Stability of 3D black hole with torsion

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dc.creatorCvetković, B.
dc.creatorBlagojević, M.
dc.date2007-12-10
dc.date.accessioned2026-07-07T11:39:17Z
dc.date.available2026-07-07T11:39:17Z
dc.descriptionUsing $N=1+1$ supersymmetric extension of the three-dimensional gravity with torsion, we show that a generic black hole has no exact supersymmetries, the extremal black hole has only one, while the zero-energy black hole has two. Combining these results with the asymptotic supersymmetry algebra, we are naturally led to interpret the zero-energy black hole as the ground state of the Ramond sector, and analogously, the anti-de Sitter solution as the ground state of the Neveau-Schwartz sector.
dc.descriptionLATEX, 9 pages
dc.identifierhttps://arxiv.org/abs/0712.1434
dc.identifierhttp://arxiv.org/abs/0712.1434
dc.identifierMod.Phys.Lett.A22:3047-3055,2007
dc.identifierdoi:10.1142/S0217732307026126
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/199864
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleStability of 3D black hole with torsion
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