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
Quasi-Normal Modes of Gravitational Perturbation around a Reissner-Nordström Black Hole Surrounded by Quintessence
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
摘要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.
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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2009, Vol. 26 
