Complexity geometry and Schwarzian dynamics

被引:13
|
作者
Lin, Henry W. [1 ,4 ]
Susskind, Leonard [2 ,3 ,4 ]
机构
[1] Princeton Univ, Jadwin Hall, Princeton, NJ 08540 USA
[2] Stanford Univ, Stanford Inst Theoret Phys, Stanford, CA 94305 USA
[3] Stanford Univ, Dept Phys, Stanford, CA 94305 USA
[4] Google, Mountain View, CA 94043 USA
基金
美国国家科学基金会;
关键词
2D Gravity; AdS-CFT Correspondence;
D O I
10.1007/JHEP01(2020)087
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
A celebrated feature of SYK-like models is that at low energies, their dynamics reduces to that of a single variable. In many setups, this "Schwarzian" variable can be interpreted as the extremal volume of the dual black hole, and the resulting dynamics is simply that of a 1D Newtonian particle in an exponential potential. On the complexity side, geodesics on a simplified version of Nielsen's complexity geometry also behave like a 1D particle in a potential given by the angular momentum barrier. The agreement between the effective actions of volume and complexity succinctly summarizes various strands of evidence that complexity is closely related to the dynamics of black holes.
引用
收藏
页数:19
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