Fast scrambling of mutual information in Kerr-AdS4 spacetime

被引:5
|
作者
Malvimat, Vinay [1 ]
Poojary, Rohan R. [2 ]
机构
[1] Homi Bhaba Natl Inst HBNI, Saha Inst Nucl Phys, Theory Div, 1-AF, Bidhannagar, Kolkata 700064, India
[2] TU Wien, Inst Theoret Phys, Wiedner Hauptstr 8-10, A-1040 Vienna, Austria
关键词
D O I
10.1103/PhysRevD.107.026019
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We compute the disruption of mutual information between the hemispherical subsystems on the left and right conformal field theories of a thermofield double state described by a Kerr geometry in AdS4 due to shock waves along the equatorial plane. The shock waves and the subsystems considered respect the axisymmetry of the geometry. At late times, the disruption of the mutual information is given by the lengthening of the Hubeny-Rangamani-Takayanagi surface connecting the two subsystems; we compute the minimum value of the Lyapunov index-lambda(min)Lat late times and find that it is bounded by kappa = 2 pi TH (1-mu L), where mu is the horizon velocity, and L is the angular momentum per unit energy of the shock wave. At very late times, we find the scrambling time for such a system is governed by kappa with kappa t* = log S for large black holes with a large entropy S. We also find a term that increases the scrambling time by log(1 - mu L)-1 but which does not scale with the entropy of the Kerr geometry.
引用
收藏
页数:16
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