首页|Thermal analysis of the Rindler-Schwarzschild black hole via corrected entropy
Thermal analysis of the Rindler-Schwarzschild black hole via corrected entropy
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In this study,we investigate the thermodynamic characteristics of the Rindler-Schwarzschild black hole solution.Our analysis encompasses the examination of energy emission,Gibbs free energy,and thermal fluctuations.We calculate various quantities such as the Hawking temperature,geometric mass,and heat capacity to assess the local and global thermodynamic stability.The temperature of the black hole is determined using the first law of thermodynamics,while the energy emission rate is evaluated as well.By computing the Gibbs free energy,we explore the phase transition behavior exhibited by Rindler-Schwarzschild black hole,specifically examining the swallowing tails.Moreover,we derive the corrected entropy to investigate the influence of thermal fluctuations on small and large black holes.Notably,we compare the impact of correction terms on the thermodynamic system by comparing the results obtained for large black holes and small black holes.
black holesthermodynamicsthermal fluctuationsheat capacityGibbs free energyenergy emissionRindler-Schwarzschild black hole
Allah Ditta、Xia Tiecheng、Riasat Ali、Ali Övgün
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Department of Mathematics,Shanghai University and Newtouch Center for Mathematics of Shanghai University,Shanghai 200444,China
Physics Department,Eastern Mediterranean University,Famagusta,99628 North Cyprus,via Mersin 10,Turkiye
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