Large-Scale Structures and Streaming Velocities Due to Open Cosmic Strings : Astrophysics and Relativity
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概要
- 論文の詳細を見る
Large-scale structures of the universe could be simply explained by wakes, which are the traces of open cosmic strings. Sheet-like structures would be the wakes, filaments would be intersections of such wakes, and rich clusters of galaxies would be high density regions where three wakes intersect. The streaming velocities and density distributions around such objects are calculated assuming planar, cylindrical and spherical symmetries. Under some plausible assumptions, the large values of the large-scale streaming velocities (〜600 km/sec, 〜50 Mpc) could be produced.
- 理論物理学刊行会の論文
- 1989-06-25
著者
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HARA Tetsuya
Department of Anesthesiology, Nagasaki University School of Medicine
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Hariu T.
Yamagata University
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MIYOSHI Shigeru
Department of Physics, Kyoto Sangyo University
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Hara Tetsuya
Research Institute For Fundamental Physics Kyoto University
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Miyoshi Shigeru
Department Of Physics Kyoto Sangyo University
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HARA Takashi
Institute of Physics, College of Arts and Sciences University of Tokyo
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Hara Tetsuya
Department Of Anesthesiology Nagasaki Rosai Hospital
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HARA Takashi
Institute of Physics, College of Arts and Science University of Tokyo : Courant Institute of Mathematical Sciences, New York University
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MIYOSHI Shigeru
Department of Physics,Kyoto Sangyo University
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HARA Tetsuya
Department of Physics, Kyoto University
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Miyoshi Sigeru
Department of Physics, Kyoto Sangyo University
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Hara Tetsuya
Research Center for Nuclear Physics, Osaka. University
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