Three-Orbital Spin-Fermion Model for CuO2 Planes

ORAL

Abstract

High Tc superconducting cuprates have been studied using single orbital Hubbard or t-J models because numerical studies of more realistic multiorbital Hamiltonians could not be done in sufficiently large systems. The use of these simplified models was justified by the experimental observation of a single band Fermi surface. However, the single band models are Mott insulators in the undoped state while it is well-known that the parent compound of the cuprates are charge-transfer insulators. The discovery of the iron-based superconductors brought to the forefront the need to develop models and numerical approaches for multiorbital systems. Thus, effective multiorbital spin-fermion models were developed [1] that allowed the study of many properties of these materials. A spin-fermion model for the CuO2 planes of the cuprates will be presented.[2] Using techniques developed for the pnictides results will be presented for magnetic and charge ordering, pairing tendencies, spectral functions and density of states as a function of temperature and doping. Comparisons with experimental data for the real materials and numerical results for single orbital models will be presented.

[1] S. Liang et al., Phys. Rev. Lett. 109, 047001 (2012).
[2] M. Hussein et al., in preparation.

Presenters

  • Mostafa Hussein

    Department of Physics and Astronomy, University of Tennessee, Knoxville

Authors

  • Mostafa Hussein

    Department of Physics and Astronomy, University of Tennessee, Knoxville

  • Christopher Bishop

    Department of Physics and Astronomy, University of Tennessee, Knoxville

  • Elbio Dagotto

    Univ. of Tennessee, Physics and Astronomy, University of Tennessee, Department of Physics and Astronomy, Univ of Tennessee, Knoxville, Department of Physics and Astronomy, University of Tennessee, University of Tennessee, University of Tennessee & Oak Ridge National Laboratory, Department of Physics and Astronomy, University of Tennessee, Knoxville

  • Adriana Moreo

    Univ. of Tennessee, Department of Physics and Astronomy, Univ of Tennessee, Knoxville, Univ of Tennessee and ORNL., University of Tennessee, Univ of Tennessee, Knoxville, Department of Physics and Astronomy, University of Tennessee, Knoxville