Tunnelling From Gödel Black Holes

dc.creatorKerner, Ryan
dc.creatorMann, R. B.
dc.date2007-01-11
dc.date2007-01-19
dc.date.accessioned2026-07-07T11:03:06Z
dc.date.available2026-07-07T11:03:06Z
dc.descriptionWe consider the spacetime structure of Kerr-Gödel black holes, analyzing their parameter space Kerr-Gödel 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 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.
dc.description19 pages, 5 figures, added reference
dc.identifierhttps://arxiv.org/abs/hep-th/0701107
dc.identifierhttp://arxiv.org/abs/hep-th/0701107
dc.identifierPhys.Rev.D75:084022,2007
dc.identifierdoi:10.1103/PhysRevD.75.084022
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/188476
dc.subjectHigh Energy Physics - Theory
dc.titleTunnelling From Gödel Black Holes
dc.typetext

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