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Quasinormal Modes of Electromagnetic Perturbation around a Stringy Black Hole

         

摘要

We investigate the electromagnetic perturbation around a stringy black hole. A second-order differential equation is obtained for the perturbation. The variation of the effective potential with r is presented. The complex frequencies of the quasinormal modes of electromagnetic perturbation around a stringy black hole are computed by the third Wentzel-Kramers-Brillouin (WKB) approximation. The results show that the parameters resulted from the compactification of higher dimensions can influence the quasinormal complex frequencies, and the Maxwell field around a stringy black hole damps more slowly than that around a Schwarzschild black hole.

著录项

  • 来源
    《中国物理快报:英文版》 |2007年第10期|2749-2751|共3页
  • 作者单位

    School of Physics and Optoelectronic Technology, Dalian University of Technology, Dalian 116024;

    School of Physics and Optoelectronic Technology, Dalian University of Technology, Dalian 116024;

    School of Physics and Optoelectronic Technology, Dalian University of Technology, Dalian 116024;

    School of Physics and Optoelectronic Technology, Dalian University of Technology, Dalian 116024;

  • 原文格式 PDF
  • 正文语种 chi
  • 中图分类 物理学;
  • 关键词

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