Equilibrium Condition in the Axisymmetric N-Reissner-Nordstrom Solution : Astrophysics and Relativity
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概要
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We solve the source-free Einstein-Maxwell equations in a static and axisymmetric spacetime by using the inverse scattering method that is one of the soliton techniques to solve the gravitational field equation. We obtain an exact solution that describes n Reissner-Nordstrom black holes located along the symmetry axis. We define the mass and charge of each black hole and study the condition for static equilibrium of black holes. We show that the equilibrium is realized only when all the black holes are extremal and the spacetime becomes Majumdar-Papapetrou type.
- 理論物理学刊行会の論文
- 1994-12-25
著者
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KOIKAWA Takao
School of Social Information Studies, Otsuma Women's University
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Koikawa Takao
School Of Social Information Studies Otsuma Women's University
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Koikawa Takao
Research Institute For Fundamental Physics Kyoto University
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Azuma Takahiro
Dokkyo Univ. Soka Jpn
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Azuma Takahiro
Research Institute For Theoretical Physics Hiroshima University
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AZUMA Takahiro
Department of Mathematics, King's College London
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