Thermalization of Strongly Coupled Field Theories

被引:266
作者
Balasubramanian, V. [1 ]
Bernamonti, A. [2 ,3 ]
de Boer, J. [4 ]
Copland, N. [2 ,3 ]
Craps, B. [2 ,3 ]
Keski-Vakkuri, E. [5 ,6 ]
Mueller, B. [7 ,8 ]
Schaefer, A. [9 ]
Shigemori, M. [10 ]
Staessens, W. [2 ,3 ]
机构
[1] Univ Penn, David Rittenhouse Lab, Philadelphia, PA 19104 USA
[2] Vrije Univ Brussel, B-1050 Brussels, Belgium
[3] Int Solvay Inst, B-1050 Brussels, Belgium
[4] Univ Amsterdam, Inst Theoret Phys, NL-1090 GL Amsterdam, Netherlands
[5] Univ Helsinki, Helsinki Inst Phys, FIN-00014 Helsinki, Finland
[6] Univ Helsinki, Dept Phys, FIN-00014 Helsinki, Finland
[7] Duke Univ, Dept Phys, Durham, NC 27708 USA
[8] Duke Univ, CTMS, Durham, NC 27708 USA
[9] Univ Regensburg, Inst Theoret Phys, D-93040 Regensburg, Germany
[10] Nagoya Univ, Kobayashi Maskawa Inst Origin Particles & Univers, Nagoya, Aichi 4648602, Japan
基金
芬兰科学院;
关键词
METRIC INVARIANT; ENTROPY; MATTER;
D O I
10.1103/PhysRevLett.106.191601
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
Using the holographic mapping to a gravity dual, we calculate 2-point functions, Wilson loops, and entanglement entropy in strongly coupled field theories in d = 2, 3, and 4 to probe the scale dependence of thermalization following a sudden injection of energy. For homogeneous initial conditions, the entanglement entropy thermalizes slowest and sets a time scale for equilibration that saturates a causality bound. The growth rate of entanglement entropy density is nearly volume-independent for small volumes but slows for larger volumes. In this setting, the UV thermalizes first.
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页数:4
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