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Black holes in Goedel-type universes with a cosmological constant

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arxiv hep-th/0401239 v3 pith:XGQR335F submitted 2004-01-30 hep-th gr-qc

Klaus Behrndt , Dietmar Klemm This is my paper · ORCID
classification hep-thgr-qc
keywords blackclosedconstantcosmologicalcurvesdeformationgoedel-typeholes
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We discuss supersymmetric black holes embedded in a Goedel-type universe with cosmological constant in five dimensions. The spacetime is a fibration over a four-dimensional Kaehler base manifold, and generically has closed timelike curves. Asymptotically the space approaches a deformation of AdS_5, which suggests that the appearance of closed timelike curves should have an interpretation in some deformation of D=4, N=4 super-Yang-Mills theory. Finally, a Goedel-de Sitter universe is also presented and its causal structure is discussed.

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Cited by 1 Pith paper

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  1. Extended uncertainty principle inspired black hole in a G\"odel Universe

    gr-qc 2025-05 reject novelty 4.0 of 10

    A Godel-rotation-modified uncertainty principle is used to define a corrected black hole mass, producing enlarged horizon, shadow, and deflection with lower bounds a/M ~ 10^5 from EHT and PPN data.

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