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Thermodynamics evaluation in Einstein–Gauss–Bonnet gravity like black holes

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Abstract

From D-dimensional black holes, we investigate the Hawking radiation of charged boson particles from charged black holes without and with quantum gravity. We apply the field equation and WKB approximation to solve the Einstein–Gauss–Bonnet gravity like spacetime and obtain the tunneling radiation from charged black holes using complex path integration. We also calculate the temperature of the radiation from these black holes using the tunneling probability of outgoing particles without and with the influence of quantum gravity. We also look into the entropy and heat capacity of well-known thermodynamic properties for the geometry under consideration. It is concluded that the D dimension like black holes is stable or unstable under Einstein–Gauss–Bonnet gravity.

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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 Science and Technology, Echahid Cheikh Larbi Tebessi University, Tebessa, Algeria

    Houcine Aounallah

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

    Rimsha Babar

Authors
  1. Riasat Ali
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  2. Xia Tiecheng
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  3. Houcine Aounallah
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  4. Rimsha Babar
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Correspondence to Xia Tiecheng.

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Ali, R., Tiecheng, X., Aounallah, H. et al. Thermodynamics evaluation in Einstein–Gauss–Bonnet gravity like black holes. Indian J Phys (2024). https://doi.org/10.1007/s12648-024-03122-6

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