Corrected thermodynamics and stability of magnetic charged AdS black holes surrounded by quintessence

被引:2
作者
Gogoi, Dhruba Jyoti [1 ,2 ]
Sekhmani, Yassine [3 ,11 ]
Bora, Shyamalee [4 ]
Rayimbaev, Javlon [5 ,6 ,7 ,8 ,12 ]
Bora, Jyatsnasree [9 ]
Myrzakulov, Ratbay [10 ,13 ]
机构
[1] Moran Coll, Dept Phys, Charaideo 785670, Assam, India
[2] Dibrugarh Univ, Ctr Atmospher Studies, Theoret Phys Div, Dibrugarh 786004, Assam, India
[3] Khazar Univ, Ctr Theoret Phys, 41 Mehseti St, AZ-1096 Baku, Azerbaijan
[4] Tezpur Univ, Dept Phys, Tezpur 784028, Assam, India
[5] Natl Res Univ TIIAME, Inst Fundamental & Appl Res, Kori Niyoziy 39, Tashkent 100000, Uzbekistan
[6] Univ Tashkent Appl Sci, Gavhar str 1, Tashkent 100149, Uzbekistan
[7] Urgench State Univ, Kh Alimdjan Str 14, Urgench 220100, Uzbekistan
[8] Shahrisabz State Pedag Inst, Shahrisabz Str 10, Shahrisabz 181301, Uzbekistan
[9] DHSK Coll, Dept Phys, Dibrugarh 786001, Assam, India
[10] LN Gumilyov Eurasian Natl Univ, Astana 010008, Kazakhstan
[11] Chitkara Univ, Inst Engn Technol, Ctr Res Impact & Outcome, Rajpura 140401, Punjab, India
[12] Tashkent State Tech Univ, Tashkent 100095, Uzbekistan
[13] Ratbay Myrzakulov Eurasian Int Ctr Theoret Phys, Astana 010009, Kazakhstan
来源
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS | 2024年 / 11期
关键词
Exact solutions; black holes and black hole thermodynamics in GR and beyond; quantum black holes; GR black holes; modified gravity; FLUCTUATIONS; STATISTICS; ENTROPY;
D O I
10.1088/1475-7516/2024/11/019
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
In this study, we explore the corrected thermodynamics of non-linear magnetic charged anti-de Sitter (AdS) black holes surrounded by quintessence, incorporating thermal fluctuations and deriving the corrected thermodynamic potentials. We analyze the effects of corrections due to thermal fluctuations on various thermodynamic potentials, including enthalpy, Helmholtz free energy, and Gibbs free energy. Our results show significant impacts on smaller black holes, with first-order corrections destabilizing them, while second-order corrections enhance stability with increasing parameter values. The specific heat analysis further elucidates the stability criteria, indicating that the large black holes ensure stability against phase transitions. However, the thermal fluctuations do not affect the physical limitation points as well as the second-order phase transition points of the black hole. Our findings highlight the intricate role of thermal fluctuations in black hole thermodynamics and their influence on stability, providing deeper insights into the behaviour of black holes under corrected thermodynamic conditions.
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页数:29
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