Characterizing the antiferromagnetic ordering of fermions in a compensated optical lattice

POSTER

Abstract

We realize the Fermi-Hubbard model with fermionic $^{6}$Li atoms in a three-dimensional, red-detuned optical lattice. The lattice is compensated by the addition of three blue-detuned gaussian beams which overlap each of the lattice laser beams, but are not retro-reflected. Using the compensated lattice potential, we have reached temperatures low enough to produce antiferromagnetic (AF) spin correlations, which we detect via Bragg scattering of light. The variation of the measured AF correlations as a function of the Hubbard interaction strength, $U/t$, provides a way to determine the temperature of the atoms in the lattice by comparison with quantum Monte Carlo calculations. This method suggests our temperature is in the range of 2-3 times the N\'{e}el ordering temperature. In this poster we present our Bragg scattering results along with our studies of the effect of the compensating potential in helping us cool the atoms in the lattice and also enlarge the size of the AF phase.\footnote{C. J. M. Mathy et al., Phys. Rev. A \textbf{86}, 023606 (2011)}

Authors

  • P.M. Duarte

    Department of Physics and Astronomy and Rice Quantum Institute, Rice University, Houston TX, Department of Physics and Astronomy and Rice Quantum Institute, Rice University, Houston, TX 77005

  • R.A. Hart

    Department of Physics and Astronomy and Rice Quantum Institute, Rice University, Houston TX

  • T.L. Yang

    Department of Physics and Astronomy and Rice Quantum Institute, Rice University, Houston TX, Department of Physics and Astronomy and Rice Quantum Institute, Rice University, Houston, TX 77005

  • X. Liu

    Department of Physics and Astronomy and Rice Quantum Institute, Rice University, Houston TX, Department of Physics and Astronomy and Rice Quantum Institute, Rice University, Houston, TX 77005

  • Randall Hulet

    Rice University, Department of Physics and Astronomy and Rice Quantum Institute, Rice University, Houston TX, Department of Physics and Astronomy and Rice Quantum Institute, Rice University, Houston, TX 77005

  • T.C.L. Paiva

    Instituto de Fisica, Universidade Federal do Rio de Janeiro, Rio de Janeiro RJ, Brazil, Instituto de Fisica, Universidade Federal do Rio de Janeiro Cx.P. 68.528, 21941-972 Rio de Janeiro RJ, Brazil

  • D. Huse

    Department of Physics, Princeton University, Princeton NJ, Department of Physics, Princeton University, Princeton, New Jersey 08544

  • R. Scalettar

    Department of Physics, University of California, Davis, CA

  • N. Trivedi

    Department of Physics, The Ohio State University, Columbus OH