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arXiv · 0809.2001

Charged Rotating Kaluza-Klein Black Holes Generated by G2(2) Transformation

Shinya Tomizawa·Yukinori Yasui·Yoshiyuki Morisawa
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Abstract

Applying the G_{2(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 particlar, the extreme solution is non-supersymmetric, which is 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.

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Shinya Tomizawa, Yukinori Yasui, Yoshiyuki Morisawa. 2008-09-17. Charged Rotating Kaluza-Klein Black Holes Generated by G2(2) Transformation. https://doi.org/10.1088/0264-9381%2F26%2F14%2F145006

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