The European Physical Journal C

, Volume 63, Issue 1, pp 133–138 | Cite as

Hawking radiation of Kerr–Newman–de Sitter black hole

  • Li Huaifan
  • Zhang Shengli
  • Wu Yueqin
  • Zhang Lichun
  • Zhao Ren
Regular Article - Theoretical Physics

Abstract

We extend the classical Damour–Ruffini method and discuss Hawking radiation in Kerr–Newman–de Sitter (KNdS) black hole. Under the condition that the total energy, angular momentum and charge of spacetime are conserved, taking the reaction of the radiation of the particle to the spacetime and the relation between the black hole event horizon and the cosmological horizon into consideration, we derive the black hole radiation spectrum. The radiation spectrum is no longer a pure thermal one. It is related to the change of the Bekenstein–Hawking entropy corresponding the black hole event horizon and the cosmological horizon. It is consistent with the underlying unitary theory.

PACS

04.70.Dy 04.62.+v 

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Copyright information

© Springer-Verlag / Società Italiana di Fisica 2009

Authors and Affiliations

  • Li Huaifan
    • 1
    • 2
  • Zhang Shengli
    • 1
  • Wu Yueqin
    • 2
  • Zhang Lichun
    • 2
  • Zhao Ren
    • 2
  1. 1.Department of Applied PhysicsXi’an Jiaotong UniversityXi’anP.R. China
  2. 2.Institute of Theoretical PhysicsShanxi Datong UniversityDatongP.R. China

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