Large-Scale Structures Due to Wakes of Open Cosmic Strings : Astrophysics and Relativity
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概要
- 論文の詳細を見る
Numerical calculations are performed for the large scale distribution of dark matter and galaxies under the open cosmic string model. According to the scenario, sheetlike structures are wakes which are traces of open cosmic strings, filaments are intersections of such wakes, and rich clusters of galaxies are high density regions where three wakes intersect. Typical isodensity surfaces and cone diagrams are shown for the three types of structures. Patterns by a slice selection of the wakes around a rich cluster are compared with the CfA observations.
- 理論物理学刊行会の論文
- 1990-11-25
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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MORIOKA Shorji
Department of Physics, Kyoto Sangyo University
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MIYOSHI Shigeru
Institute of Astronomy
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Hara Tetsuya
Research Institute For Fundamental Physics Kyoto University
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MORIOKA Shin-ichi
Faculty of Engineering Science Osaka University
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Morioka S
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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HARA Tetsuya
Department of Physics, Kyoto University
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MORIOKA Shin-ichi
Department of Nuclear Engineering, Osaka 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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