Quasi-Normal Modes of Gravitational Perturbation around a Reissner-Nordstr(o)m Black Hole Surrounded by Quintessence
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摘要:
We investigate quasi-normal (QN) modes of gravitational perturbation around a Reissner-Nordstr(O)m black hole surrounded by quintessence.The third-order Wentzel-Kramers-BriIlouin 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-Nordstr(O)m black hole damp at a slower rate.