Abstract
In this work, the thermodynamics of the Bardeen black hole with quintessence matter associated with dark energy in the context of the extended generalized uncertainty principle is investigated. The corrections to the Hawking temperature, heat capacity, and entropy are obtained via a heuristic method. These modifications show that the modified uncertainty principles and normalization factor will restrict the lower bound value of horizon radius to affect the Hawking temperature, the remnant temperature and mass do not depend on the extended uncertainty principle parameter and the quintessence matter will not affect the entropy of the Bardeen black hole. In addition, the equation of state associated with the pressure and the volume are examined.
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This manuscript has associated data in a data repository. [Authors’ comment: All data included in this manuscript are available upon reasonable request by contacting with the corresponding author.]
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Acknowledgements
The authors are grateful to anonymous reviewers for their very crucial and detailed comments. This research was funded by the Guizhou Scientific Foundation-ZK[2022] General 491 and the National Natural Science Foundation of China (Grant No.11465006).
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Wu, S., Wang, BQ., Chen, H. et al. EGUP-corrected Bardeen black hole thermodynamics with quintessence matter. Eur. Phys. J. Plus 137, 970 (2022). https://doi.org/10.1140/epjp/s13360-022-03163-y
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DOI: https://doi.org/10.1140/epjp/s13360-022-03163-y