Embedding hairy black holes in a magnetic universe

被引：29

作者：

Astorino, Marco ^{[1
]}

机构：

[1] Ctr Estudios Cient, Valdivia 5110466, Chile

来源：

PHYSICAL REVIEW D | 2013年 / 87卷 / 08期

关键词：

FORMULATION;

D O I：

10.1103/PhysRevD.87.084029

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Ernst's solution-generating technique is adapted to Einstein-Maxwell theory conformally (and minimally) coupled to a scalar field. This integrable system enjoys an SU(2,1) symmetry which enables one to move, by Kinnersley transformations, through the axisymmetric and stationary solution space, building an infinite tower of physically inequivalent solutions. As a specific application, metrics associated to scalar hairy black holes-such as the ones discovered by Bocharova, Bronnikov, Melnikov, and Bekenstein-are embedded in the external magnetic field of the Melvin universe. DOI: 10.1103/PhysRevD.87.084029

引用

页数：10

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