Exact asymptotically flat charged hairy black holes with a dilaton potential

被引:62
作者
Anabalon, Andres [1 ,2 ]
Astefanesei, Dumitru [3 ]
Mann, Robert [4 ,5 ]
机构
[1] Univ Adolfo Ibanez, Fac Artes Liberales, Dept Ciencias, Vina Del Mar, Chile
[2] Univ Adolfo Ibanez, Fac Ingn & Ciencias, Vina Del Mar, Chile
[3] Pontificia Univ Catolica Valparaiso, Inst Fis, Valparaiso, Chile
[4] Univ Waterloo, Dept Phys & Astron, Waterloo, ON N2L 3G1, Canada
[5] Perimeter Inst, Waterloo, ON N2L 2Y5, Canada
来源
JOURNAL OF HIGH ENERGY PHYSICS | 2013年 / 10期
基金
加拿大自然科学与工程研究理事会;
关键词
Classical Theories of Gravity; Black Holes; RELATIVISTIC GRAVITATIONAL COLLAPSE; NONSPHERICAL PERTURBATIONS; SCALAR; SUPERSYMMETRY; STATIONARY; ENTROPY; THEOREM; MODULI;
D O I
10.1007/JHEP10(2013)184
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 find broad classes of exact 4-dimensional asymptotically flat black hole solutions in Einstein-Maxwell theories with a non-minimally coupled dilaton and its non-trivial potential. We consider a few interesting limits, in particular, a regular generalization of the dilatonic Reissner-Nordstrom solution and, also, smooth deformations of supersymmetric black holes. Further examples are provided for more general dilaton potentials. We discuss the thermodynamical properties and show that the first law is satisfied. In the non-extremal case the entropy depends, as expected, on the asymptotic value of the dilaton. In the extremal limit, the entropy is determined purely in terms of charges and is independent of the asymptotic value of the dilaton. The attractor mechanism can be used as a criterion for the existence of the regular solutions. Since there is a 'competition' between the effective potential and dilaton potential, we also obtain regular extremal black hole solutions with just one U(1) gauge field turned on.
引用
收藏
页数:22
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