Quasinormal modes of gravitational perturbation around a Schwarzschild black hole surrounded by quintessence
Yu ZhangDepartment of Physics, Dalian University of Technology, Dalian, 116024, People's Republic of ChinaY. X. GuiDepartment of Physics, Dalian University of Technology, Dalian, 116024, People's Republic of China
2006en
ABI
Аннотация
In this paper, the quasinormal modes of gravitational perturbation around a Schwarzschild black hole surrounded by quintessence were evaluated by using the third-order WKB approximation. Due to the presence of quintessence, the gravitational wave damps more slowly.
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