Abstract

By employing the mean field and variational Monte Carlo methods, we investigate the iron-based superconductors (FeSCs) based on a realistic five-orbital Hubbard model in which an off-site Coulomb interaction is explicitly included. Our results demonstrate that plays an important role in stabilizing the nematic state in both Fe-pnictides and FeSe. Below a critical , the model is shown to lie in the striped antiferromagnetic ground state, and an increasing of leads to an energy degeneracy between different magnetic configurations. This finding provides a natural explanation for the magnetism in Fe-pnictides with relatively small , and more importantly, unveils the microscopic mechanism behind the absence of magnetic order in FeSe with larger . Simultaneously, the common anisotropy of and orbital occupations in different magnetic configurations accounts for the similar orbital ordering observed in Fe-pnictides and FeSe. In addition, the unusual smallness of the Fermi surfaces in FeSe can be obtained when the renormalization effect of on the band structure is taken into account.

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