AdS and Lifshitz black holes in conformal and Einstein-Weyl gravities

被引:152
作者
Lu, H. [1 ,2 ]
Pang, Yi [3 ]
Pope, C. N. [3 ,4 ]
Vazquez-Poritz, J. F. [5 ,6 ,7 ]
机构
[1] Cent Univ Finance & Econ, China Econ & Management Acad, Beijing 100081, Peoples R China
[2] Shenzhen Univ, Inst Adv Study, Shenzhen 518060, Peoples R China
[3] Texas A&M Univ, George P & Cynthia Woods Mitchell Inst Fundamenta, College Stn, TX 77843 USA
[4] Univ Cambridge, DAMTP, Ctr Math Sci, Cambridge CB3 OWA, England
[5] CUNY, New York City Coll Technol, Brooklyn, NY 11201 USA
[6] CUNY, Grad Sch, New York, NY 10016 USA
[7] CUNY, Univ Ctr, New York, NY 10016 USA
来源
PHYSICAL REVIEW D | 2012年 / 86卷 / 04期
关键词
THERMODYNAMICS; LAW;
D O I
10.1103/PhysRevD.86.044011
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We study black hole solutions in extended gravities with higher-order curvature terms, including conformal and Einstein-Weyl gravities. In addition to the usual anti-de Sitter (AdS) vacuum, the theories admit Lifshitz and Schrodinger vacua. The AdS black hole in conformal gravity contains an additional parameter over and above the mass, which may be interpreted as a massive spin-2 hair. By considering the first law of thermodynamics, we find that it is necessary to introduce an associated additional intensive/extensive pair of thermodynamic quantities. We also obtain new Lifshitz black holes in conformal gravity and study their thermodynamics. We use a numerical approach to demonstrate that AdS black holes beyond the Schwarzschild-AdS solution exist in Einstein-Weyl gravity. We also demonstrate the existence of asymptotically Lifshitz black holes in Einstein-Weyl gravity. The Lifshitz black holes arise at the boundary of the parameter ranges for the AdS black holes. Outside the range, the solutions develop naked singularities. The asymptotically AdS and Lifshitz black holes provide an interesting phase transition, in the corresponding boundary field theory, from a relativistic Lorentzian system to a nonrelativistic Lifshitz system.
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页数:22
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