Generalized near horizon extreme binary black hole geometry
Generalized near horizon extreme binary black hole geometry
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DOI：
10.1103/physrevd.100.044033
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发表时间：
2019-06
影响因子：
5
通讯作者：
J. Ciafre;Shahar Hadar;Erin Rickenbach;Maria J Rodriguez
中科院分区：
文献类型：
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作者：
J. Ciafre;Shahar Hadar;Erin Rickenbach;Maria J Rodriguez
我们提出了一个新的真空解决方案的爱因斯坦方程描述近视界区的两个中性，极端（零温度），同向旋转，不同的克尔黑洞。度规是固定的，渐近接近视界极值克尔（NHEK），并包含一个本地化的无质量支柱沿着黑洞之间的对称轴。在深红外线中，它流向两个独立的喉道，我们称之为“刺穿的NHEK”几何：每个喉道都是被锥形奇点刺穿的NHEK。我们发现，尽管存在的支柱穿刺NHEK几何的等距群SL（2，R）xU（1）的恢复。我们找到物理参数和熵。
We present a new vacuum solution of Einstein's equations describing the near horizon region of two neutral, extreme (zero-temperature), co-rotating, non-identical Kerr black holes. The metric is stationary, asymptotically near horizon extremal Kerr (NHEK), and contains a localized massless strut along the symmetry axis between the black holes. In the deep infrared, it flows to two separate throats which we call "pierced-NHEK" geometries: each throat is NHEK pierced by a conical singularity. We find that in spite of the presence of the strut for the pierced-NHEK geometries the isometry group SL(2,R)xU(1) is restored. We find the physical parameters and entropy.