Jackiw-Teitelboim gravity with matter, generalized eigenstate thermalization hypothesis, and random matrices

被引:28
作者
Jafferis, Daniel Louis [1 ]
Kolchmeyer, David K. [1 ,2 ]
Mukhametzhanov, Baur [3 ,4 ]
Sonner, Julian [5 ]
机构
[1] Harvard Univ, Dept Phys, Cambridge, MA 02138 USA
[2] MIT, Ctr Theoret Phys, Cambridge, MA 02139 USA
[3] Inst Adv Study, Princeton, NJ 08540 USA
[4] Cornell Univ, Dept Phys, Ithaca, NY 14853 USA
[5] Univ Geneva, Dept Theoret Phys, Geneva, Switzerland
基金
美国国家科学基金会;
关键词
D O I
10.1103/PhysRevD.108.066015
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present evidence for a duality between Jackiw-Teitelboim gravity minimally coupled to a free massive scalar field and a single-trace two-matrix model. One matrix is the Hamiltonian H of a holographic disorder-averaged quantum mechanics, while the other matrix is the light operator O dual to the bulk scalar field. The single-boundary observables of interest are thermal correlation functions of O. We study the matching of the genus zero-, one- and two-boundary expectation values in the matrix model to the disk and cylinder Euclidean path integrals. The non-Gaussian statistics of the matrix elements of O correspond to a generalization of the eigenstate thermalization hypothesis ansatz. We describe multiple ways to construct double-scaled matrix models that reproduce the gravitational disk correlators. One method involves imposing an operator equation obeyed by H and O as a constraint on the two matrices. Separately, we design a model that reproduces certain double-scaled Sachdev-Ye-Kitaev correlators that may be scaled once more to obtain the disk correlators. We show that in any single-trace, two-matrix model, the genus zero two-boundary expectation value, with up to one O insertion on each boundary, can be computed directly from all of the genus zero one-boundary correlators. Applied to the models of interest, we find that these cylinder observables depend on the details of the double-scaling limit. To the extent we have checked, it is possible to reproduce the gravitational double-trumpet, which is UV divergent, from a systematic classification of matrix model 't Hooft diagrams. The UV divergence indicates that the matrix integral saddle of interest is perturbatively unstable. A nonperturbative treatment of the matrix models discussed in this work is left for future investigations.
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页数:90
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