Inside the BTZ black hole

dc.creatorde Berredo-Peixoto, G.
dc.creatorKatanaev, M. O.
dc.date2006-11-27
dc.date.accessioned2026-07-07T10:22:03Z
dc.date.available2026-07-07T10:22:03Z
dc.descriptionWe consider static circularly symmetric solution of three-dimensional Einstein's equations with negative cosmological constant (the BTZ black hole). The case of zero cosmological constant corresponding to the interior region of a black hole is analyzed in detail. We prove that the maximally extended BTZ solution with zero cosmological constant coincides with flat three-dimensional Minkowskian space-time without any singularity and horizons. The Euclidean version of this solution is shown to have physical interpretation in the geometric theory of defects in solids describing combined wedge and screw dislocations.
dc.description24 pages, 8 figures
dc.identifierhttps://arxiv.org/abs/gr-qc/0611143
dc.identifierhttp://arxiv.org/abs/gr-qc/0611143
dc.identifierPhys.Rev.D75:024004,2007
dc.identifierdoi:10.1103/PhysRevD.75.024004
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/175380
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleInside the BTZ black hole
dc.typetext

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