On generalized quasi-topological cubic-quartic gravity: thermodynamics and holography

被引:30
|
作者
Mir, Mozhgan [1 ,2 ]
Mann, Robert B. [1 ,3 ]
机构
[1] Univ Waterloo, Dept Phys & Astron, Waterloo, ON N2L 3G1, Canada
[2] Ferdowsi Univ Mashhad, Fac Sci, Dept Phys, POB 1436, Mashhad, Razavi Khorasan, Iran
[3] Perimeter Inst, 31 Caroline St North, Waterloo, ON N2L 2Y5, Canada
基金
加拿大自然科学与工程研究理事会;
关键词
Black Holes; AdS-CFT Correspondence; SYMMETRICAL-SOLUTIONS; EINSTEIN; DESITTER;
D O I
10.1007/JHEP07(2019)012
中图分类号
O412 [相对论、场论]; O572.2 [粒子物理学];
学科分类号
摘要
We investigate the thermodynamic behaviour of asymptotically anti de Sitter black holes in generalized quasi-topological gravity containing terms both cubic and quartic in the curvature. We investigate the general conditions required for physical phase transitions and critical behaviour in any dimension and then consider in detail specific properties in spacetime dimensions 4, 5, and 6. We find for spherical black holes that there are respectively at most two and three physical critical points in five and six dimensions. For hyperbolic black holes we find the occurrence of Van der Waals phase transitions in four dimensions and reverse Van der Waals phase transitions in dimensions greater than 4 if both cubic and quartic curvature terms are present. We also observe the occurrence of phase transitions in for fixed chemical potential. We consider some applications of our work in the dual CFT, investigating how the ratio of viscosity to entropy is modified by inclusion of these higher curvature terms. We conclude that the presence of the quartic curvature term results in a violation of the KSS bound in five dimensions, but not in other dimensions.
引用
收藏
页数:58
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