Thermodynamic geometry of black hole in the deformed Horava-Lifshitz gravity

被引:34
|
作者
Wei, Shao-Wen [1 ]
Liu, Yu-Xiao [1 ]
Wang, Yong-Qiang [1 ]
Guo, Heng [1 ]
机构
[1] Lanzhou Univ, Inst Theoret Phys, Lanzhou 730000, Peoples R China
基金
中国国家自然科学基金;
关键词
RIEMANNIAN GEOMETRY; CURVATURE;
D O I
10.1209/0295-5075/99/20004
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
We investigate the thermodynamic geometry and phase transition of Kehagias-Sfetsos black hole in the deformed Horava-Lifshitz gravity with coupling constant lambda = 1. The phase transition in black-hole thermodynamics is thought to be associated with the divergence of the capacities. And the structures of these divergent points are studied. We also find that the thermodynamic curvature produced by the Ruppeiner metric is positive definite for all r(1) > r and is divergent at eta(2) = 0 corresponding to the divergent points of C-Phi and C-tau. These results suggest that the microstructure of the black hole has an effective repulsive interaction, which is very similar to the ideal gas of fermions. These may shed some light on the microstructure of the black hole. Copyright (c) EPLA, 2012
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页数:5
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