Quantum nonthermal radiation and horizon surface gravity of an arbitrarily accelerating black hole with electric charge and magnetic charge

doi:10.1088/1674-1056/22/3/039701

Abstract With a new tortoise coordinate transformation, we discussed the quantum nonthermal radiation characteristics near the event horizon by studying the Hamilton–Jacobi equation of a scalar particle in the curve space–time, and obtained the event horizon surface gravity and the Hawking temperature on the event horizon. The results showed that there is a crossing of particle energy near the event horizon. We derived the maximum overlap of the positive and negative energy levels. It was also found that the Hawking temperature of a black hole depends on not only the time, but also the angle. There is a problem of dimension in the usual tortoise coordinate, so the present results obtained by using a correct-dimension new tortoise coordinate transformation may be more reasonable.

Keywords: tortoise coordinate transformation black hole quantum nonthermal radiation event horizon surface gravity

Received: 31 May 2012
Revised: 17 August 2012
Accepted manuscript online:

PACS:	97.60.Lf	(Black holes)
	04.70.-s	(Physics of black holes)

Fund: Project supported by the National Natural Science Foundation of China (Grant Nos. 10873003 and 11045005) and the Natural Science Foundation of Zhejiang Province, China (Grant No. Y6090739).

Corresponding Authors: Pan Wei-Zhen
E-mail: panwz8@usx.edu.cn

Cite this article:

Xie Zhi-Kun (谢志堃), Pan Wei-Zhen (潘伟珍), Yang Xue-Jun (杨学军) Quantum nonthermal radiation and horizon surface gravity of an arbitrarily accelerating black hole with electric charge and magnetic charge 2013 Chin. Phys. B 22 039701

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Quantum nonthermal radiation and horizon surface gravity of an arbitrarily accelerating black hole with electric charge and magnetic charge

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