On Quantum Microstates in the Near Extremal, Near Horizon Kerr Geometry

被引:2
|
作者
Guneratne, A. [1 ]
Rodriguez, L. [2 ]
Wickramasekara, S. [1 ,3 ]
Yildirim, T. [4 ]
机构
[1] Univ Iowa, Dept Phys & Astron, Iowa City, IA 52242 USA
[2] Assumption Coll, Dept Phys, Worcester, MA 01609 USA
[3] Grinnell Coll, Dept Phys, Grinnell, IA 50112 USA
[4] Arizona State Univ, Dept Phys, Tempe, AZ 85287 USA
来源
QUANTUM FEST 2015 | 2016年 / 698卷
关键词
CONFORMAL FIELD-THEORY; BLACK-HOLE ENTROPY; GRAVITATIONAL ANOMALIES; HAWKING RADIATION;
D O I
10.1088/1742-6596/698/1/012010
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
We study the thermodynamics of near horizon near extremal Kerr (NHNEK) geometry within the framework of AdS(2)/CFT1 correspondence. We start by shifting the horizon of near horizon extremal Kerr (NHEK) geometry by a general finite mass. While this shift does not alter the geometry in that the resulting classical solution is still diffeomorphic to the NHEK solution, it does lead to a quantum theory different from that of NHEK. We obtain this quantum theory by means of a Robinson-Wilczek two-dimensional Kaluza-Klein reduction which enables us to introduce a finite regulator on the AdS(2) boundary and compute the full asymptotic symmetry group of the two-dimensional quantum conformal field theory on the respective AdS(2) boundary. The s-wave contribution of the energy-momentum-tensor of this conformal field theory, together with the asymptotic symmetries, generate a Virasoro algebra with a calculable center, which agrees with the standard Kerr/CFT result, and a non-vanishing lowest Virasoro eigenmode. The central charge and lowest eigenmode produce the Bekenstein-Hawking entropy and Hawking temperature for NHNEK.
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页数:11
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