Anti-de Sitter-type 2+1 spacetime of a charged rotating mass

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dc.creatorMitskievich, Nikolai V.
dc.creatorGarcia, Alberto A.
dc.date2001-01-09
dc.date2001-02-13
dc.date.accessioned2026-07-07T03:25:35Z
dc.date.available2026-07-07T03:25:35Z
dc.descriptionThe exact charged rotating solution of 2+1 Einstein-Maxwell equations with $Λ$ term is obtained and its properties outlined. It generalizes the Cataldo-Cruz-del Campo-Garc{\'ı}a relativistic charged massive black hole on the 2+1 anti-de Sitter cosmological background. We show that rotating solutions correspond to inhomogeneous field equations, thus presence of sources in 2+1 Maxwell's equations cannot be identified with existence of a charge distribution. Instead, these sources are related to the 2+1 Machian 2-form field, and the overall Lagrangian structure of the rotating system is reconstructed.
dc.description9 pages, LaTeX file using amssym.def; corrected references and extended content
dc.identifierhttps://arxiv.org/abs/gr-qc/0101029
dc.identifierhttp://arxiv.org/abs/gr-qc/0101029
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/33768
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleAnti-de Sitter-type 2+1 spacetime of a charged rotating mass
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