Thermodynamic behavior and phase transitions of black holes with a cloud of strings and perfect fluid dark matter

This paper presents an exact black hole solution within a cloud of strings (CoS) and a perfect fluid dark matter (PFDM) field. The derived black hole solution interpolates between the AdS-charged Letelier black hole in the absence of the PFDM field and the AdS Reissner-Nordström black hole in the limiting case of the PFDM and CoS parameters. The thermodynamic properties of the black hole, including temperature, entropy, heat, and free energy, are modified in the presence of the PFDM field and CoS parameter. Furthermore, we investigate the black hole's critical points and phase structure in an extended phase space. We find that the critical temperature and pressure decrease with the CoS parameter but increase with the PFDM field. The Gibbs free energy versus temperature plot reveals a swallow-tail behavior, indicating a first-order phase transition, which terminates at a second-order phase transition.

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Publication Details

Journal
Nuclear Physics B
Published
2025-04-23
DOI
https://doi.org/10.1016/j.nuclphysb.2025.116915
Citations
5
Primary Topic
Black Holes and Theoretical Physics
Type
article
Field-Weighted Citation Impact
9.35

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Thermodynamic behavior and phase transitions of black holes with a cloud of strings and perfect fluid dark matter

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article

Thermodynamic behavior and phase transitions of black holes with a cloud of strings and perfect fluid dark matter

Dharm Veer Singh, Kairat Myrzakulov, Manish Kumar, Yerlan Myrzakulov, Sudhaker Upadhyay, Bhupendra Singh
article en
5 citations

Abstract

This paper presents an exact black hole solution within a cloud of strings (CoS) and a perfect fluid dark matter (PFDM) field. The derived black hole solution interpolates between the AdS-charged Letelier black hole in the absence of the PFDM field and the AdS Reissner-Nordström black hole in the limiting case of the PFDM and CoS parameters. The thermodynamic properties of the black hole, including temperature, entropy, heat, and free energy, are modified in the presence of the PFDM field and CoS parameter. Furthermore, we investigate the black hole's critical points and phase structure in an extended phase space. We find that the critical temperature and pressure decrease with the CoS parameter but increase with the PFDM field. The Gibbs free energy versus temperature plot reveals a swallow-tail behavior, indicating a first-order phase transition, which terminates at a second-order phase transition.

Nuclear Physics BVol. 1016
Department of Science and Technology, Ministry of Science and Technology, India, Ministry of Education and Science of the Republic of Kazakhstan
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Openalex Percentile: Top 3%
Black Holes and Theoretical Physics
9.35
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