeda Kei-ichi

  Department of Physics, Waseda University

• Maeda Kei-ichi

  Research Institute For Fundamental Physics Kyoto University

• Maeda Kei-ichi

  Department Of Physics Kyoto University

• Maeda Kei-ichi

  Department Of Physics Waseda University

• Maeda Kei-ichi

  Research Institute For Fundamental Physics Kyoto Unviersity

• SUGIURA Norimasa

  Department of Physics, Kyoto University

• Sakai Nobuyuki

  Department Of Applied Chemistry Faculty Of Engineering The University Of Tokyo

• MAEDA Keiichi

  Department of Astronomy, University of Tokyo

• MAEDA Kei-ichi

  Research Institute for Fundamental Physics, Kyoto Unviersity ./ Department of Physics, Kyoto University

• Maeda Kei-ichi

  Department of Earth Science and Astronomy, College of Arts and Science, University of Tokyo

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