Shinya Tomizawa et al 2009 Class. Quantum Grav. 26 145006 doi:10.1088/0264-9381/26/14/145006
Shinya Tomizawa1, Yukinori Yasui2 and Yoshiyuki Morisawa3
Show affiliationsApplying the G2(2) generating technique for minimal D = 5 supergravity to the Rasheed black hole solution, we present a new rotating charged Kaluza–Klein black hole solution to the five-dimensional Einstein–Maxwell–Chern–Simons equations. At infinity, our solution behaves as a four-dimensional flat spacetime with a compact extra dimension and hence describes a Kaluza–Klein black hole. In particular, the extreme solution is non-supersymmetric, which is in contrast to a static case. Our solution has the limits to the asymptotically flat charged rotating black hole solution and a new charged rotating black string solution.
04.70.Bw Classical 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
83C30 Asymptotic procedures (radiation, news functions, H-spaces, etc.)
Issue 14 (21 July 2009)
Received 13 February 2009, in final form 12 April 2009
Published 19 June 2009
Shinya Tomizawa et al 2009 Class. Quantum Grav. 26 145006
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