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Quasinormal modes of a Schwarzschild black hole surrounded by free static spherically symmetric quintessence: electromagnetic perturbations

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Abstract

In this paper, we evaluated the quasinormal modes of electromagnetic perturbation in a Schwarzschild black hole surrounded by the static spherically symmetric quintessence by using the third-order WKB approximation when the quintessential state parameter w q in the range of −1/3 <  w q <  0. Due to the presence of quintessence, Maxwell field damps more slowly. And when at −1 <  w q <  −1/3, it is similar to the black hole solution in the ds/Ads spacetime. The appropriate boundary conditions need to be modified.

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Authors and Affiliations

  1. School of Physics and Optoelectronic Technology, Dalian University of Technology, Dalian, 116024, People’s Republic of China

    Yu Zhang, Yuanxing Gui & Fei Yu

  2. Department of Materials Science and Engineering, Chungnam National University, 220 Gung-dong, Yuseong-gu, Daejeon, 305-764, Korea

    FengLin Li

Authors
  1. Yu Zhang
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  2. Yuanxing Gui
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  3. Fei Yu
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  4. FengLin Li
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Correspondence to Yu Zhang.

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Zhang, Y., Gui, Y., Yu, F. et al. Quasinormal modes of a Schwarzschild black hole surrounded by free static spherically symmetric quintessence: electromagnetic perturbations. Gen Relativ Gravit 39, 1003–1010 (2007). https://doi.org/10.1007/s10714-007-0434-2

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  • DOI: https://doi.org/10.1007/s10714-007-0434-2

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