Black diamonds at brane junctions -: art. no. 044012

被引:27
作者
Chamblin, A
Csáki, C
Erlich, J
Hollowood, TJ
机构
[1] MIT, Ctr Theoret Phys, Cambridge, MA 02139 USA
[2] Los Alamos Natl Lab, Div Theory T8, Los Alamos, NM 87545 USA
[3] Univ Wales Swansea, Dept Phys, Swansea, W Glam, Wales
来源
PHYSICAL REVIEW D | 2000年 / 62卷 / 04期
关键词
D O I
10.1103/PhysRevD.62.044012
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We discuss the properties of black holes in brane-world scenarios where our Universe is viewed as a four-dimensional sub-manifold of some higher-dimensional spacetime. We consider in detail such a model where four-dimensional spacetime lies at the junction of several domain walls in a higher dimensional anti-de Sitter spacetime. In this model there may be any number p of infinitely large extra dimensions transverse to the brane-world. We present an exact solution describing a black p-brane which will induce on the brane-world the Schwarzschild solution. This exact solution is unstable to the Gregory-Laflamme instability, whereby long-wavelength perturbations cause the extended horizon to fragment. We therefore argue that at late times a non-rotating uncharged black hole in the brane-world is described by a deformed event horizon in p+4 dimensions which will induce, to good approximation, the Schwarzschild solution in the four-dimensional brane world. When p=2, this deformed horizon resembles a black diamond and more generally fur p>2, a polyhedron.
引用
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页码:1 / 7
页数:7
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