Non-equilibrium Landauer transport model for Hawking radiation from a Reissner–Nordstrom black hole

doi:10.1088/1674-1056/21/9/090402

Abstract The recent work of Nation et al., in which the Hawking radiation energy and entropy flow from a black hole is considered to be produced in a one-dimensional Landauer transport process, is extended to the case of a Reissner-Nordstrom black hole. The energy flow contains not only the contribution of the thermal flux but also that of the particle flux. It is found that the charge can also be transported via the one-dimensional quantum tunnel. Because of the existence of the electrostatic potential, the entropy production rate is shown to be smaller than that of the Schwarzschild black hole.

Keywords: Hawking radiation entropy Landauer transport model black hole

Received: 29 March 2011
Revised: 23 May 2012
Accepted manuscript online:

PACS:	04.70.Dy	(Quantum aspects of black holes, evaporation, thermodynamics)
	03.67.Hk	(Quantum communication)
	05.30.-d	(Quantum statistical mechanics)

Fund: Project supported by the National Natural Science Foundation of China (Grant Nos. 10773002, 10875012, and 11175019) and the Fundamental Research Funds for the Central Universities, China (Grant No. 105116).

Corresponding Authors: Liu Wen-Biao
E-mail: wbliu@bnu.edu.cn

Cite this article:

Zeng Xiao-Xiong (曾晓雄), Zhou Shi-Wei (周史薇), Liu Wen-Biao (刘文彪) Non-equilibrium Landauer transport model for Hawking radiation from a Reissner–Nordstrom black hole 2012 Chin. Phys. B 21 090402

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Non-equilibrium Landauer transport model for Hawking radiation from a Reissner–Nordstrom black hole

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