Rotating black holes in a Gödel universe | Zendy

Dominic Brecher | Zendy; Ulf Danielsson | Zendy; James P Gregory | Zendy; Martin E Olsson | Zendy

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Rotating black holes in a Gödel universe

Author(s) -

Dominic Brecher,

Ulf Danielsson,

James P Gregory,

Martin E Olsson

Publication year - 2003

Publication title -

journal of high energy physics

Language(s) - English

Resource type - Journals

SCImago Journal Rank - 0.998

H-Index - 261

eISSN - 1126-6708

pISSN - 1029-8479

DOI - 10.1088/1126-6708/2003/11/033

Subject(s) - physics , closed timelike curve , black hole (networking) , supergravity , black brane , plane (geometry) , theoretical physics , rotating black hole , rotation (mathematics) , mathematical physics , extremal black hole , classical mechanics , astrophysics , supersymmetry , quantum mechanics , geometry , accretion (finance) , angular momentum , mathematics , computer network , routing protocol , routing (electronic design automation) , computer science , spacetime , link state routing protocol

We construct a five--dimensional, asymptotically Goedel, three--charge blackhole via dimensional reduction of an asymptotically plane wave, rotatingD1-D5-brane solution of type IIB supergravity. This latter is itselfconstructed via the solution generating procedure of Garfinkle and Vachaspati,applied to the standard rotating D1-D5-brane solution. Taking all charges to beequal gives a "BMPV Goedel black hole", which is closely related to thatrecently found by Herdeiro. We emphasise, however, the importance of ourten--dimensional microscopic description in terms of branes. We discuss variousproperties of the asymptotically Goedel black hole, including the physicalbound on the rotation of the hole, the existence of closed timelike curves, andpossible holographic protection of chronology.Comment: 27 pages, 2 figures, LaTeX. v2: references and minor comments added. v3: very minor comments added, version published in JHE

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