Black holes in symmetric spaces : anti-de Sitter spaces

Simple item page
dc.creatorClaessens, Laurent
dc.creatorDetournay, Stéphane
dc.date2005-10-20
dc.date.accessioned2026-07-07T06:47:43Z
dc.date.available2026-07-07T06:47:43Z
dc.descriptionUsing 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.
dc.description23 pages, no figure
dc.identifierhttps://arxiv.org/abs/math/0510442
dc.identifierhttp://arxiv.org/abs/math/0510442
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/103749
dc.subjectDifferential Geometry
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectHigh Energy Physics - Theory
dc.titleBlack holes in symmetric spaces : anti-de Sitter spaces
dc.typetext

Files

Collections

arXiv