Leading-order corrections to the thermodynamics of Rindler modified Schwarzschild black hole

Mandal, Surajit; Das, Surajit; Gogoi, Dhruba Jyoti; Pramanik, Ananda

doi:10.1016/j.dark.2023.101349

Cited by 5 publications

(1 citation statement)

References 67 publications

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“…In equation (8), M is an integral constant related to the mass (AdM mass) of the Rindler-Schwarzschild black hole [45], and a is Rindler coupling parameter [43]. It is obvious that the considered spacetime transforms [45] into the well-known Schwarzschild BH for a = 0 = Λ. This study examines the geodesic evaluation of Grumiller's metric, which measures gravity over extended distances.…”

Section: Introductory Review Of the Rindler-schwarzschild Black Holementioning

confidence: 99%

Thermal analysis of the Rindler–Schwarzschild black hole via corrected entropy

Ditta,

Tiecheng,

Ali

et al. 2024

Commun. Theor. Phys.

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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.

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Section: Introductory Review Of the Rindler-schwarzschild Black Holementioning

confidence: 99%

Thermal analysis of the Rindler–Schwarzschild black hole via corrected entropy

Ditta,

Tiecheng,

Ali

et al. 2024

Commun. Theor. Phys.

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Weak deflection angle, Hawking radiation, greybody bound and shadow cast for static black hole in the framework of f(R) gravity

Mandal

2023

Physics of the Dark Universe

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Corrected thermodynamics and stability of magnetic charged AdS black holes surrounded by quintessence

Gogoi,

Sekhmani,

Bora

et al. 2024

J. Cosmol. Astropart. Phys.

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In this study, we explore the corrected thermodynamics of non-linear magnetic charged anti-de Sitter (AdS) black holes surrounded by quintessence, incorporating thermal fluctuations and deriving the corrected thermodynamic potentials. We analyze the effects of corrections due to thermal fluctuations on various thermodynamic potentials, including enthalpy, Helmholtz free energy, and Gibbs free energy. Our results show significant impacts on smaller black holes, with first-order corrections destabilizing them, while second-order corrections enhance stability with increasing parameter values. The specific heat analysis further elucidates the stability criteria, indicating that the large black holes ensure stability against phase transitions. However, the thermal fluctuations do not affect the physical limitation points as well as the second-order phase transition points of the black hole. Our findings highlight the intricate role of thermal fluctuations in black hole thermodynamics and their influence on stability, providing deeper insights into the behaviour of black holes under corrected thermodynamic conditions.

show abstract

Leading-order corrections to the thermodynamics of Rindler modified Schwarzschild black hole

Cited by 5 publications

References 67 publications

Thermal analysis of the Rindler–Schwarzschild black hole via corrected entropy

Thermal analysis of the Rindler–Schwarzschild black hole via corrected entropy

Weak deflection angle, Hawking radiation, greybody bound and shadow cast for static black hole in the framework of f(R) gravity

Corrected thermodynamics and stability of magnetic charged AdS black holes surrounded by quintessence

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