Hayward–Letelier Black Holes in AdS Spacetime

We analyze Hayward black holes (BHs) with a negative cosmological constant surrounded by a cloud of strings, which we designate Hayward–Letelier AdS BHs. These solutions can be obtained by coupling the Einstein equations with nonlinear electrodynamics and the energy–momentum tensor of clouds of strings. We show that these solutions are no longer regular and have a curvature singularity at the center. In turn, we analyze the thermodynamics associated with these BHs by establishing the form of the Smarr formula and the first law of thermodynamics. We derive the expressions for the thermodynamic quantities such as pressure, temperature, heat capacity, Gibbs free energy, and isothermal compressibility. We explore the phase structure of these solutions by analyzing the behavior of the heat capacity and Gibbs free energy. These solutions exhibit a first-order phase transition, similar to van der Waals fluids. We also check the behavior of the thermodynamic quantities near the critical points and calculate the values of the critical exponents. This illustrates a robust analogy between our solutions and van der Waals fluids.

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Publication Details

Journal
Particles
Published
2024-11-20
DOI
https://doi.org/10.3390/particles7040062
Citations
5
Primary Topic
Black Holes and Theoretical Physics
Type
article
Field-Weighted Citation Impact
3.30
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article

Hayward–Letelier Black Holes in AdS Spacetime

Sushant G. Ghosh, Arun Kumar, Aroonkumar Beesham, Ashima Sood
5 citations
Particles
Black Holes and Theoretical Physics
3.30
article

Hayward–Letelier Black Holes in AdS Spacetime

Sushant G. Ghosh, Arun Kumar, Aroonkumar Beesham, Ashima Sood
article en
5 citations

Abstract

We analyze Hayward black holes (BHs) with a negative cosmological constant surrounded by a cloud of strings, which we designate Hayward–Letelier AdS BHs. These solutions can be obtained by coupling the Einstein equations with nonlinear electrodynamics and the energy–momentum tensor of clouds of strings. We show that these solutions are no longer regular and have a curvature singularity at the center. In turn, we analyze the thermodynamics associated with these BHs by establishing the form of the Smarr formula and the first law of thermodynamics. We derive the expressions for the thermodynamic quantities such as pressure, temperature, heat capacity, Gibbs free energy, and isothermal compressibility. We explore the phase structure of these solutions by analyzing the behavior of the heat capacity and Gibbs free energy. These solutions exhibit a first-order phase transition, similar to van der Waals fluids. We also check the behavior of the thermodynamic quantities near the critical points and calculate the values of the critical exponents. This illustrates a robust analogy between our solutions and van der Waals fluids.

ParticlesVol. 7(4)
University of Zululand (ZA), Mangosuthu University of Technology (ZA), Netaji Subhas University of Technology (IN), Zhejiang University of Technology (CN), Jamia Millia Islamia (IN), University of KwaZulu-Natal (ZA)
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Openalex Percentile: Top 6%
Black Holes and Theoretical Physics
3.30
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Hayward–Letelier Black Holes in AdS Spacetime — Sushant G. Ghosh, Arun Kumar, et al. · Particles (2024) | TGRS Research Map | TGRS