Rotating Charged Solutions to Einstein-Maxwell-ChernSimons Theory in 2+1 Dimensions

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dc.creatorFernando, Sharmanthie
dc.creatorMansouri, Freydoon
dc.date1997-05-09
dc.date1999-09-13
dc.date.accessioned2026-07-07T09:03:03Z
dc.date.available2026-07-07T09:03:03Z
dc.descriptionWe obtain a class of rotating charged stationary circularly symmetric solutions of Einstein-Maxwell theory coupled to a topological mass term for the Maxwell field. These solutions are regular, have finite mass and angular momentum, and are asymptotic to the uncharged extreme BTZ black hole.
dc.description15 pages, LaTeX, Improvements on presentation. All the results remain unchanged
dc.identifierhttps://arxiv.org/abs/gr-qc/9705016
dc.identifierhttp://arxiv.org/abs/gr-qc/9705016
dc.identifierComm. Math. Theor. Phys. , 1 (1998) 14
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/148865
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleRotating Charged Solutions to Einstein-Maxwell-ChernSimons Theory in 2+1 Dimensions
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