Rotating Einstein–Maxwell–dilaton black holes in D dimensions
Rotating Einstein–Maxwell–dilaton black holes in D dimensions
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DOI：
10.1016/j.physletb.2006.06.024
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发表时间：
2006-06
影响因子：
4.4
通讯作者：
J. Kunz;D. Maison;F. Navarro-Lérida;J. Viebahn
中科院分区：
文献类型：
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作者：
J. Kunz;D. Maison;F. Navarro-Lérida;J. Viebahn
通过在D+1维中嵌入D维MyersPerry解，并在随后的⩾约化过程中进行加速，我们构造了D时空维爱因斯坦-麦克斯韦伸缩理论中的精确带电旋转黑洞。像迈尔斯-佩里解一样，这些黑洞一般具有N=[(D−1)/2]独立的角动量。我们给出了这些黑洞的整体性质和视界性质，并讨论了它们的存在范围。
We construct exact charged rotating black holes in Einstein–Maxwell–dilaton theory in D spacetime dimensions, D⩾5, by embedding the D-dimensional Myers–Perry solutions in D+1 dimensions, and performing a boost with a subsequent Kaluza–Klein reduction. Like the Myers–Perry solutions, these black holes generically possess N=[(D−1)/2] independent angular momenta. We present the global and horizon properties of these black holes, and discuss their domains of existence.