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

Non-equilibrium Landauer transport model for Hawking radiation from a Reissner-Nordstrom black hole
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摘要 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. 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.
出处 《Chinese Physics B》 SCIE EI CAS CSCD 2012年第9期109-112,共4页 中国物理B(英文版)
基金 Project supported by the National Natural Science Foundation of China (Grant Nos. 10773002, 10875012, and 11175019) the Fundamental Research Funds for the Central Universities, China (Grant No. 105116)
关键词 Hawking radiation ENTROPY Landauer transport model black hole Hawking radiation, entropy, Landauer transport model, black hole
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参考文献34

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