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Phase Transition and Quasinormal Modes for Spherical Black Holes in 5D Gauss–Bonnet Gravity |
| Ming Zhang1,2**, Rui-Hong Yue3** |
1Faculty of Science, Xi'an Aeronautical University, Xi'an 710077
2National Joint Engineering Research Center of Special Pump System Technology, Xi'an 710077
3Center for Gravitation and Cosmology, College of Physical Science and Technology, Yangzhou University, Yangzhou 225009
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| Cite this article: |
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Ming Zhang, Rui-Hong Yue 2018 Chin. Phys. Lett. 35 040401 |
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Abstract We study the quasinormal modes (QNMs) of massless scalar perturbations to probe the van der Waals like SBH/LBH phase transition of anti-de Sitter black holes in five-dimensional (5D) Gauss–Bonnet gravity. It is found that the signature of this SBH/LBH phase transition is detected when the slopes of the QNMs frequency change drastically and differently in small and large black holes near the critical point. The obtained results further support that the QNMs can be a dynamic probe to investigate the thermodynamic properties in black holes.
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Received: 28 November 2017
Published: 13 March 2018
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| Fund: Supported by the National Natural Science Foundation of China under Grant Nos 11647050, 11675139 and 51575420, and the Scientific Research Program Funded by Shaanxi Provincial Education Department under Grant No 16JK1394. |
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