Charged rotating Kaluza–Klein black holes generated by G2(2) transformation
Charged rotating Kaluza–Klein black holes generated by G2(2) transformation
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DOI：
10.1088/0264-9381/26/14/145006
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发表时间：
2008-09
影响因子：
3.5
通讯作者：
Shinya Tomizawa;Y. Yasui;Y. Morisawa
中科院分区：
文献类型：
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作者：
Shinya Tomizawa;Y. Yasui;Y. Morisawa
将最小D = 5超引力的G2(2)生成技术应用于Rasheed黑洞解，给出了五维einstein - maxwell - chen - simons方程的一个新的旋转带电Kaluza-Klein黑洞解。在无穷远处，我们的解表现为具有紧致额外维度的四维平坦时空，因此描述了卡鲁扎-克莱因黑洞。特别地，极端解是非超对称的，这与静态情况相反。我们的解具有渐近平荷旋转黑洞解和一个新的荷荷旋转黑弦解的极限。
Applying 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.