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Chin. Phys. B, 2010, Vol. 19(6): 060401    DOI: 10.1088/1674-1056/19/6/060401
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Quasinormal modes of the scalar field in five-dimensional Lovelock black hole spacetime

Chen Ju-Hua(陈菊华) and Wang Yong-Jiu(王永久)
College of Physics and Information Science, Hunan Normal University, Changsha 410081, China
Abstract  In this paper, using the third-order WKB approximation, we investigate the quasinormal frequencies of the scalar field in the background of a five-dimensional Lovelock black hole. We find that the ultraviolet correction to Einstein theory in the Lovelock theory makes the scalar field decay more slowly and oscillate more quickly, and the cosmological constant makes the scalar field decay more slowly and oscillate more slowly in the Lovelock black hole background.
Keywords:  quasinormal modes      third-order WKB approximation      Lovelock black hole  
Received:  08 August 2009      Accepted manuscript online: 
PACS:  04.70.Dy (Quantum aspects of black holes, evaporation, thermodynamics)  
  98.80.Jk (Mathematical and relativistic aspects of cosmology)  
  04.60.-m (Quantum gravity)  
Fund: Project supported by the National Natural Science Foundation of China (Grant No.~10873004), the Key Project of the National Natural Science Foundation of China (Grant No.~10935013), the Scientific Research Fund of the Educational Department of Hunan Pro

Cite this article: 

Chen Ju-Hua(陈菊华) and Wang Yong-Jiu(王永久) Quasinormal modes of the scalar field in five-dimensional Lovelock black hole spacetime 2010 Chin. Phys. B 19 060401

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