Neutron and ARPES constraints on the couplings of the multiorbital Hubbard model for the iron pnictides

Qinlong Luo, George Martins, Dao-Xin Yao, Maria Daghofer, Rong Yu, Adriana Moreo, and Elbio Dagotto
Phys. Rev. B 82, 104508 – Published 15 September 2010

Abstract

The results of neutron-scattering and angle-resolved photoemission experiments for the Fe-pnictide parent compounds, and their metallic nature, are shown to impose severe constraints on the range of values that can be considered “realistic” for the intraorbital Hubbard repulsion U and Hund coupling J in multiorbital Hubbard models treated in the mean-field approximation. Phase diagrams for three- and five-orbital models are here provided, and the physically realistic regime of couplings is highlighted, to guide future theoretical work into the proper region of parameters of Hubbard models. In addition, using the random phase approximation, the pairing tendencies in these realistic coupling regions are investigated. It is shown that the dominant spin-singlet pairing channels in these coupling regimes correspond to nodal superconductivity, with strong competition between several states that belong to different irreducible representations. This is compatible with experimental bulk measurements that have reported the existence of nodes in several Fe-pnictide compounds.

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  • Received 1 July 2010

DOI:https://doi.org/10.1103/PhysRevB.82.104508

©2010 American Physical Society

Authors & Affiliations

Qinlong Luo1,2, George Martins3, Dao-Xin Yao1,2,4, Maria Daghofer5, Rong Yu6, Adriana Moreo1,2, and Elbio Dagotto1,2

  • 1Department of Physics and Astronomy, University of Tennessee, Knoxville, Tennessee 37996, USA
  • 2Materials Science and Technology Division, Oak Ridge National Laboratory, Oak Ridge, Tennessee 32831, USA
  • 3Physics Department, Oakland University, Rochester, Michigan 48309, USA
  • 4State Key Laboratory of Optoelectronic Materials and Technologies, School of Physics and Engineering, Sun Yat-Sen University, Guangzhou 510275, China
  • 5IFW Dresden, P.O. Box 27 01 16, D-01171 Dresden, Germany
  • 6Department of Physics and Astronomy, Rice University, Houston, Texas 77005, USA

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Issue

Vol. 82, Iss. 10 — 1 September 2010

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