Maximizing the Neel temperature of fermions in a simple-cubic optical lattice
C.J.M. Mathy, David A. Huse

TL;DR
This paper investigates how to maximize the Neel temperature in a fermionic optical lattice by analyzing the effects of interactions and model approximations, focusing on the Hubbard model's limitations.
Contribution
It identifies the conditions near the Hubbard model's validity limit that optimize the Neel temperature, highlighting the impact of direct ferromagnetic interactions.
Findings
Maximum Neel temperature occurs near the Hubbard model's edge.
Direct ferromagnetic interactions limit the Neel temperature.
Corrections to the Hubbard model are crucial for understanding magnetic ordering.
Abstract
For a simple-cubic optical lattice with lattice spacing d, occupied by two species of fermionic atoms of mass m that interact repulsively, we ask what conditions maximize the Neel temperature in the Mott insulating phase at density one atom per site, with equal numbers of the two species. This maximum occurs near the edge of the regime where the system is well-approximated by the usual Hubbard model. The correction to the Hubbard-model approximation that produces a "direct" ferromagnetic interaction between atoms in nearest-neighbor Wannier orbitals is the leading term that limits how high the Neel temperature can be made.
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