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Tunneling Radiation of Vector Particles from a Quantum Correction Black Hole

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Abstract

The purpose of this paper is to discuss the Hawking radiation of vector particles from a quantum correction black hole by the mean of quantum tunneling. In order to achieve this purpose, based on the Proca field equation and WKB approximation, the quantum tunneling method is used to calculate the tunneling rate and Hawking temperature of the black hole. According to the analysis of the consequences, we find that the tunneling rate and Hawking temperature are related to the quantum parameter besides the horizon radius and mass of the black hole. Furthermore, when the results are compared with those of scalar particles and fermions of the black hole, no difference is found. Therefore, the tunneling rate and Hawing temperature of the black hole do not change with the type of radiation particles.

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Acknowledgments

This work is supported in part by the National Natural Science Foundation of China (Grant No. 11703018).

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Authors and Affiliations

  1. College of Physics Science and Technology, Shenyang Normal University, Shenyang, 110034, China

    De-Wen Song & Hui-Ling Li

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  1. De-Wen Song
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  2. Hui-Ling Li
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Correspondence to Hui-Ling Li.

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Song, DW., Li, HL. Tunneling Radiation of Vector Particles from a Quantum Correction Black Hole. Int J Theor Phys 58, 656–662 (2019). https://doi.org/10.1007/s10773-018-3964-3

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  • DOI: https://doi.org/10.1007/s10773-018-3964-3

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