Complexity as a holographic probe of strong cosmic censorship

被引:3
作者
Alishahiha, Mohsen [1 ]
Banerjee, Souvik [2 ]
Kames-King, Joshua [3 ,4 ,5 ]
Loos, Emma [2 ]
机构
[1] Inst Res Fundamental Sci IPM, Sch Phys, POB 19395-5531, Tehran, Iran
[2] Julius Maximilians Univ Wurzburg, Inst Theoret Phys & Astrophys, D-97074 Wurzburg, Germany
[3] Univ Bonn, Bethe Ctr Theoret Phys, Nussallee 12, D-53115 Bonn, Germany
[4] Univ Bonn, Phys Inst, Nussallee 12, D-53115 Bonn, Germany
[5] Univ Calif Santa Barbara, Kavli Inst Theoret Phys, Santa Barbara, CA 93106 USA
基金
美国国家科学基金会;
关键词
D O I
10.1103/PhysRevD.105.026001
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Based on reasonable assumptions, we propose a new expression for Lloyd's bound, which confines the complexity growth of charged black holes. We then revisit holographic complexity for charged black branes in the presence of a finite cutoff. Using the proposed Lloyd's bound we find a relation between the UV and the behind the horizon cutoff. This is found to be consistent with the factorization of the partition function at leading order in large N. We argue that the result may be thought of as a holographic realization of strong cosmic censorship.
引用
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页数:14
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