Study of thermodynamics for Dymnikova regular black hole under the influence of quantum gravity

In this article, we examine the corrected Hawking temperature for Dymnikova regular black hole (DRBH) under the influence of quantum gravity. In linear thermodynamics, we follow the semi-classical phenomenon, Wentzel-Kramers-Brillouin (WKB) approximation and Lagrangian equation in the background of...

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Bibliographic Details
Published inIndian journal of physics Vol. 97; no. 10; pp. 3155 - 3166
Main Authors Babar, Rimsha, Akhtar, Z., Asgher, Muhammad, Ali, Riasat
Format Journal Article
LanguageEnglish
Published New Delhi Springer India 01.09.2023
Springer Nature B.V
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Summary:In this article, we examine the corrected Hawking temperature for Dymnikova regular black hole (DRBH) under the influence of quantum gravity. In linear thermodynamics, we follow the semi-classical phenomenon, Wentzel-Kramers-Brillouin (WKB) approximation and Lagrangian equation in the background of generalized uncertainty principle (GUP). In order to check the gravitational effects on the corresponding black hole geometry, we examine the graphical interpretation of the corrected Hawking temperature versus horizon in the presence of gravity parameter β . We graphically examine the physical state of corresponding black hole under the influence of electric charge and quantum gravity parameter. Moreover, using graphical analysis, we examine the thermal fluctuations effects and thermodynamics logarithmic corrections on the entropy, Hawking temperature, heat capacity, internal energy, specific heat, enthalpy, Helmholtz free energy, pressure and Gibbs free energy.
ISSN:0973-1458
0974-9845
DOI:10.1007/s12648-023-02668-1