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The Concrete Quantum Tunneling Spectrum of Reissner-Nordstrom Black Holes

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Abstract

A canonical ensemble model for a R-N black hole quantum tunneling radiation is introduced in this paper. We discover that the probability distribution function is equal to the emission rate of a spherical shell in the Parikh-Wilczek tunneling framework. Taking the generalized uncertainty principle into account, the probability distribution function corresponding to the emission shell system can be calculated with this model. As a result the concrete quantum tunneling spectrum for a R-N black hole is obtained.

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Authors and Affiliations

  1. Center for Astrophysics, Guangzhou University, Guangzhou, 510006, People’s Republic of China

    Sina Chen & Jingyi Zhang

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  1. Sina Chen
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  2. Jingyi Zhang
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Correspondence to Jingyi Zhang.

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Project supported by the National Natural Science Foundation of China Under Grant Nos. 11273009 and 11303006.

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Chen, S., Zhang, J. The Concrete Quantum Tunneling Spectrum of Reissner-Nordstrom Black Holes. Int J Theor Phys 55, 1652–1657 (2016). https://doi.org/10.1007/s10773-015-2802-0

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  • DOI: https://doi.org/10.1007/s10773-015-2802-0

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