Thermodynamics of non-linear magnetic-charged AdS black hole surrounded by quintessence, in the background of perfect fluid dark matter

被引:7
|
作者
Ndongmo, Ragil [1 ]
Mahamat, Saleh [2 ,5 ]
Tabi, Conrad Bertrand [3 ]
Bouetou, Thomas Bouetou [1 ,3 ]
Kofane, Timoleon Crepin [1 ,4 ]
机构
[1] Univ Yaounde I, Fac Sci, Dept Phys, PO Box 812, Yaounde, Cameroon
[2] Univ Maroua, Higher Teachers Training Coll, Dept Phys, POB 55, Maroua, Cameroon
[3] Univ Yaounde I, Natl Adv Sch Engn, POB 8390, Yaounde, Cameroon
[4] Botswana Int Univ Sci & Technol, Dept Phys & Astron, Private Mail Bag, Palapye, Botswana
[5] Univ Maroua, Res Ctr Didact Fundamental & Appl Sci, POB 55, Maroua, Cameroon
来源
PHYSICS OF THE DARK UNIVERSE | 2023年 / 42卷
关键词
Black hole; Thermodynamics; Quintessence; Magnetic-charged black hole; Phase transition; PHASE-TRANSITION; SCHWARZSCHILD; ENERGY;
D O I
10.1016/j.dark.2023.101299
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
In this paper, we study the thermodynamic features of a non-linear magnetic-charged AdS black hole surrounded by quintessence, in the background of perfect fluid dark matter(PFDM). After having constructed the corresponding metric, we analyse the structure of the horizon. We find that the existence of inner or outer horizon are constrained by the presence of dark matter. Afterwards, we put out the mass and the temperature of the black hole, in order to get its entropy. Subsequently, we find the expression of the pressure which leads us to get the table of critical values and the isothermal diagram. Especially, we find that the critical values of the temperature and the pressure increase as the dark matter parameter increases. Also, analysing the isothermal diagram, we observe a van der Waals-like behaviour remarked by the presence of a first-order phase transition when we cross the critical temperature. Additionally, we compute and plot the heat capacity and the Hessian matrix of the black hole mass. For the heat capacity, we find that a second-order phase transition occurs, leading the black hole to move from stable phase to unstable one. Furthermore, it comes out that this phase transition point is shifted towards higher values of the horizon radius, as we decrease the dark matter density and increase the quintessence density.
引用
收藏
页数:10
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