Abstract

We argue that “stringy” effects in a putative gravity-dual picture for SYK-like models are related to the branching time, a kinetic coefficient defined in terms of the retarded kernel. A bound on the branching time is established assuming that the leading diagrams are ladders with thin rungs. Thus, such models are unlikely candidates for sub-AdS holography. In the weak coupling limit, we derive a relation between the branching time, the Lyapunov exponent, and the quasiparticle lifetime using two different approximations.

Highlights

  • We present a proof of the Lemma stated in the main text

  • The lemma asserts a bound on the rate of phase winding for the retarded and advanced fermionic Green functions

  • Our goal is to find a bound on the derivative of f (z) at z0 = ω + is

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Summary

Outline of the paper

The remainder of this paper is organized as follows. It is derived by relating the branching time to the winding speed of the phase of the Green function. The required upper bound for the winding speed is proved in appendix B.

Preliminaries
Rung function in SYK-like models
Kinetic equation in the frequency domain
Branching time and a generating function
A bound on the branching time
Branching time at weak coupling
A bound state problem
Comments on various approximation methods
Summary and discussion
A An alternative derivation of the ladder identity
B Proof of the Lemma
C Keldysh formalism for multiple contour folds
Green function in the Keldysh basis
Diagrammatic rules
Quasiparticle decay rate Γ for SYK at weak coupling
E Branching time for Brownian SYK
F Branching time for the regular SYK model at large q
Full Text
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