Gravitating defects of codimension-two

dc.creatorKofinas, Georgios
dc.creatorTomaras, Theodore
dc.date2007-02-01
dc.date2007-10-24
dc.date.accessioned2026-07-07T11:23:37Z
dc.date.available2026-07-07T11:23:37Z
dc.descriptionThin gravitating defects with conical singularities in higher codimensions and with generalized Israel matching conditions are known to be inconsistent for generic energy-momentum. A way to remove this inconsistency is proposed and is realized for an axially symmetric gravitating codimension-two defect in six dimensional Einstein gravity. By varying with respect to the brane embedding fields, alternative matching conditions are derived, which are generalizations of the Nambu-Goto equations of motion of the defect, consistent with bulk gravity. For a maximally symmetric defect the standard picture is recovered. The four-dimensional perfect fluid cosmology coincides with conventional FRW in the case of radiation, but for dust it has rho^{4/3} instead of rho. A four-dimensional black hole solution is presented having the Schwarzschild form with a short-distance correction r^{-2}.
dc.descriptionMinor changes, to appear in Classical and Quantum Gravity
dc.identifierhttps://arxiv.org/abs/hep-th/0702010
dc.identifierhttp://arxiv.org/abs/hep-th/0702010
dc.identifierClass.Quant.Grav.24:5861-5867,2007
dc.identifierdoi:10.1088/0264-9381/24/23/009
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/194948
dc.subjectHigh Energy Physics - Theory
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleGravitating defects of codimension-two
dc.typetext

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