中国物理B ›› 2004, Vol. 13 ›› Issue (6): 974-978.doi: 10.1088/1009-1963/13/6/032

• • 上一篇    

Quantum statistical entropy for Kerr－de Sitter black hole

张丽春, 武月琴, 赵仁   

  1. Department of Physics, Yanbei Normal Institute, Datong 037000, China
  • 收稿日期:2003-07-28 修回日期:2003-12-12 出版日期:2004-07-05 发布日期:2005-07-05
  • 基金资助:
    Project supported by the Natural Science Foundation of Shanxi Province, China (Grant No 20001009).

Quantum statistical entropy for Kerr－de Sitter black hole

Zhang Li-Chun (张丽春), Wu Yue-Qin (武月琴), Zhao Ren (赵仁)   

  1. Department of Physics, Yanbei Normal Institute, Datong 037000, China
  • Received:2003-07-28 Revised:2003-12-12 Online:2004-07-05 Published:2005-07-05
  • Supported by:
    Project supported by the Natural Science Foundation of Shanxi Province, China (Grant No 20001009).

PDF (PC)

435

赞

摘要： Improving the membrane model by which the entropy of the black hole is studied, we study the entropy of the black hole in the non-thermal equilibrium state. To give the problem stated here widespread meaning, we discuss the (n+2)-dimensional de Sitter spacetime. Through discussion, we obtain that the black hole's entropy which contains two horizons (a black hole's horizon and a cosmological horizon) in the non-thermal equilibrium state comprises the entropy corresponding to the black hole's horizon and the entropy corresponding to the cosmological horizon. Furthermore, the entropy of the black hole is a natural property of the black hole. The entropy is irrelevant to the radiation field out of the horizon. This deepens the understanding of the relationship between black hole's entropy and horizon's area. A way to study the bosonic and fermionic entropy of the black hole in high non-thermal equilibrium spacetime is given.

关键词: quantum statistics, brick-wall method, membrane model, entropy of black hole, higher-dimensional black hole

Abstract: Improving the membrane model by which the entropy of the black hole is studied, we study the entropy of the black hole in the non-thermal equilibrium state. To give the problem stated here widespread meaning, we discuss the (n+2)-dimensional de Sitter spacetime. Through discussion, we obtain that the black hole's entropy which contains two horizons (a black hole's horizon and a cosmological horizon) in the non-thermal equilibrium state comprises the entropy corresponding to the black hole's horizon and the entropy corresponding to the cosmological horizon. Furthermore, the entropy of the black hole is a natural property of the black hole. The entropy is irrelevant to the radiation field out of the horizon. This deepens the understanding of the relationship between black hole's entropy and horizon's area. A way to study the bosonic and fermionic entropy of the black hole in high non-thermal equilibrium spacetime is given.

Key words: quantum statistics, brick-wall method, membrane model, entropy of black hole, higher-dimensional black hole

中图分类号:  (Black holes)

  • 97.60.Lf
04.20.Gz (Spacetime topology, causal structure, spinor structure) 98.80.-k (Cosmology) 04.70.Dy (Quantum aspects of black holes, evaporation, thermodynamics)