Quasinormal modes of dilaton-de Sitter black holes: scalar perturbations

被引:0
作者
Sharmanthie Fernando
机构
[1] Northern Kentucky University,Department of Physics and Geology
来源
General Relativity and Gravitation | 2016年 / 48卷
关键词
Static; Dilation; Near-extreme; Black hole; Stability; Quasinormal modes; Pöschl Teller;
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摘要
Dilaton black hole solutions in low energy string theory (well known as GMGHS black holes) have analogue black holes with a cosmological constant derived by Gao and Zhang. Here, we study quasi normal modes of this dilaton-de Sitter black hole under neutral scalar field perturbations. We have employed the sixth order WKB analysis to compute the quasi normal mode frequencies. A detailed study is done for the quasi normal mode frequencies by varying the parameters in the theory such as the mass, cosmological constant, dilaton charge and the spherical harmonic index. For the massive scalar field we observed that the usual quasi resonance modes that exists for asymptotically flat black holes do not exist for this particular black hole. We have approximated the scalar field potential of the near-extreme dilaton de Sitter black hole with the Pöschl-Teller potential and have presented exact quasi normal frequencies.
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