A Solution of the Einstein Equation in a Stationary Gravitational Field Due to a Rotating Source : Astrophysics and Relativity
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概要
- 論文の詳細を見る
The stationary and axially symmetric gravitational field due to a rotating deformed source can be treated by the Ernst equation. We prove analytically the validity of the solution of the Ernst equation that was presented as a possible solution in a previous paper for arbitrary real values of the deformation parameter δ. By means of analytic continuations of the solution we obtain a new solution in oblate spheroidal coordinates. This leads to a metric different from the Tomimatsu-Sato metric. From these solutions for real δ we determine the metric functions both in prolate and oblate spheroidal coordinates.
- 理論物理学刊行会の論文
- 1999-02-25
著者
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Tanimura Osamu
Faculty Of General Education Kanazawa University
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Shoichi HORI
Department of Physics, Kanazawa University
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HORI Shoichi
Faculty of General Educations, Kanazawa University:Kanazawa University
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TANIMURA Osamu
Faculty of General Education, Kanazawa University
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TANIMURA Osamu
Faculty of General Educations, Kanazawa University
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