No dynamics in the extremal Kerr throat

被引:83
作者
Amsel, Aaron J. [1 ]
Horowitz, Gary T. [1 ]
Marolf, Donald [1 ]
Roberts, Matthew M. [1 ]
机构
[1] Univ Calif Santa Barbara, Dept Phys, Santa Barbara, CA 93106 USA
来源
JOURNAL OF HIGH ENERGY PHYSICS | 2009年 / 09期
基金
美国国家科学基金会;
关键词
Gauge-gravity correspondence; Black Holes; Space-Time Symmetries; ROTATING BLACK-HOLE; LINEARIZATION STABILITY; PERTURBATIONS; SYMMETRIES; UNIQUENESS; EQUATIONS; ENERGY; SPACE; FIELD; TENSOR;
D O I
10.1088/1126-6708/2009/09/044
中图分类号
O412 [相对论、场论]; O572.2 [粒子物理学];
学科分类号
摘要
Motivated by the Kerr/CFT conjecture, we explore solutions of vacuum general relativity whose asymptotic behavior agrees with that of the extremal Kerr throat, sometimes called the Near-Horizon Extreme Kerr (NHEK) geometry. We argue that all such solutions are diffeomorphic to the NHEK geometry itself. The logic proceeds in two steps. We first argue that certain charges must vanish at all times for any solution with NHEK asymptotics. We then analyze these charges in detail for linearized solutions. Though one can choose the relevant charges to vanish at any initial time, these charges are not conserved. As a result, requiring the charges to vanish at all times is a much stronger condition. We argue that all solutions satisfying this condition are diffeomorphic to the NHEK metric.
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页数:35
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