Joule-Thomson expansion of lower-dimensional black holes

被引:9
|
作者
Liang, Jing [1 ,2 ]
Mu, Benrong [1 ,2 ]
Wang, Peng [2 ]
机构
[1] Chengdu Univ Tradit Chinese Med, Coll Med Technol, Phys Teaching & Res Sect, Chengdu 611137, Peoples R China
[2] Sichuan Univ, Coll Phys, Ctr Theoret Phys, Chengdu 610064, Peoples R China
基金
美国国家科学基金会;
关键词
HAWKING RADIATION; FIELD; THERMODYNAMICS; BEHAVIOR; ENTROPY;
D O I
10.1103/PhysRevD.104.124003
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Herein, we extend Joule-Thomson expansion to the low-dimensional regime by considering the rotating Banados-Teitelboim-Zanelli (BTZ) metric in the (2 + 1)-dimensional space-time. Specifically, the properties of three important aspects of the Joule-Thomson expansion, including the Joule-Thomson coefficient, inversion curve, and isenthalpic curve were studied. The divergence point of the Joule-Thomson coefficient and the zero point of the Hawking temperature were investigated. The inversion temperature and isenthalpic curves in the T-P plane were obtained, and the cooling-heating regions were determined. Furthermore, the minimum inversion temperature was found to be zero, and the black hole becomes an extremal black hole. The ratio of the minimum inversion and critical temperatures for BTZ black holes does not exist, since the BTZ black hole does not exhibit the critical behavior in the critical pressure Pc, critical temperature Tc, and critical volume Vc.
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页数:9
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