Black holes in symmetric spaces : anti-de Sitter spaces

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Using symmetric space techniques, we show that closed orbits of the Iwasawa subgroups of $SO(2,l-1)$ naturally define singularities of a black hole causal structure in anti-de Sitter spaces in $l \geq 3$ dimensions. In particular, we recover for $l=3$ the non-rotating massive BTZ black hole. The method presented here is very simple and in principle generalizable to any semi-simple symmetric space.
23 pages, no figure

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Differential Geometry, General Relativity and Quantum Cosmology, High Energy Physics - Theory

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http://salesiana.dossiersoluciones.com/handle/123456789/103749

Consulte el texto completo en el siguiente enlace:

https://arxiv.org/abs/math/0510442
 http://arxiv.org/abs/math/0510442

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arXiv