Leading and beyond leading-order spectral form factor in chaotic quantum many-body systems across all Dyson symmetry classes
arXiv:2502.04152
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), , up to two leading orders in time, . We explicitly consider the presence or absence of time reversal () symmetry to investigate all three Dyson's symmetry classes. Our derivation only assumes random phase approximation to enable ensemble average. For -invariant systems with , we show that beyond the Thouless time , the SFF takes the form up to second order in time, where is the Hilbert space dimension. This is identical to the result from circular orthogonal ensemble of RMT. In the absence of -symmetry, we show that beyond , and there is no universal term in the second order, unlike the case, in agreement with the result of circular unitary ensemble. For -invariant systems with , we show that up to two orders in time beyond , in agreement with the result of circular symplectic ensemble. In all three cases, the system-size, , scaling of is determined by eigenvalues of a doubly stochastic matrix . For strongly interacting fermionic chains, is invariant in all three cases, leading to in the presence of symmetry. In the absence of symmetry, we find , due to gapped non-degenerate second-largest eigenvalue of or due to gapped second-largest eigenvalue with degeneracy . Our calculation of SFF is plausible in higher space dimensions as well, where similar system-size scalings of can be obtained.