Charged Black Holes in a Rotating Gross-Perry-Sorkin Monopole Background
arXiv:0807.1564 · doi:10.1088/0264-9381/25/24/245007
Abstract
We 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.
25 pages, 6 figures
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