Restricted Phase Space Thermodynamics of Nonlinear Electrodynamics-Anti-de Sitter Black Holes
We study the Restricted Phase Space Thermodynamics (RPST) of magnetically charged anti-de Sitter (AdS) black holes sourced by nonlinear electrodynamics (NED). The first law and the corresponding Euler relation are examined using the scaling properties. While the mass is homogeneous in the first orde...
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| Published in | Progress of theoretical and experimental physics Vol. 2024; no. 11 |
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| Main Authors | , |
| Format | Journal Article |
| Language | English |
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Oxford University Press
01.11.2024
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| ISSN | 2050-3911 2050-3911 |
| DOI | 10.1093/ptep/ptae154 |
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| Abstract | We study the Restricted Phase Space Thermodynamics (RPST) of magnetically charged anti-de Sitter (AdS) black holes sourced by nonlinear electrodynamics (NED). The first law and the corresponding Euler relation are examined using the scaling properties. While the mass is homogeneous in the first order, the intensive variables are observed to follow zeroth-order homogeneity. We use numerical and graphical techniques to find the critical points of the various thermodynamic quantities. By utilizing the rescaling properties of the equation of states, we study the thermodynamic processes using different pairs of variables. From our analysis, we infer that although the RPST of the NED-AdS black hole resembles those of Reissner–Nordström-AdS, Kerr-AdS, and Kerr–Sen-AdS black holes in most of its aspects, hinting at a possible universality, there exists one particular $\mu -C$ process that differs in its behavior from its counterparts in earlier reported works. |
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| AbstractList | We study the Restricted Phase Space Thermodynamics (RPST) of magnetically charged anti-de Sitter (AdS) black holes sourced by nonlinear electrodynamics (NED). The first law and the corresponding Euler relation are examined using the scaling properties. While the mass is homogeneous in the first order, the intensive variables are observed to follow zeroth-order homogeneity. We use numerical and graphical techniques to find the critical points of the various thermodynamic quantities. By utilizing the rescaling properties of the equation of states, we study the thermodynamic processes using different pairs of variables. From our analysis, we infer that although the RPST of the NED-AdS black hole resembles those of Reissner–Nordström-AdS, Kerr-AdS, and Kerr–Sen-AdS black holes in most of its aspects, hinting at a possible universality, there exists one particular $\mu -C$ process that differs in its behavior from its counterparts in earlier reported works. We study the Restricted Phase Space Thermodynamics (RPST) of magnetically charged anti-de Sitter (AdS) black holes sourced by nonlinear electrodynamics (NED). The first law and the corresponding Euler relation are examined using the scaling properties. While the mass is homogeneous in the first order, the intensive variables are observed to follow zeroth-order homogeneity. We use numerical and graphical techniques to find the critical points of the various thermodynamic quantities. By utilizing the rescaling properties of the equation of states, we study the thermodynamic processes using different pairs of variables. From our analysis, we infer that although the RPST of the NED-AdS black hole resembles those of Reissner–Nordström-AdS, Kerr-AdS, and Kerr–Sen-AdS black holes in most of its aspects, hinting at a possible universality, there exists one particular $\mu -C$ process that differs in its behavior from its counterparts in earlier reported works. |
| Author | Phukon, Prabwal Awal, Mozib Bin |
| Author_xml | – sequence: 1 givenname: Mozib Bin orcidid: 0009-0007-8797-667X surname: Awal fullname: Awal, Mozib Bin email: mozibawal@gmail.com – sequence: 2 givenname: Prabwal orcidid: 0000-0002-4465-7974 surname: Phukon fullname: Phukon, Prabwal email: prabwal@dibru.ac.in |
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| Cites_doi | 10.1007/JHEP12(2015)073 10.1103/PhysRevD.96.124018 10.1155/2017/3819246 10.1088/1674-1137/ace9c2 10.1142/S0218271817501516 10.1007/JHEP04(2016)142 10.1016/j.nuclphysb.2022.115949 10.1088/0264-9381/22/9/002 10.12942/lrr-1999-2 10.1103/PhysRevD.63.044005 10.3390/e24081131 10.1016/j.physletb.2014.07.019 10.1016/j.nuclphysb.2023.116184 10.1007/BF02345020 10.1007/JHEP07(2012)033 10.1140/epjc/s10052-014-2970-8 10.1103/PhysRevLett.127.091301 10.1103/PhysRevD.7.2333 10.1016/j.dark.2023.101261 10.1103/PhysRevD.15.2752 10.1103/PhysRevD.91.044028 10.1007/s10714-022-03024-0 10.1140/epjc/s10052-017-4937-z 10.1088/0264-9381/28/23/235017 10.1016/j.physletb.2016.12.004 10.1088/0264-9381/26/19/195011 10.1140/epjc/s10052-022-10080-y 10.1103/PhysRevD.84.127503 10.1103/PhysRevLett.26.1344 10.1007/BF01645742 10.1103/PhysRevD.105.106014 10.1016/j.physletb.2024.138801 10.1007/JHEP09(2013)005 10.1088/0264-9381/31/20/205002 10.1103/PhysRevD.60.064018 10.1103/RevModPhys.83.793 10.4310/ATMP.1998.v2.n2.a1 10.1088/1361-6382/ac566c 10.1103/PhysRevD.105.024058 10.1088/0264-9381/28/12/125020 10.1088/1361-6382/aa5c69 10.1103/PhysRevD.108.044045 10.3390/e25040687 10.1007/BF01208266 10.1016/j.aop.2023.169569 10.1007/JHEP11(2014)120 |
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