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Thermodynamic Phase Transition of Black Hole

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Abstract

In the thermodynamic evolution of black holes, the generalized uncertainty principle and quantum tunneling effect prevent the complete evaporation of black holes and produce remnants, and thermodynamic phase transition occurs during evaporation. Based on the generalized uncertainty principle and the method of quantum tunneling, we study the phase transition of the quantum–corrected black hole. Using the modified Hamiltonian–Jacobi equation to analyze the corrected thermodynamic quantity, we find that the thermodynamic phase transition of the black hole is not only depending on the nature of the black hole itself, it also depends on quantum parameter ξ, generalized uncertainty parameter β and parameter λ.

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Acknowledgements

This work is supported in part by the National Natural Science Foundation of China (Grant No. 11703018), Natural Science Foundation of Liaoning Province, China (Grant No. 20180550275) and Doctoral Scientific Research Foundation of Shenyang Normal University (Grant No. BS201843).

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

    Hui-Ling Li & Wei Li

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  1. Hui-Ling Li
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  2. Wei Li
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Correspondence to Hui-Ling Li.

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Li, HL., Li, W. Thermodynamic Phase Transition of Black Hole. Int J Theor Phys 59, 3032–3042 (2020). https://doi.org/10.1007/s10773-020-04510-4

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