Machine learning Green's functions of strongly correlated Hubbard models.

We demonstrate that a machine learning framework based on kernel ridge regression can encode and predict the self-energy of one-dimensional Hubbard models using only mean-field features such as static and dynamic Hartree-Fock quantities and first-orderGWcalculations. This approach is applicable across a wide range of on-site Coulomb interaction strengthsU/t, ranging from weakly interacting systems (U/t < 1) to strong correlations (U/t > 8). The predicted self-energy is transformed via Dyson's equation and analytic continuation to obtain the real-frequency Green's function, which allows access to the spectral function and density of states. This method can be used for nearest-neighbor interactionstand long-range hopping termst',t'', andt'''.