Photon orbits and phase transition for Letelier AdS black holes immersed in perfect fluid dark matter

被引:6
|
作者
Sood, Ashima [1 ,2 ]
Ali, Md Sabir [3 ,4 ,5 ,6 ,7 ]
Singh, J. K. [1 ]
Ghosh, Sushant G. [2 ,8 ]
机构
[1] Netaji Subhas Univ Technol, Dept Math, New Delhi 110078, India
[2] Jamia Millia Islamia, Ctr Theoret Phys, New Delhi 110025, India
[3] Mahishadal Raj Coll, Dept Phys, Purba Medinipur 721628, W Bengal, India
[4] Lanzhou Univ, Inst Theoret Phys & Res Ctr Gravitat, Lanzhou 730000, Peoples R China
[5] Lanzhou Univ, Key Lab Quantum Theory & Applicat, MoE, Lanzhou 730000, Peoples R China
[6] Lanzhou Univ, Lanzhou Ctr Theoret Phys, Lanzhou 730000, Peoples R China
[7] Lanzhou Univ, Key Lab Theoret Phys Gansu Prov, Lanzhou 730000, Peoples R China
[8] Univ KwaZulu Natal, Sch Math Stat & Comp Sci, Astrophys & Cosmol Res Unit, Private Bag X54001, ZA-4000 Durban, South Africa
基金
中国国家自然科学基金;
关键词
AdS black holes; perfect fluid dark matter; Letelier spacetime; photon orbit; extended phase space thermodynamics; correlation of photon orbit and thermodynamics; QUASI-NORMAL MODES; THERMODYNAMICS; CLOUD; CHEMISTRY; DESITTER; BEHAVIOR; GRAVITY; VAN;
D O I
10.1088/1674-1137/ad361f
中图分类号
O57 [原子核物理学、高能物理学];
学科分类号
070202 ;
摘要
We obtain an exact solution for spherically symmetric Letelier AdS black holes immersed in perfect fluid dark matter (PFDM). Considering the cosmological constant as the positive pressure of the system and volume as its conjugate variable, we analyze the thermodynamics of our black holes in the extended phase space. Owing to the background clouds of strings parameter (a) and the parameter endowed with PFDM (beta), we analyze the Hawking temperature, entropy, and specific heat. Furthermore, we investigate the relationship between the photon sphere radius and phase transition for the Letelier AdS black holes immersed in PFDM. Through the analysis, with a particular condition, non-monotonic behaviors are found between the photon sphere radius, impact parameter, PFDM parameter, temperature, and pressure. We can regard the changes in both the photon sphere radius and impact parameter before and after phase transition as the order parameter; their critical exponents near the critical point are equal to the same value, 1/2, similar to that in ordinary thermal systems. This indicates that a universal relation of gravity may exist near the critical point for a black hole thermodynamic system.
引用
收藏
页数:13
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