Three-dimensional origin of Gödel spacetimes and black holes

dc.creatorBañados, M.
dc.creatorBarnich, G.
dc.creatorCompere, G.
dc.creatorGomberoff, A.
dc.date.accessioned2021-06-19T23:46:29Z
dc.date.accessioned2024-05-02T15:07:04Z
dc.date.available2021-06-19T23:46:29Z
dc.date.available2024-05-02T15:07:04Z
dc.date.created2021-06-19T23:46:29Z
dc.date.issued2006-02
dc.identifierPhysical Review D - Particles, Fields, Gravitation and CosmologyOpen AccessVolume 73, Issue 42006 Article number 044006
dc.identifier1550-2368
dc.identifierhttp://repositorio.unab.cl/xmlui/handle/ria/19146
dc.identifier10.1103/PhysRevD.73.044006
dc.identifier.urihttps://repositorioslatinoamericanos.uchile.cl/handle/2250/9262734
dc.description.abstractWe construct Gödel-type black hole and particle solutions to Einstein-Maxwell theory in 2+1 dimensions with a negative cosmological constant and a Chern-Simons term. On-shell, the electromagnetic stress-energy tensor effectively replaces the cosmological constant by minus the square of the topological mass and produces the stress-energy of a pressure-free perfect fluid. We show how a particular solution is related to the original Gödel universe and analyze the solutions from the point of view of identifications. Finally, we compute the conserved charges and work out the thermodynamics. © 2006 The American Physical Society.
dc.languageen
dc.publisherAmerican Physical Society
dc.subjectBlack Holes
dc.subjectEvent Horizon
dc.subjectSupergravity
dc.titleThree-dimensional origin of Gödel spacetimes and black holes
dc.typeArtículo


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