Feed-forward neural network based variational wave function for the fermionic Hubbard model in one dimension

We explore the suitability of a feed-forward neural network (FNN) to represent the ground state of the fermionic Hubbard model in one dimension (1D). We consider the model at half-filling, represent the ground state wave function in terms of an FNN and optimize it using the variational Monte Carlo (VMC) method. The results are compared with the exact Bethe Ansatz solution. We find that for lattice sizes which give a 'filled-shell' condition for the non-interacting Fermi sea wave function, a simple FNN performs very well at all values of Hubbard interactionU. For lattice sizes where this condition is not obtained, the simple FNN fails and we find a modified network with a 'sign' component (sFNN) to work in such cases. On the flip side, though we find the FNN to be successful in providing an unbiased variational wave function for the fermionic many-body system in 1D, the computational cost for the wave function scales up rapidly with lattice size which limits its applicability.