中国物理B ›› 2005, Vol. 14 ›› Issue (9): 1736-1744.doi: 10.1088/1009-1963/14/9/009

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Quantum radiation of non-stationary Kerr-Newman-de Sitter black hole

蒋青权, 杨树政, 李慧玲   

  1. Institute of Theoretical Physics, China West Normal University,Nanchong 637002, China}
  • 收稿日期:2005-01-20 修回日期:2005-05-16 出版日期:2005-09-20 发布日期:2005-09-20
  • 基金资助:
    Project supported by the National Natural Science Foundation of China (Grant No 10347008).

Quantum radiation of non-stationary Kerr-Newman-de Sitter black hole

Jiang Qing-Quan (蒋青权), Yang Shu-Zheng (杨树政), Li Hui-Ling (李慧玲)   

  1. Institute of Theoretical Physics, China West Normal University, Nanchong 637002, China
  • Received:2005-01-20 Revised:2005-05-16 Online:2005-09-20 Published:2005-09-20
  • Supported by:
    Project supported by the National Natural Science Foundation of China (Grant No 10347008).

摘要: By introducing a new tortoise coordinate transformation, we investigate the quantum thermal and non-thermal radiations of a non-stationary Kerr--Newman--de Sitter black hole. The accurate location and radiate temperature of the event horizon as well as the maximum energy of the non-thermal radiation are derived. It is shown that the radiate temperature and the maximum energy are related to not only the evaporation rate, but also the shape of the event horizon, moreover the maximum energy depends on the electromagnetic potential. Finally, we use the results to reduce the non-stationary Kerr--Newman black hole, the non-stationary Kerr black hole, the stationary Kerr--Newman--de Sitter black hole, and the static Schwarzshild black hole.

关键词: quantum thermal radiation, quantum non-thermal radiation, tortoise coordinate trans-formation, Kerr-Newman-de Sitter black hole

Abstract: By introducing a new tortoise coordinate transformation, we investigate the quantum thermal and non-thermal radiations of a non-stationary Kerr--Newman--de Sitter black hole. The accurate location and radiate temperature of the event horizon as well as the maximum energy of the non-thermal radiation are derived. It is shown that the radiate temperature and the maximum energy are related to not only the evaporation rate, but also the shape of the event horizon, moreover the maximum energy depends on the electromagnetic potential. Finally, we use the results to reduce the non-stationary Kerr--Newman black hole, the non-stationary Kerr black hole, the stationary Kerr--Newman--de Sitter black hole, and the static Schwarzshild black hole.

Key words: quantum thermal radiation, quantum non-thermal radiation, tortoise coordinate trans-formation, Kerr-Newman-de Sitter black hole

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

  • 04.70.Dy
97.60.Lf (Black holes)