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Orbital-selective Mott phase in multiorbital models for iron pnictides and chalcogenides

机译:铁p和硫属元素化物多轨道模型中的轨道选择莫特相

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摘要

There is increasing recognition that the multiorbital nature of the 3d electrons is important to the proper description of the electronic states in the normal state of the iron-based superconductors. Earlier studies of the pertinent multiorbital Hubbard models identified an orbital-selective Mott phase, which anchors the orbital-selective behavior seen in the overall phase diagram. An important characteristics of the models is that the orbitals are kinetically coupled, i.e., hybridized, to each other, which makes the orbital-selective Mott phase especially nontrivial. A U(1) slave-spin method was used to analyze the model with nonzero orbital-level splittings. Here we develop a Landau free-energy functional to shed further light on this issue. We put the microscopic analysis from the U(1) slave-spin approach in this perspective, and show that the intersite spin correlations are crucial to the renormalization of the bare hybridization amplitude towards zero and the concomitant realization of the orbital-selective Mott transition. Based on this insight, we discuss additional ways to study the orbital-selective Mott physics from a dynamical competition between the interorbital hybridization and collective spin correlations. Our results demonstrate the robustness of the orbital-selective Mott phase in the multiorbital models appropriate for the iron-based superconductors.
机译:人们越来越认识到3d电子的多轨道性质对于正确描述铁基超导体正常状态下的电子状态很重要。有关多轨道Hubbard模型的早期研究确定了轨道选择性Mott相,该相固定了整个相图中看到的轨道选择性行为。这些模型的重要特征是,轨道之间是动力学耦合的,即相互杂交的,这使得轨道选择的莫特相特别平凡。 U(1)从属自旋方法用于分析具有非零轨道级分裂的模型。在这里,我们开发了Landau自由能功能,以进一步阐明该问题。我们从这个角度从U(1)从动自旋方法进行了微观分析,并表明站点间自旋相关性对于裸杂交幅度向零的重新归一化以及轨道选择性Mott过渡的同时实现至关重要。基于这一见解,我们讨论了从轨道间杂交与集体自旋相关性之间的动力学竞争研究轨道选择性莫特物理学的其他方法。我们的结果证明了在适用于铁基超导体的多轨道模型中,轨道选择Mott相的鲁棒性。

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  • 来源
    《Physical review. B, Condensed Matter And Materals Physics》 |2017年第12期|125110.1-125110.10|共10页
  • 作者

    Rong Yu; Qimiao Si;

  • 作者单位

    Department of Physics, Renmin University of China, Beijing 100872, China,Department of Physics and Astronomy, Shanghai Jiao Tong University, Shanghai 200240, China and Collaborative Innovation Center of Advanced Microstructures, Nanjing 210093, China;

    Department of Physics & Astronomy, Rice University, Houston, Texas 77005, USA;

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