Three-dimensional accelerating AdS black holes in F(R) gravity

Panah, B. Eslam; Khorasani, M.; Sedaghat, J.

doi:10.1140/epjp/s13360-023-04339-w

Eur. Phys. J. Plus

2023

DOI: 10.1140/epjp/s13360-023-04339-w

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Three-dimensional accelerating AdS black holes in F(R) gravity

B. Eslam Panah,

M. Khorasani,

J. Sedaghat

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2024

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Cited by 5 publications

(1 citation statement)

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“…For 3D C-metrics not in the pure Einstein gravity see[43,44] 3. We used the standard convention in AdS/BCFT[46,47], the brane tension here is 4πGN times the one defined in[45].…”

mentioning

confidence: 99%

Aspects of three-dimensional C-metric

Tian,

Lai

2024

J. High Energ. Phys.

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In this work, we present an extensive analysis of the thermodynamics and holographic properties of three-dimensional C-metrics in the FG gauge, where we find that the free energy is equal to the Euclidean on-shell action with a generic conformal factor. For the black hole solutions we find that Smarr relation and the first law of thermodynamics can be formulated when the contributions of the boundary entropy are considered. We also compute holographic entanglement entropy following the AdS/BCFT formalism. By comparing the free energies of different bulk solutions with a fixed flat torus boundary geometry, we find that a specific type of accelerating black hole is dominant in the high temperature regime.

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“…For 3D C-metrics not in the pure Einstein gravity see[43,44] 3. We used the standard convention in AdS/BCFT[46,47], the brane tension here is 4πGN times the one defined in[45].…”

mentioning

confidence: 99%

Aspects of three-dimensional C-metric

Tian,

Lai

2024

J. High Energ. Phys.

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Thermodynamic Topology of Topological Black Hole in F(R)-ModMax Gravity’s Rainbow

Eslam Panah,

Hazarika,

Phukon

2024

Progress of Theoretical and Experimental Physics

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In order to include the effect of high energy and topological parameters on black holes in F(R) gravity, we consider two corrections to this gravity: energy-dependent spacetime with different topological constants, and a nonlinear electrodynamics field. In other words, we combine F(R) gravity’s rainbow with ModMax nonlinear electrodynamics theory to see the effects of high energy and topological parameters on the physics of black holes. For this purpose, we first extract topological black hole solutions in F(R) -ModMax gravity’s rainbow. Then, by considering black holes as thermodynamic systems, we obtain thermodynamic quantities and check the first law of thermodynamics. The effect of the topological parameter on the Hawking temperature and the total mass of black holes is obvious. We also discuss the thermodynamic topology of topological black holes in F(R)-ModMax gravity’s rainbow using the off-shell free energy method. In this formalism, black holes are assumed to be equivalent to defects in their thermodynamic spaces. For our analysis, we consider two different types of thermodynamic ensembles. These are: fixed q ensemble and fixed φ ensemble. We take into account all the different types of curvature hypersurfaces that can be constructed in these black holes. The local and global topology of these black holes are studied by computing the topological charges at the defects in their thermodynamic spaces. Finally, in accordance with their topological charges, we classify the black holes into three topological classes with total winding numbers corresponding to −1, 0, and 1. We observe that the topological classes of these black holes are dependent on the value of the rainbow function, the sign of the scalar curvature, and the choice of ensembles.

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Analytic three-dimensional primary hair charged black holes with Coulomb-like electrodynamics and their thermodynamics

Daripa,

Mahapatra

2024

Phys. Rev. D

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Three-dimensional accelerating AdS black holes in F(R) gravity

Cited by 5 publications

References 86 publications

Aspects of three-dimensional C-metric

Aspects of three-dimensional C-metric

Thermodynamic Topology of Topological Black Hole in F(R)-ModMax Gravity’s Rainbow

Analytic three-dimensional primary hair charged black holes with Coulomb-like electrodynamics and their thermodynamics

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