Non-Abelian black holes in D=5 maximal gauged supergravity

被引:12
作者
Cvetic, M. [1 ]
Lue, H. [2 ,3 ]
Pope, C. N. [2 ,4 ]
机构
[1] Univ Penn, Dept Phys & Astron, Philadelphia, PA 19104 USA
[2] Texas A&M Univ, George & Cynthia Woods Mitchell Inst Fundamental, College Stn, TX 77843 USA
[3] Cent Univ Finance & Econ, China Inst Adv Study, Div Appl Math & Theoret Phys, Beijing 100081, Peoples R China
[4] Univ Cambridge, Ctr Math Sci, DAMTP, Cambridge CB3 OWA, England
来源
PHYSICAL REVIEW D | 2010年 / 81卷 / 04期
基金
美国国家科学基金会;
关键词
N=4; MONOPOLES;
D O I
10.1103/PhysRevD.81.044023
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We investigate static non-Abelian black hole solutions of anti-de Sitter (AdS) Einstein-Yang-Millsdilaton gravity, which is obtained as a consistent truncation of five-dimensional maximal gauged supergravity. If the dilaton is (consistently) set to zero, the remaining equations of motion, with a spherically-symmetric ansatz, may be derived from a superpotential. The associated first-order equations admit an explicit solution supported by a non-Abelian SU(2) gauge potential, which has a logarithmically growing mass term. In an extremal limit the horizon geometry becomes AdS(2) x S-3. If the dilaton is also excited, the equations of motion cannot easily be solved explicitly, but we obtain the asymptotic form of the more general non-Abelian black holes in this case. An alternative consistent truncation, in which the Yang-Mills fields are set to zero, also admits a description in terms of a superpotential. This allows us to construct explicit wormhole solutions (neutral spherically-symmetric domain walls). These solutions may be generalized to dimensions other than five.
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页数:7
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