Extremal isolated horizon/CFT correspondence

Extremal isolated horizon/CFT correspondence
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极值孤立层位/CFT对应

DOI:
10.1103/physrevd.80.024014
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发表时间:
2009-04
期刊:
影响因子:
5
通讯作者:
Wu, Xiao-Ning
Wu, Xiao-Ning
中科院分区:
物理与天体物理2区
文献类型:
--
作者:
Tian, Yu;Wu, Xiao-Ning

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在类Bondi坐标下,得到了极值(弱)孤立视界的近视界极限。在真空情形下,得到了类Bondi坐标系下的近视界度规与极值Kerr黑洞的标准Poincare型或整体近视界度规之间的显式坐标变换,表明这两种几何是相同的.结合已知的(弱)孤立视界的热力学,我们认为Kerr/共形场论对应可以推广到一大类非稳态极值黑洞的情况。
The near-horizon limit of the extremal (weakly) isolated horizon is obtained under the Bondi-like coordinates. For the vacuum case, explicit coordinate transformation relating the near-horizon metric under the Bondi-like coordinates and the standard Poincare-type or global near-horizon metric of the extremal Kerr black hole is found, which shows that the two geometries are the same. Combined with the known thermodynamics of the (weakly) isolated horizon, it is argued that the Kerr/conformal field theory correspondence can be generalized to the case of a large class of nonstationary extremal black holes.
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