General Relativistic Modification of a Pulsar Electromagnetic Field
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概要
- 論文の詳細を見る
We consider an exterior electromagnetic field surrounding a rotating star endowed with a dipole magnetic field in the context of general relativity. The analytic solution for a stationary configuration is obtained, and the general relativistic modifications and the implications for pulsar radiation are investigated in detail. We find that the general relativistic corrections of both the electric field strength and the curvature redii of magnetic field lines tend to enhance the curvature radiation photon energy.
- 理論物理学刊行会の論文
- 2000-12-25
著者
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KONNO Kohkichi
Department of Applied Physics, Hokkaido University
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Konno Kohkichi
Department Of Applied Physics Hokkaido University:center Of Education And Research For Topological S
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Konno K
Department Of Physics Hiroshima University
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Kojima Yasuaki
Graduate School Of Engineering Hiroshima University
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KOJIMA Yasufumi
Department of Physics, Tokyo Metropolitan University
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Kojima Y
Department Of Physics Hiroshima University
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Kojima Yasufumi
Department Of Physics Hiroshima University
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KOJIMA Yasufumi
Department of Physics, University of Wales
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