$N=2$ JT Supergravity and Matrix Models
Gustavo J. Turiaci, Edward Witten
TL;DR
This work establishes a precise holographic duality between ${ t N}=2$ JT supergravity on asymptotically AdS${}_2$ spaces and a family of independent ${ t N}=2$ random-matrix ensembles, one for each $R$-charge multiplet. By extending Mirzakhani’s recursion to ${ t N}=2$ hyperbolic surfaces and deriving the corresponding measure via torsion, the authors show that gravity loop equations match random-matrix loop equations for an AZ$(1,2)$ ensemble, validating the duality to all orders in the topological expansion. They analyze the disk, cylinder, and three-holed sphere, compute the leading black-hole spectrum, and identify how BPS states contribute discretely while non-BPS sectors yield continuous densities governed by the spectral curve $y_q(x)$. Time-reversal symmetry (both ${ t T}$ and ${ t CT}$) is incorporated, with detailed matrix-model predictions for crosscaps and unorientable geometries, including anomalies and possible deformations via defects. The paper also sketches extensions to ${ t N}=4$ JT gravity, where the multiplets remain statistically independent and the dual random-matrix description persists, providing a comprehensive framework linking Jackiw–Teitelboim supergravity, topological recursion, and random-matrix theory in a supersymmetric setting.
Abstract
Generalizing previous results for $N=0$ and $N=1$, we analyze $N=2$ JT supergravity on asymptotically AdS${}_2$ spaces with arbitrary topology and show that this theory of gravity is dual, in a holographic sense, to a certain random matrix ensemble in which supermultiplets of different $R$-charge are statistically independent and each is described by its own $N=2$ random matrix ensemble. We also analyze the case with a time-reversal symmetry, either commuting or anticommuting with the $R$-charge. In order to compare supergravity to random matrix theory, we develop an $N=2$ analog of the recursion relations for Weil-Petersson volumes originally discovered by Mirzakhani in the bosonic case.
