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The research on the quantum tunneling characteristics and the radiation spectrum of the stationary axisymmetric black hole
作者姓名:YANG ShuZheng  LI HuiLing  JIANG QingQuan & LIU MenQuan Institute of Theoretical Physics  China West Normal University  Nanchong  China
作者单位:YANG ShuZheng,LI HuiLing,JIANG QingQuan & LIU MenQuan Institute of Theoretical Physics,China West Normal University,Nanchong 637002,China
基金项目:the Foundation for Fundamental Research Projects of Sichuan Province(Grant No. 05JY029-092)
摘    要:At the event horizon and the cosmological horizon of the stationary axisymmetric Kerr-Newman black hole in the de Sitter space-time background, the tunneling rate of the charged particles is relevant with Bekenstein-Hawking entropy and the real radiation spectrum is not strictly pure thermal, but consistent with the underlying unitary theory in quantum mechanics. This is a feasible interpretation for the paradox of the black hole information loss. Taking the self-gravitation action, energy conservation, angular momentum conservation and charge conservation into account, the derived radiation spectrum is a correct amendment to the Hawking pure thermal spectrum.

收稿时间:11 December 2005
修稿时间:21 September 2006

The research on the quantum tunneling characteristics and the radiation spectrum of the stationary axisymmetric black hole
YANG ShuZheng,LI HuiLing,JIANG QingQuan & LIU MenQuan Institute of Theoretical Physics,China West Normal University,Nanchong ,China.The research on the quantum tunneling characteristics and the radiation spectrum of the stationary axisymmetric black hole[J].Science in China(Physics Astronomy),2007,50(2):249-260.
Authors:Yang ShuZheng  Li HuiLing  Jiang QingQuan  Liu MenQuan
Institution:Institute of Theoretical Physics,China West Normal University,Nanchong 637002,China
Abstract:At the event horizon and the cosmological horizon of the stationary axisymmetric Kerr-Newman black hole in the de Sitter space-time background,the tunneling rate of the charged particles is relevant with Bekenstein-Hawking entropy and the real radiation spectrum is not strictly pure thermal,but consistent with the underlying unitary theory in quantum mechanics.This is a feasible interpretation for the paradox of the black hole information loss.Taking the self-gravitation action,energy conservation,angular momentum conservation and charge conservation into account,the derived radiation spectrum is a correct amendment to the Hawking pure thermal spectrum.
Keywords:Kerr-Newman de Sitter black hole  energy conservation  charge conservation  angular momentum conservation  funneling rate  Bekenstein-Hawking entropy
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