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Quasi-Normal Modes of Gravitational Perturbation around a Reissner-Nordström Black Hole Surrounded by Quintessence |
| Mahamat Saleh1, Bouetou Bouetou Thomas1,2,3, Timoleon Crepin Kofane1,3 |
| 1Department of Physics, Faculty of Science, University of Yaounde I, PO Box 812, Cameroon2Ecole Nationale Supérieure Polytechnique, University of Yaounde I, PO Box 8390, Cameroon3The Abdus Salam International Centre for Theoretical Physics, PO Box 586, Strada Costiera, II-34014, Trieste, Italy |
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Mahamat Saleh, Bouetou Bouetou Thomas, Timoleon Crepin Kofane 2009 Chin. Phys. Lett. 26 109802 |
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Abstract We investigate quasi-normal (QN) modes of gravitational perturbation around a Reissner-Nordström black hole surrounded by quintessence. The third-order Wentzel-Kramers-Brillouin approximation is used to evaluate QN frequencies. The behavior of the gravitational perturbation is plotted for some frequencies. Due to the presence of quintessence, QN modes of the Reissner-Nordström black hole damp at a slower rate.
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98.80.Hw
95.30.Sf
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Received: 13 March 2009
Published: 27 September 2009
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