Energy‐Dependent Topological Black Holes in Massive Gravity Coupled to Double‐Logarithmic Electrodynamics

Ali, Askar

doi:10.1002/andp.202200224

Cited by 3 publications

(1 citation statement)

References 171 publications

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“…In Refs. [27][28][29][30][31][32][33][34][35][36][37][38][39][40], different black holes of the massive gravity and their physical properties have recently been examined. Among these, the anti-de Sitter black holes play a significant role in various usages of gauge/gravity duality [10] and black hole chemistry [41].…”

Section: Introductionmentioning

confidence: 99%

Thermodynamics and Logarithmic Corrections of Symmergent Black Holes

Ali¹,

Babar²,

Akhtar³

et al. 2023

Preprint

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In this paper, we study quantum gravity effect on the symmergent black hole which is derived from quadratic-curvature gravity. To do so, we use the Klein-Gordon equation which is modified by generalized uncertainty principle (GUP). After solving the field equations, we examine the symmergent black hole's tunneling and Hawking temperature. We explore the graphs of the temperature through the outer horizon to check the GUP influenced conditions of symmergent black hole stability. We also explain how symmergent black holes behave physically when influenced by quantum gravity. The impacts of thermal fluctuations on the thermodynamics of a symmergent black holes spacetime are examined. We first evaluate the model under consideration's thermodynamic properties, such as its Hawking temperature, angular velocity, entropy, and electric potential. We evaluate the logarithmic correction terms for entropy around the equilibrium state in order to examine the impacts of thermal fluctuations. In the presence of these correction terms, we also examine the viability of the first law of thermodynamics. Finally, we evaluate the system's stability using the Hessian matrix and heat capacity. It is determined that a stable model is generated by logarithmic corrections arising from thermal fluctuations.

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Section: Introductionmentioning

confidence: 99%

Thermodynamics and Logarithmic Corrections of Symmergent Black Holes

Ali¹,

Babar²,

Akhtar³

et al. 2023

Preprint

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show abstract

Modified FRW cosmology with massive gravity in the spectrum of the rainbow

Naeem,

Bibi

2024

Gen Relativ Gravit

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Topological dyonic black holes of massive gravity with generalized quasitopological electromagnetism

Ali,

Övgün

2024

Eur. Phys. J. C

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In this paper we investigate new dyonic black holes of massive gravity sourced by generalized quasitopological electromagnetism in arbitrary dimensions. We begin by deriving the exact solution to the field equations defining these black holes and look at how graviton’s mass, dimensionality parameter, and quasitopological electromagnetic field affect the horizon structure of anti-de Sitter dyonic black holes. We also explore the asymptotic behaviour of the curvature invariants at both the origin and infinity to analyze the geometric structure of the resultant black holes. We also compute the conserved and thermodynamic quantities of these dyonic black holes with the help of established techniques and known formulas. After investigating the relevancy of first law, we look at how various parameters influence the local thermodynamic stability of resultant black hole solution. We also examine how thermal fluctuations affect the local stability of dyonic black holes in massive gravity. Finally, we study the shadow cast of the black hole.

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Energy‐Dependent Topological Black Holes in Massive Gravity Coupled to Double‐Logarithmic Electrodynamics

Cited by 3 publications

References 171 publications

Thermodynamics and Logarithmic Corrections of Symmergent Black Holes

Thermodynamics and Logarithmic Corrections of Symmergent Black Holes

Modified FRW cosmology with massive gravity in the spectrum of the rainbow

Topological dyonic black holes of massive gravity with generalized quasitopological electromagnetism

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