Bumpy black holes

被引:30
作者
Emparan R. [1 ,2 ]
Figueras P. [3 ]
Martínez M. [2 ]
机构
[1] Institució Catalana de Recerca i Estudis Avançats (ICREA), Passeig Lluís Companys 23, Barcelona
[2] Departament de Física Fonamental, Institut de Ciències del Cosmos, Universitat de Barcelona, Martí i Franquès 1, Barcelona
[3] DAMTP, Centre for Mathematical Sciences, Wilberforce Road, Cambridge
基金
英国科学技术设施理事会; 欧洲研究理事会;
关键词
Black Holes; Black Holes in String Theory;
D O I
10.1007/JHEP12(2014)072
中图分类号
学科分类号
摘要
Abstract: We study six-dimensional rotating black holes with bumpy horizons: these are topologically spherical, but the sizes of symmetric cycles on the horizon vary nonmonotonically with the polar angle. We construct them numerically for the first three bumpy families, and follow them in solution space until they approach critical solutions with localized singularities on the horizon. We find strong evidence of the conical structures that have been conjectured to mediate the transitions to black rings, to black Saturns, and to a novel class of bumpy black rings. For a different, recently identified class of bumpy black holes, we find evidence that this family ends in solutions with a localized singularity that exhibits apparently universal properties, and which does not seem to allow for transitions to any known class of black holes. © 2014, The Author(s).
引用
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页数:23
相关论文
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