Charged Black Holes in a Rotating Gross-Perry-Sorkin Monopole Background

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dc.creatorTomizawa, Shinya
dc.creatorIshibashi, Akihiro
dc.date2008-07-10
dc.date.accessioned2026-07-07T12:14:58Z
dc.date.available2026-07-07T12:14:58Z
dc.descriptionWe present a new class of stationary charged black hole solutions to five-dimensional Einstein-Maxwell-Chern-Simons theories. We construct the solutions by utilizing so called the squashing transformation. At infinity, our solutions behave as a four-dimensional flat spacetime plus a `circle' and hence describe a Kaluza-Klein black hole. More precisely, our solutions can be viewed as a charged rotating black hole in a rotating Gross-Perry-Sorkin monopole background with the black hole rotation induced from the background rotation.
dc.description25 pages, 6 figures
dc.identifierhttps://arxiv.org/abs/0807.1564
dc.identifierhttp://arxiv.org/abs/0807.1564
dc.identifierClass.Quant.Grav.25:245007,2008
dc.identifierdoi:10.1088/0264-9381/25/24/245007
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/211372
dc.subjectHigh Energy Physics - Theory
dc.titleCharged Black Holes in a Rotating Gross-Perry-Sorkin Monopole Background
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