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2008 | 6 | 2 | 194-198
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Massive scalar field quasinormal modes of a Schwarzschild black hole surrounded by quintessence

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Abstracts
EN
We present the quasinormal frequencies of the massive scalar field in the background of a Schwarzchild black hole surrounded by quintessence with the third-order WKB method. The mass of the scalar field u plays an important role in studying the quasinormal frequencies, the real part of the frequencies increases linearly as mass of the field u increases, while the imaginary part in absolute value decreases linearly which leads to damping more slowly than the massless scalar field. The frequencies have a limited value, so it is easier to detect the quasinormal modes. Moreover, owing to the presence of the quintessence, the massive scalar field damps more slowly.
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author
  • School of Physics and Optoelectronic Technology, Dalian university of Technology, 116024, Dalian, China, machunrui0312@163.com
author
  • School of Physics and Optoelectronic Technology, Dalian university of Technology, 116024, Dalian, China
author
  • College of Physical Science and Technology of Dalian University, 116024, Dalian, China
author
  • School of Physics and Optoelectronic Technology, Dalian university of Technology, 116024, Dalian, China
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Document Type
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YADDA identifier
bwmeta1.element.-psjd-doi-10_2478_s11534-008-0056-7
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