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Study on the Influence of Lorentz Dispersion Relation on Fermions Tunneling Radiation of Kerr-TAUB-NUT Black Hole

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Abstract

In this paper, by applying the correction of Lorentz dispersion relation, the fermion tunneling radiation of the stationary axisymmetric Kerr-TAUB-NUT black hole in curved space-time is studied. Based on the modified Lorentz dispersion relation, the revised Rarita-Schwinger equation has been obtained. Then, we get the dynamic equation of fermions via semi-classical theory, which is the modified Hamilton-Jacobi equation. So at the event horizon the tunneling radiation in the space-time of stationary axisymmetric Kerr-TAUB-NUT black hole has been effectively investigated. At last, the modified tunneling radiation and Hawking temperature have been obtained in the same space-time.

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Acknowledgements

The authors would like to thank the anonymous reviewers for their helpful comments and suggestions, which helped to improve the quality of this paper. This work was supported by the National Natural Science Foundation of China (Grant No. 11573022).

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Authors and Affiliations

  1. School of sciences, Southwest Petroleum University, Chengdu, 610500, China

    Tin-Ping Liu & Qun-Chao Ding

  2. Physics and Space Science College, China West Normal University, Nanchong, 637009, China

    Shu-Zheng Yang

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  1. Tin-Ping Liu
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  2. Qun-Chao Ding
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  3. Shu-Zheng Yang
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Correspondence to Tin-Ping Liu.

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Liu, TP., Ding, QC. & Yang, SZ. Study on the Influence of Lorentz Dispersion Relation on Fermions Tunneling Radiation of Kerr-TAUB-NUT Black Hole. Int J Theor Phys 59, 3015–3022 (2020). https://doi.org/10.1007/s10773-020-04461-w

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  • DOI: https://doi.org/10.1007/s10773-020-04461-w

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