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First-order quantum corrections of tunneling radiation in modified Schwarzschild–Rindler black hole

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Abstract

In this work, we study the first order corrections of Hawking temperature and entropy for modified Schwarzschild–Rindler black hole. To do so, we use the modified Lagrangian equation for vector particles in the background of quantum correction parameter \(\delta \). We examine the graphical interpretation of the corrected Hawking temperature with respect to horizon under the effects of correction parameter in order to verify the gravitational effects on the geometry of the modified Schwarzschild–Rindler black hole. We perform a graphic analysis of the modified Schwarzschild–Rindler black hole’s physical state as a function of the mass and Rindler acceleration under the effects of correction parameter. Moreover, we derive the corrected entropy and study the effects of mass and Rindler acceleration parameter on entropy under different variations of correction parameter.

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Data Availibility Statement

The data that support the findings of this study are available from the corresponding author upon reasonable request.

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Acknowledgements

The paper was funded by the National Natural Science Foundation of China 11975145.

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Authors and Affiliations

  1. Department of Mathematics, Shanghai University and Newtouch Center for Mathematics of Shanghai University, Shanghai, 200444, People’s Republic of China

    Riasat Ali & Xia Tiecheng

  2. Department of Mathematics, GC University Faisalabad Layyah Campus, Layyah, 31200, Pakistan

    Rimsha Babar

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  1. Riasat Ali
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  2. Xia Tiecheng
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Correspondence to Xia Tiecheng.

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Ali, R., Tiecheng, X. & Babar, R. First-order quantum corrections of tunneling radiation in modified Schwarzschild–Rindler black hole. Gen Relativ Gravit 56, 13 (2024). https://doi.org/10.1007/s10714-024-03206-y

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