Energy of General Spherically Symmetric Solution in the Tetrad Theory of Gravitation

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概要

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• We find the most general spherically symmetric solution in a special class of the tetrad theory of gravitation. The tetrad gives the Schwarzschild metric. The energy is calculated using both the superpotential nethod and the Euclidean continuation method. We find that unless the time-space components of the tetrad go to zero faster than 1/√<r> at infinity, the two methods give different results and tha these results differ from the gravitational mass of the central gravitating body. This fact implies tha the time-space components of the tetrad describing an isolated spherical body must vanish faster tha 1/√<r> at infinity.

• 理論物理学刊行会の論文
• 1996-03-25

著者

• Shirafuji Takeshi

  Physics Department Saitama University

• HAYASHI Kenji

  Max-Planck-Institut fur Physik und Astrophysik Munchen

• HAYASHI Kenji

  Institute of Biological Sciences, University of Tsukuba

• SHIRAFUJI Tadahiko

  Department of Physics, Chiba University

• Hayashi K

  北海道大学水産科学研究科

• NACHED Gamal

  Physics Department, Saitama University

• Nached Gamal

  Physics Department Saitama University

• Nashed Gamal

  Physics Department Saitama University

• HAYASI Kenji

  Institute of Physics, University of Tokyo

• Hayashi Kenji

  Institute Of Physicsm Kitasato University

• Hayashi Kenji

  Max-planck Institut Fur Physik Und Astrophysik

• Hayashi Kenji

  Institute Of Biological Sciences University Of Tsukuba

• HAYASHI Kenji

  Institute of Physics, University of Tokyo

• HAYASHI Kenji

  Institute of Physics, Kitasato University

• HAYASHI Kenji

  Institute of Physics, Tokyo University

• SHIRAFUJI Takeshi

  Physics Department,Saitama University

• HAYASHI kiyoshi

  Faculty of Commerce, Meiji University

• NASHED Gamal

  Physics Department, Saitama University

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