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Quasi-Normal Oscillations of a Black Hole with Deficit Angle for Electromagnetic Perturbations |
LI Xin-Zhou;ZHOU Bing-Lu;ZHU Jiong-Ming |
Department of Physics, Shanghai Normal University, Shanghai 200234 |
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Cite this article: |
LI Xin-Zhou, ZHOU Bing-Lu, ZHU Jiong-Ming 2001 Chin. Phys. Lett. 18 482-484 |
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Abstract We consider an electromagnetic perturbation in the external space-time of a black hole with deficit angle, and describe the perturbation equation. Approximate analytic formulas for the quasi-normal frequencies have been provided, which may play a significant role in the continuing search for gravitational radiation and black hole. These frequencies can be distinguished from the ordinary quasi-normal frequencies of Schwarzschild black hole.
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Keywords:
04.20.Jb
04.30.Nk
04.25.Nx
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Published: 01 April 2001
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PACS: |
04.20.Jb
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(Exact solutions)
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04.30.Nk
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(Wave propagation and interactions)
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04.25.Nx
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(Post-Newtonian approximation; perturbation theory; related Approximations)
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