Black Holes and Wormholes in 2+1 Dimensions

dc.creatorBrill, Dieter
dc.date1999-04-30
dc.date1999-06-12
dc.date.accessioned2026-07-07T03:33:09Z
dc.date.available2026-07-07T03:33:09Z
dc.descriptionVacuum Einstein theory in three spacetime dimensions is locally trivial, but admits many solutions that are globally different, particularly if there is a negative cosmological constant. The classical theory of such locally "anti-de Sitter" spaces is treated in an elementary way, using visualizable models. Among the objects discussed are black holes, spaces with multiple black holes, their horizon structure, closed universes, and the topologies that are possible.
dc.description37 pages Latex2e including 17 LaTeX figures. Submitted to Proceedings of 2nd Samos Meeting on Cosmology Geometry and Relativity (Springer-Verlag) Typos crrected, section 4.3 (Multiple Black Holes with Angular Momentum) revised
dc.identifierhttps://arxiv.org/abs/gr-qc/9904083
dc.identifierhttp://arxiv.org/abs/gr-qc/9904083
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/36509
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleBlack Holes and Wormholes in 2+1 Dimensions
dc.typetext

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