Jackiw-Teitelboim gravity with matter, generalized eigenstate thermalization hypothesis, and random matrices
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 $\mathcal{O}$ d...
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Veröffentlicht in: | Physical review. D 2023-09, Vol.108 (6), Article 066015 |
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Sprache: | eng |
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Zusammenfassung: | 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 $\mathcal{O}$ dual to the bulk scalar field. The single-boundary observables of interest are thermal correlation functions of $\mathcal{O}$. 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 $\mathcal{O}$ 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 $\mathcal{O}$ 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 $\mathcal{O}$ 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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ISSN: | 2470-0010 2470-0029 |
DOI: | 10.1103/PhysRevD.108.066015 |