Tunnelling from Gödel black holes
- 12 April 2007
- journal article
- research article
- Published by American Physical Society (APS) in Physical Review D
- Vol. 75 (8) , 084022
Abstract
We consider the spacetime structure of Kerr-Gödel black holes, analyzing their parameter space in detail. We apply the tunnelling method to compute their temperature and compare the results to previous calculations obtained via other methods. We claim that it is not possible to have the closed timelike curve (CTC) horizon in between the two black hole horizons and include a discussion of issues that occur when the radius of the CTC horizon is smaller than the radius of both black hole horizons.Keywords
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This publication has 31 references indexed in Scilit:
- Classical and quantum strings in compactifiedppwaves and Gödel type universesPhysical Review D, 2004
- The Taming of Closed Time-like CurvesJournal of High Energy Physics, 2004
- Rotating black holes in a Gödel universeJournal of High Energy Physics, 2003
- The Kerr–Newman–Gödel black holeClassical and Quantum Gravity, 2003
- Closed timelike curves and holography in compact plane wavesJournal of High Energy Physics, 2003
- All supersymmetric solutions of minimal supergravity in five dimensionsClassical and Quantum Gravity, 2003
- Spinning deformations of the D1–D5 system and a geometric resolution of closed timelike curvesNuclear Physics B, 2003
- Black Holes in Gödel Universes andWavesPhysical Review Letters, 2003
- Supersymmetric Gödel Universes in string theoryNuclear Physics B, 2003
- Holographic protection of chronology in universes of the Gödel typePhysical Review D, 2003