Abstract

We investigate the magnetic shell structure of repulsively interacting two-component Fermi gases trapped in a two-dimensional harmonic potential and loaded on the optical Lieb lattices. We employ the real-space dynamical mean-field theory (R-DMFT) to explicitly consider the trap potential in a self-consistent way. Computing the profiles of particle density and local magnetization across the lattice sites in the trap, we find that the incompressible core with ferrimagnetic ordering appears with the density plateau at the trap center, which is surrounded by the shell of the normal metallic phase. We examine the incompressibility of the core by adding more particles and creating the higher spin-population imbalance. While the core area expands from the outer shell with added particles and increased polarization, the excess particles are prohibited from going inside the core, and thus the density plateau is unchanged at the half-filling with the same magnetic ordering. In addition, we find that the feature of the phase separation differs with the sublattices, where the interstitial sites causing the flat band dispersion shows the signature of the abrupt transition in the density and magnetization at the boundary between the core and surrounding shells.

Highlights

  • IntroductionUltracold Fermi gases have attracted much attention because of its potential as an ideal test bed of condensed matter phenomena that can simulate or emulate a designed quantum many-bodyHamiltonian in highly controllable environments [1,2,3,4,5]

  • Ultracold Fermi gases have attracted much attention because of its potential as an ideal test bed of condensed matter phenomena that can simulate or emulate a designed quantum many-bodyHamiltonian in highly controllable environments [1,2,3,4,5]

  • We have investigated the flat-band ferromagnetism in the Hubbard model of repulsively interacting Fermi gases confined in a harmonic trap and loaded on the optical Lieb lattices by using the real-space dynamical mean-field theory

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Summary

Introduction

Ultracold Fermi gases have attracted much attention because of its potential as an ideal test bed of condensed matter phenomena that can simulate or emulate a designed quantum many-bodyHamiltonian in highly controllable environments [1,2,3,4,5]. The pseudospin components of the fermionic atom are given by its hyperfine states of which two are typically used in the popular systems of 6 Li or 40 K atoms, providing the up-spin and down-spin species of fermions. The scattering between these two-component fermionic atoms can be controlled by using the Feshbach resonance [9], providing a way to tune the particle–particle interaction to be attractive or repulsive. The seminal experiments [11,12] realizing the repulsive Hubbard model demonstrated the Mott-insulating phase of the Fermi gases in cubic optical lattices in a trap by examining the bulk compressibility of the atomic cloud. Theoretical calculations using the real-space dynamical mean-field theory [13] found that the Mott-insulating core appeared with the plateau in the density profile in the three-dimensional trap

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