Thermodynamic stability and P–V criticality of nonsingular-AdS black holes endowed with clouds of strings

Abstract We investigate the extended phase space thermodynamics of nonsingular-AdS black holes minimally coupled to clouds of strings in which we consider the cosmological constant ( $$\Lambda $$ Λ ) as the pressure (P) of the black holes and its conjugate variable thermodynamical volume (V) of the...

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Main Authors: Ashima Sood, Arun Kumar, J. K. Singh, Sushant G. Ghosh
Format: Article
Language:English
Published: SpringerOpen 2022-03-01
Series:European Physical Journal C: Particles and Fields
Online Access:https://doi.org/10.1140/epjc/s10052-022-10181-8
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author Ashima Sood
Arun Kumar
J. K. Singh
Sushant G. Ghosh
author_facet Ashima Sood
Arun Kumar
J. K. Singh
Sushant G. Ghosh
author_sort Ashima Sood
collection DOAJ
description Abstract We investigate the extended phase space thermodynamics of nonsingular-AdS black holes minimally coupled to clouds of strings in which we consider the cosmological constant ( $$\Lambda $$ Λ ) as the pressure (P) of the black holes and its conjugate variable thermodynamical volume (V) of the black holes. Owing to the background clouds of strings parameter (a), we analyse the Hawking temperature, entropy and specific heat on horizon radius for fixed-parameter k. We find that the strings clouds background does not alter small/large black hole (SBH/LBH) phase transition but occurs at a larger horizon radius, and two second-order phase transitions occur at a smaller horizon radius. Indeed, the G–T plots exhibit a swallowtail below the critical pressure, implying that the first-order phase transition is analogous to the liquid–gas phase transition at a lower temperature and lower critical pressure. To further examine the analogy between nonsingular-AdS black holes and a liquid–gas system, we derive the exact critical points and probe the effects of a cloud of strings on $$P-V$$ P - V criticality to find that the isotherms undergo liquid–gas like phase transition for $${\tilde{T}}\,<\,{\tilde{T}}_c$$ T ~ < T ~ c at lower $${\tilde{T}}_c$$ T ~ c . We have also calculated the critical exponents identical with Van der Walls fluid, i.e., same as those obtained before for arbitrary other AdS black holes, which implies that the background clouds of strings do not change the critical exponents.
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spelling doaj.art-b853257563a14c4f810f03b5a83ae7c62022-12-21T23:51:28ZengSpringerOpenEuropean Physical Journal C: Particles and Fields1434-60441434-60522022-03-0182311110.1140/epjc/s10052-022-10181-8Thermodynamic stability and P–V criticality of nonsingular-AdS black holes endowed with clouds of stringsAshima Sood0Arun Kumar1J. K. Singh2Sushant G. Ghosh3Centre for Theoretical Physics, Jamia Millia IslamiaCentre for Theoretical Physics, Jamia Millia IslamiaDepartment of Mathematics, Netaji Subhas University of TechnologyCentre for Theoretical Physics, Jamia Millia IslamiaAbstract We investigate the extended phase space thermodynamics of nonsingular-AdS black holes minimally coupled to clouds of strings in which we consider the cosmological constant ( $$\Lambda $$ Λ ) as the pressure (P) of the black holes and its conjugate variable thermodynamical volume (V) of the black holes. Owing to the background clouds of strings parameter (a), we analyse the Hawking temperature, entropy and specific heat on horizon radius for fixed-parameter k. We find that the strings clouds background does not alter small/large black hole (SBH/LBH) phase transition but occurs at a larger horizon radius, and two second-order phase transitions occur at a smaller horizon radius. Indeed, the G–T plots exhibit a swallowtail below the critical pressure, implying that the first-order phase transition is analogous to the liquid–gas phase transition at a lower temperature and lower critical pressure. To further examine the analogy between nonsingular-AdS black holes and a liquid–gas system, we derive the exact critical points and probe the effects of a cloud of strings on $$P-V$$ P - V criticality to find that the isotherms undergo liquid–gas like phase transition for $${\tilde{T}}\,<\,{\tilde{T}}_c$$ T ~ < T ~ c at lower $${\tilde{T}}_c$$ T ~ c . We have also calculated the critical exponents identical with Van der Walls fluid, i.e., same as those obtained before for arbitrary other AdS black holes, which implies that the background clouds of strings do not change the critical exponents.https://doi.org/10.1140/epjc/s10052-022-10181-8
spellingShingle Ashima Sood
Arun Kumar
J. K. Singh
Sushant G. Ghosh
Thermodynamic stability and P–V criticality of nonsingular-AdS black holes endowed with clouds of strings
European Physical Journal C: Particles and Fields
title Thermodynamic stability and P–V criticality of nonsingular-AdS black holes endowed with clouds of strings
title_full Thermodynamic stability and P–V criticality of nonsingular-AdS black holes endowed with clouds of strings
title_fullStr Thermodynamic stability and P–V criticality of nonsingular-AdS black holes endowed with clouds of strings
title_full_unstemmed Thermodynamic stability and P–V criticality of nonsingular-AdS black holes endowed with clouds of strings
title_short Thermodynamic stability and P–V criticality of nonsingular-AdS black holes endowed with clouds of strings
title_sort thermodynamic stability and p v criticality of nonsingular ads black holes endowed with clouds of strings
url https://doi.org/10.1140/epjc/s10052-022-10181-8
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AT sushantgghosh thermodynamicstabilityandpvcriticalityofnonsingularadsblackholesendowedwithcloudsofstrings