中国物理B ›› 2006, Vol. 15 ›› Issue (6): 1184-1189.doi: 10.1088/1009-1963/15/6/010

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Thermodynamical quantities around\\[1.8mm] a RNAdS black hole

米丽琴1, 黎忠恒2   

  1. (1)Department of Physics, Zhanjiang Normal College, Zhanjiang 524048, China; (2)Department of Physics, Zhejiang University of Technology, Hangzhou 310032, China
  • 收稿日期:2005-10-08 修回日期:2005-12-18 出版日期:2006-06-20 发布日期:2006-06-20
  • 基金资助:
    Project supported by the National Natural Science Foundation of China (Grant No 10375051).

Thermodynamical quantities around a RNAdS black hole

Mi Li-Qin (米丽琴)a, Li Zhong-Heng (黎忠恒)ab   

  1. a Department of Physics, Zhanjiang Normal College, Zhanjiang 524048, China; b Department of Physics, Zhejiang University of Technology, Hangzhou 310032, China
  • Received:2005-10-08 Revised:2005-12-18 Online:2006-06-20 Published:2006-06-20
  • Supported by:
    Project supported by the National Natural Science Foundation of China (Grant No 10375051).

摘要: The entropy density, energy density, pressure and equation of state around the RNAdS black hole are calculated in the WKB approximation on the Teukolsky-type master equation. The appearance of spin-dependent terms is demonstrated. The existence of these terms shows that the black hole radiation is not exactly thermal radiation and the black hole entropy is not strictly proportional to the area of the event horizon.

关键词: thermodynamical quantities, equation of state, RNAdS black hole, WKB approximation, Boulware state

Abstract: The entropy density, energy density, pressure and equation of state around the RNAdS black hole are calculated in the WKB approximation on the Teukolsky-type master equation. The appearance of spin-dependent terms is demonstrated. The existence of these terms shows that the black hole radiation is not exactly thermal radiation and the black hole entropy is not strictly proportional to the area of the event horizon.

Key words: thermodynamical quantities, equation of state, RNAdS black hole, WKB approximation, Boulware state

中图分类号:  (Quantum aspects of black holes, evaporation, thermodynamics)

  • 04.70.Dy
04.62.+v (Quantum fields in curved spacetime) 97.60.Lf (Black holes)