Abstract

We investigate the supersymmetric Sachdev-Ye-Kitaev (SYK) model, $N$ Majorana fermions with infinite range interactions in $0+1$ dimensions. We have found that, close to the ground state $E \approx 0$, discrete symmetries alter qualitatively the spectral properties with respect to the non-supersymmetric SYK model. The average spectral density at finite $N$, which we compute analytically and numerically, grows exponentially with $N$ for $E \approx 0$. However the chiral condensate, which is normalized with respect the total number of eigenvalues, vanishes in the thermodynamic limit. Slightly above $E \approx 0$, the spectral density grows exponential with the energy. Deep in the quantum regime, corresponding to the first $O(N)$ eigenvalues, the average spectral density is universal and well described by random matrix ensembles with chiral and superconducting discrete symmetries. The dynamics for $E \approx 0$ is investigated by level fluctuations. Also in this case we find excellent agreement with the prediction of chiral and superconducting random matrix ensembles for eigenvalues separations smaller than the Thouless energy, which seems to scale linearly with $N$. Deviations beyond the Thouless energy, which describes how ergodicity is approached, are universality characterized by a quadratic growth of the number variance. In the time domain, we have found analytically that the spectral form factor $g(t)$, obtained from the connected two-level correlation function of the unfolded spectrum, decays as $1/t^2$ for times shorter but comparable to the Thouless time with $g(0)$ related to the coefficient of the quadratic growth of the number variance. Our results provide further support that quantum black holes are ergodic and therefore can be classified by random matrix theory.

Highlights

  • Random matrix theory [1,2,3,4,5,6] is a powerful tool to explain universal features of complex quantum systems

  • We have found that the microscopic spectral density corresponding to the OðNÞ smallest eigenvalues is universal, and is well described by chiral or superconducting random matrix ensembles depending on the value of N

  • The chiral condensate, obtained from the spectral resolvent, which is normalized with respect to the total number of eigenvalues, vanishes in the thermodynamic limit

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Summary

INTRODUCTION

Random matrix theory [1,2,3,4,5,6] is a powerful tool to explain universal features of complex quantum systems. Since global symmetries of the non-supersymmetric model match those of the standard Wigner-Dyson ensembles, the random matrix correspondence of the supersymmetric SYK model extends this to most of the known [62] universality classes in random matrix theory This raises several questions: do SYK models with different global symmetries still keep most of the features expected in a theory with gravity dual such as quantum chaos, exponential increase of low energy excitations or a finite entropy at zero temperature? Our main results are that this chiral SYK model still has all the expected features of a gravity dual: finite entropy at zero temperature, exponential increase of low energy excitations and excellent agreement of level statistics with random matrix theory predictions for sufficiently long time or small energy separations. In Appendix A we work out the large N limit of the Q-Hermite result for the spectral density while a simple analytical form for the resolvent of the SYK model is obtained in Appendix B

The SYK model
The spectral density of the supercharge
The resolvent
Thermodynamic properties
UNIVERSAL MICROSCOPIC SPECTRAL DENSITY
Spectral form factor
OUTLOOK, HOLOGRAPHIC INTERPRETATION AND CONCLUSIONS
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