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The Tunneling Radiation Characteristics of Kerr-Newman de Sitter Black Hole

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Abstract

The strictly thermal spectrum in dragging coordinate system and the tunneling radiation characteristics of stationary axisymmetry Kerr-Newman de Sitter black hole is studied. The result shows that the tunneling rates at the event and cosmological horizon are related to the change of Bekenstein-Hawking entropy and that the factual radiation spectrum is not strictly pure thermal. Thus an exact correction to the Hawking thermal spectrum is present.

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Correspondence to Shuzheng Yang.

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Yang, S., Jiang, Q. & Li, H. The Tunneling Radiation Characteristics of Kerr-Newman de Sitter Black Hole. Int J Theor Phys 46, 625–636 (2007). https://doi.org/10.1007/s10773-006-9207-z

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  • DOI: https://doi.org/10.1007/s10773-006-9207-z

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