Physically Acceptable Solution of Einstein's Equation for Many-Body System
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概要
- 論文の詳細を見る
Einstein's gravitational equation for slowly moving particles is solved up to the order of the post-post-Newtonian approximation. Though in this order the metric tensor diverges at spatial infinity when de Donder's coordinate condition is employed, it is shown that there exist a class of coordinate systems in which the metric tensor is Minkowskian at infinity. We get solutions for the metric tensor up to the order of c^<-6>. Using these solutions, we obtain, in the post-Newtonian order, the most general Hamiltonian for many-body system. The G・υ^4-part of the potential in the post-post-Newtonian order is also given.
- 理論物理学刊行会の論文
- 1973-08-25
著者
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Okamura Hiroshi
Department Of Surgery Faculty Of Medicine Tohoku University
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OHTA Tadayuki
Department of Biological Science, Aichi University of Education
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Okamura Hiroshi
Department Of Materials Processing Graduate School Of Engineering Tohoku University
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Ohta Tadayuki
Department Of Mathematical Physics College Of Technology Seikei University
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Hiida Kichiro
Institute For Nuclear Study University Of Tokyo
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KIMURA Toshiei
Research Institute for Theoretical Physics, Hiroshima University
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Kimura Toshiei
Research Institute For Theoretical Physics Hiroshima University
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Ohta Tadayuki
Department Of Biological Science Aichi University Of Education
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Hiida Kichiro
Institute For Nuclear Study Tokyo University
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