Rotating Black Holes on Codimension-2 Branes

Simple item page
dc.creatorKiley, Derrick
dc.date2007-08-07
dc.date.accessioned2026-07-07T11:18:31Z
dc.date.available2026-07-07T11:18:31Z
dc.descriptionIt has recently been demonstrated that certain types of non-tensional stress-energy can live on tensional codimension-2 branes, including gravitational shockwaves and small Schwarzschild black holes. In this note we generalize the earlier Schwarzschild results, and construct the exact gravitational fields of small rotating black holes on a codimension-2 brane. We focus on the phenomenologically interesting case of a three-brane embedded in a spacetime with two compactified extra dimensions. For a nonzero tension on the brane, we verify that these solutions also show the ``lightning rod'' effect found in the Schwarzschild solutions, the net effect of which is to rescale the fundamental Planck mass. This allows for larger black hole parameters, such as the event horizon, angular momentum, and lifetime than would be naively expected for a tensionless brane. It is also found that a black hole with angular momentum pointing purely along the brane directions has a smaller horizon angular velocity than the corresponding tensionless case, while a hole with bulk components of angular momentum has a larger angular velocity.
dc.description7 pages, uses revtex
dc.identifierhttps://arxiv.org/abs/0708.1016
dc.identifierhttp://arxiv.org/abs/0708.1016
dc.identifierPhys.Rev.D76:126002,2007
dc.identifierdoi:10.1103/PhysRevD.76.126002
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/193368
dc.subjectHigh Energy Physics - Theory
dc.subjectAstrophysics
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectHigh Energy Physics - Phenomenology
dc.titleRotating Black Holes on Codimension-2 Branes
dc.typetext

Files

Collections

arXiv