Leading and beyond leading-order spectral form factor in chaotic quantum many-body systems across all Dyson symmetry classes
Vijay Kumar, Tomaž Prosen, Dibyendu Roy
TL;DR
This work presents a unified, analytic framework to derive the spectral form factor (SFF) for generic chaotic, periodically driven many-body quantum systems across all Dyson circular ensembles (COE, CUE, CSE) using random phase averaging (RPA). By decomposing SFF contributions into X, Y, and Z-type diagrams and introducing reduced diagrams, the authors isolate universal (Type I) terms that reproduce RMT predictions beyond the Thouless time t*, while nonuniversal (Type II/III) terms either cancel or decay, respectively. They show t* is set by the second-largest eigenvalue of a doubly stochastic matrix M that encodes phase-space returns, with distinct system-size scalings depending on U(1) symmetry. The results extend to higher dimensions and provide explicit leading- and second-order SFF corrections, unveiling a mechanism for the universal emergence of RMT statistics in strongly interacting quantum chaos. The findings have potential experimental relevance for measuring SFF and spectral correlations in quantum simulators and cold-atom platforms.
Abstract
We show the emergence of random matrix theory (RMT) spectral correlations in the chaotic phase of generic periodically kicked interacting quantum many-body systems by analytically calculating spectral form factor (SFF), $K(t)$, up to two leading orders in time, $t$. We explicitly consider the presence or absence of time reversal ($\mathcal{T}$) symmetry to investigate all three Dyson's symmetry classes. Our derivation only assumes random phase approximation to enable ensemble average. For $\mathcal{T}$-invariant systems with $\mathcal{T}^2=1$, we show that beyond the Thouless time $t^*$, the SFF takes the form $K(t)\simeq 2t-2t^2/\mathcal{N}$ up to second order in time, where $\mathcal{N}$ is the Hilbert space dimension. This is identical to the result from circular orthogonal ensemble of RMT. In the absence of $\mathcal{T}$-symmetry, we show that $K(t)\simeq t$ beyond $t^*$, and there is no universal term in the second order, unlike the $\mathcal{T}^2=1$ case, in agreement with the result of circular unitary ensemble. For $\mathcal{T}$-invariant systems with $\mathcal{T}^2=-1$, we show that $K(t)\simeq 2t+2t^2/\mathcal{N}$ up to two orders in time beyond $t^*$, in agreement with the result of circular symplectic ensemble. In all three cases, the system-size, $L$, scaling of $t^*$ is determined by eigenvalues of a doubly stochastic matrix $\mathcal{M}$. For strongly interacting fermionic chains, $\mathcal{M}$ is $SU(2)$ invariant in all three cases, leading to $t^*\propto L^2$ in the presence of $U(1)$ symmetry. In the absence of $U(1)$ symmetry, we find $t^*\propto L^0$, due to gapped non-degenerate second-largest eigenvalue of $\mathcal{M}$ or $t^*\propto \ln(L)$ due to gapped second-largest eigenvalue with degeneracy $\propto L^ζ$. Our calculation of SFF is plausible in higher space dimensions as well, where similar system-size scalings of $t^*$ can be obtained.
