Three-dimensional Chern-Simons black holes

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dc.creatorMoussa, K. Ait
dc.creatorClement, G.
dc.creatorGuennoune, H.
dc.creatorLeygnac, C.
dc.date2008-07-26
dc.date.accessioned2026-07-07T11:45:06Z
dc.date.available2026-07-07T11:45:06Z
dc.descriptionWe construct black hole solutions to three-dimensional Einstein-Maxwell theory with both gravitational and electromagnetic Chern-Simons terms. These intrinsically rotating solutions are geodesically complete, and causally regular within a certain parameter range. Their mass, angular momentum and entropy are found to satisfy the first law of black hole thermodynamics. These Chern-Simons black holes admit a four-parameter local isometry algebra, which generically is $sl(2,R)\times R$, and may be generated from the corresponding vacua by local coordinate transformations.
dc.description21 pages
dc.identifierhttps://arxiv.org/abs/0807.4241
dc.identifierhttp://arxiv.org/abs/0807.4241
dc.identifierPhys.Rev.D78:064065,2008
dc.identifierdoi:10.1103/PhysRevD.78.064065
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/201774
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectHigh Energy Physics - Theory
dc.titleThree-dimensional Chern-Simons black holes
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