Shinya Tomizawa and Akihiro Ishibashi 2008 Class. Quantum Grav. 25 245007 doi:10.1088/0264-9381/25/24/245007
Shinya Tomizawa1 and Akihiro Ishibashi1,2
Show affiliationsWe 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.
04.70.-s Physics of black holes
04.40.Nr Einstein-Maxwell spacetimes, spacetimes with fluids, radiation or classical fields
04.50.-h Higher-dimensional gravity and other theories of gravity
Issue 24 (21 December 2008)
Received 21 July 2008
Published 27 November 2008
Shinya Tomizawa and Akihiro Ishibashi 2008 Class. Quantum Grav. 25 245007
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