ar X iv : g r - qc / 0 61 11 46 v 1 2 8 N ov 2 00 6 Massive scalar field quasinormal modes of a Schwarzschild black hole surrounded by quintessence
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چکیده
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 u increases, while the imaginary part in absolute value decreases linearly which leads to damping more slowly and the frequencies having a limited value. Moreover, owing to the presence of the quintessence, the massive scalar field damps more slowly. Massive scalar field quasinormal modes of a Schwarzschild black hole surrounded by quintessence2
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ar X iv : g r - qc / 0 61 11 46 v 2 2 9 N ov 2 00 6 Massive scalar field quasinormal modes of a Schwarzschild black hole surrounded by quintessence
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 u increases, while the imaginary part in absolute value decreases l...
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