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Chin. Phys. B, 2008, Vol. 17(8): 2804-2810    DOI: 10.1088/1674-1056/17/8/010
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Hawking radiation from Kerr--Newman de Sitter black hole via anomalies

Lin Kai(林恺), Yang Shu-Zheng(杨树政), and Zeng Xiao-Xiong(曾晓雄)
Institute of Theoretical Physics, China West Normal University, Nanchong 637002, China
Abstract  In this paper, Hawking radiation from the Kerr--Newman de Sitter black hole is studied via gauge anomaly and gravitational anomaly. The obtained results of Hawking radiation from the event horizon and the cosmological horizon accord with those by other methods.
Keywords:  gauge anomaly      gravitational anomaly      Hawking radiation      Kerr--Newman de Sitter black hole  
Received:  17 September 2007      Revised:  16 November 2007      Accepted manuscript online: 
PACS:  04.70.Dy (Quantum aspects of black holes, evaporation, thermodynamics)  
  04.60.-m (Quantum gravity)  
  95.30.Sf (Relativity and gravitation)  
  97.60.Lf (Black holes)  
  98.80.Cq (Particle-theory and field-theory models of the early Universe (including cosmic pancakes, cosmic strings, chaotic phenomena, inflationary universe, etc.))  
  98.80.Qc (Quantum cosmology)  
Fund: Project supported by the National Natural Science Foundation of China (Grant No 10773008).

Cite this article: 

Lin Kai(林恺), Yang Shu-Zheng(杨树政), and Zeng Xiao-Xiong(曾晓雄) Hawking radiation from Kerr--Newman de Sitter black hole via anomalies 2008 Chin. Phys. B 17 2804

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