Quantum oscillations and black hole ringing

被引:103
作者
Denef, Frederik [1 ,2 ,3 ]
Hartnoll, Sean A. [1 ,2 ]
Sachdev, Subir [1 ,2 ]
机构
[1] Harvard Univ, Dept Phys, Cambridge, MA 02138 USA
[2] Univ Calif Santa Barbara, Kavli Inst Theoret Phys, Santa Barbara, CA 93106 USA
[3] Katholieke Univ Leuven, Inst Theoret Fys, B-3001 Louvain, Belgium
来源
PHYSICAL REVIEW D | 2009年 / 80卷 / 12期
基金
美国国家科学基金会;
关键词
QUASI-NORMAL MODES; FERMI-SURFACE; WAVE-PROPAGATION;
D O I
10.1103/PhysRevD.80.126016
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We show that strongly coupled field theories with holographic gravity duals at finite charge density and low temperatures can undergo de Haas-van Alphen quantum oscillations as a function of an external magnetic field. Exhibiting this effect requires computation of the one-loop contribution of charged bulk fermions to the free energy. The one-loop calculation is performed using a formula expressing determinants in black hole backgrounds as sums over quasinormal modes. At zero temperature, the periodic nonanalyticities in the magnetic susceptibility as a function of the inverse magnetic field depend on the low energy scaling behavior of fermionic operators in the field theory, and are found to be softer than in weakly coupled theories. We also obtain numerical and WKB results for the quasinormal modes of charged bosons in dyonic black hole backgrounds, finding evidence for nontrivial periodic behavior as a function of the magnetic field.
引用
收藏
页数:25
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