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Gravitational Analysis of Rotating Charged Black‐Hole‐Like Solution in Einstein–Gauss–Bonnet Gravity

Riasat AliDepartment of Mathematics GC University Faisalabad Layyah Campus Layyah 31200 PakistanRimsha BabarDivision of Science and Technology University of Education Township Lahore 54590 PakistanMuhammad AsgherDepartment of Mathematics The Islamia University of Bahawalpur Bahawalpur 63100 Pakistan
2022en
ABI

Аннотация

Abstract This work analyzes the Einstein–Gauss–Bonnet gravity of charged black hole solutions through Newman–Janis approach. The Hawking temperature for corresponding black hole is also computed. The solution depends upon rotation parameter a , black hole mass, charge and horizon. Moreover, the graphical behavior of temperature via event horizon to analyze the stability of black hole under the effects of rotation parameter is discussed. The graphs are plotted in the presence/absence of rotation parameter and charge. Furthermore, the Hawking temperature under gravity effects is studied by using the semi‐classical method. It is also observed that the maximum temperature at non‐zero horizon depicts the BH remnant. Finally, the logarithmic corrected entropy for given black hole is computed and the logarithmic corrected entropy under effects of rotation and correction parameter are studied.

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Цитирований: 3Использованных источников: 0