Charged black holes in quartic quasi-topological gravity

被引:11
|
作者
Ghanaatian, M. [1 ]
Naeimipour, F. [1 ]
Bazrafshan, A. [2 ]
Abkar, M. [1 ]
机构
[1] PNU, Dept Phys, POB 19395-3697, Tehran, Iran
[2] Jahrom Univ, Dept Phys, Jahrom 7413766171, Iran
关键词
SHEAR VISCOSITY;
D O I
10.1103/PhysRevD.97.104054
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
In this paper, we construct exact solutions of charged black holes in the presence of quartic quasi-topological gravity. We obtain thermodynamics and conserved quantities of the solutions and check the first law of thermodynamics. In studying the physical properties of the solutions, we consider anti-de Sitter, de Sitter, and flat solutions of charged black holes in quartic quasi-topological gravity and compare them with Einstein and third-order quasi-topological gravities. We also investigate the thermal stability of the solutions and show that thermal stability is just for anti-de Sitter solutions, not for de Sitter and flat ones.
引用
收藏
页数:12
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