Kerr Metric, de Donder Condition and Gravitational Energy Density
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概要
- 論文の詳細を見る
The Kerr solution to the Einstein equation is explicitly rewritten into the one satisfying the de Donder condition. By using this result, the gravitational energy density, ht^0_0, in Einstein's definition is calculated completely. It is positive definite if a/m≲0.6, where a and m denote the angular-momentum parameter and the mass one, respectively. The validity of the conjecture proposed previously, which states that ht^0_0≧0 outside black holes if calculated under the de Donder condition, is discussed by means of the gravitational-wave solution, the Reissner-Nordstrom solution and the Kerr solution.
- 理論物理学刊行会の論文
- 1987-11-25
著者
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ABE Mitsuo
Research Institute for Mathematical Sciences, Kyoto University
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NAKANISHI Noboru
Research Institute for Mathematical Sciences Kyoto University
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Abe Mitsuo
Research Institute For Mathematical Sciences Kyoto University
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Nakanishi Noboru
Reseach Institure For Mathematical Sciences Kyoto University
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ICHINOSE Shoichi
Research Institute for Mathematical Sciences Kyoto University
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