Thermal Properties of Self-Gravitating Plane-Symmetric Configuration
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概要
- 論文の詳細を見る
As a limiting case of rotating stars, thermal properties of infinite plane-symmetric self-gravitating gas are investigated. Such a configuration is characterized by surface density of the plane instead of stellar mass. In the Kelvin contraction, temperature of the interior decreases, if the surface density is kept constant. If the accretion of matter takes place, or if the angular momenta are transferred outward, the surface density will increase. In this case, the temperature of the interior may increase. When a nuclear burning is ignited, it is thermally unstable in most cases, even when electrons are non-degenerate. This thermal instability is one of the essential differences of the plane-symmetric configuration from the spherical star. Such instabilities are computed for different cases of nuclear fuels. This type of nuclear instability is the same phenomenon as thermal instability of a thin shell burning in a spherical star.
- 理論物理学刊行会の論文
- 1976-09-25
著者
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IKEUCHI Satoru
Department of Astrophysics, Nagoya University
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HARA Tetsuya
Department of Anesthesiology, Nagasaki University School of Medicine
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SUGIMOTO Daiichiro
Department of Earth Science and Astronomy College of General Education, University of Tokyo
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Ikeuchi Satoru
Department Of Astrophysics Nagoya University
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Sugimoto Daiichiro
Department Of Earth Science And Astronomy University Of Tokyo
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Sugimoto Daiichiro
Department Of Earth Science And Astronomy College Of General Education 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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Sugimoto Daiichiro
Department of General Systems Studies, College of Arts and Sciences, The University of Tokyo
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Hara Tetsuya
Research Center for Nuclear Physics, Osaka. University
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