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 the 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 symmetry classes, namely, the circular orthogonal ensemble (COE) for -invariant systems with , the circular unitary ensemble (CUE) in the absence of symmetry, and the circular symplectic ensemble (CSE) for -invariant systems with . Our derivation applies the random phase approximation to perform ensemble averages, and we give its justification for generic many-body interactions. We express the SFF as a sum of contributions of certain diagrams. While the number of diagrams that contribute to the SFF in the first and second orders in for the COE and CUE classes is finite, the number of such diagrams is exponentially large in for the CSE class. Thus, we have developed a new diagrammatic technique that uses reduced diagrams to incorporate contributions from many diagrams. For the COE class, we show that beyond Thouless time , the SFF takes the form up to second order in time, where is the Hilbert space dimension. For the CUE class, we show that beyond , and there is no universal term in the second order, unlike the COE case. For the CSE class, we show that up to two orders in time beyond . The above findings of the SFF up to second order in time are in agreement with the RMT predictions for these classes. In all three cases, the scaling of with system size is determined by the 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 the gapped, nondegenerate, second-largest eigenvalue of , or , due to the gapped second-largest eigenvalue with degeneracy proportional to , . Our calculation of the SFF is plausible in higher space dimensions as well, where similar system-size scalings of can be obtained.