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Pairing Tendencies, Orbital Selective Mott Phases, and Magnetic Block States in Multiorbital Models for Iron-Based Ladders and Chains

Invited

Abstract

The discovery of superconductivity at high pressure in iron-based two-leg ladder 123 materials [1] established a new playground to better understand pairing tendencies in iron superconductors. Similarly as in Cu-oxide ladders, computational calculations using correlated electronic models can be performed with good accuracy in quasi-1D systems. Here, I will review our recent results for multiorbital Hubbard models varying the Hubbard and Hund couplings, and the electronic density. Clear indications of pair formation are found in lightly-doped ladders [2] and chains [3], and robust spin-singlet pair-pair correlations develop in those chains [3] (as in Cu-based ladders, we assume pressure leads to doping of the iron network [4]). An explanation for spin-singlet pairing based on an "orbital resonant valence bond" state is discussed for chains [5]. The magnetic properties in ladders and chains are also unexpectedly rich. An "orbital selective Mott phase" dominates in a wide range of parameters. In this regime, magnetic ``block'' states emerge, such as up-up-down-down patterns. We calculated the dynamical spin structure factor, finding a mixture of acoustic and optical modes [6] as in neutron experiments. Even more extended block states were recently discovered [7,8]. This complex behavior unveiled in models for 1D iron superconductors when studied accurately suggests that the physics of these materials could be far richer than anticipated.

[1] H. Takahashi et al., Nat. Mater. 14, 1008 (2015); J. Ying et al., PRB 95, 241109(R) (2017).
[2] N. Patel et al., PRB 94, 075119 (2016)
[3] N. Patel et al., PRB 96, 024520 (2017)
[4] Y. Zhang et al., PRB 95, 115154 (2017); PRB 97, 045119 (2018)
[5] N. Patel et al., submitted
[6] J. Herbrych et al., Nat. Comm. 9, 3736 (2018)
[7] J. Herbrych et al., PRL 123, 027203 (2019)
[8] J. Herbrych et al., submitted

Presenters

  • Elbio Dagotto

    Department of Physics and Astronomy, University of Tennessee and ORNL, Physics Department, University of Tennessee, University of Tennessee, Department of Physics and Astronomy, University of Tennessee at Knoxville, University of Tennessee, Knoxville, and Oak Ridge National Laboratory, University of Tennessee, Knoxville, Department of Physics and Astronomy, University of Tennessee, Knoxville, Tennessee

Authors

  • Elbio Dagotto

    Department of Physics and Astronomy, University of Tennessee and ORNL, Physics Department, University of Tennessee, University of Tennessee, Department of Physics and Astronomy, University of Tennessee at Knoxville, University of Tennessee, Knoxville, and Oak Ridge National Laboratory, University of Tennessee, Knoxville, Department of Physics and Astronomy, University of Tennessee, Knoxville, Tennessee