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首页> 外文期刊>Physical review. B, Condensed Matter And Materals Physics >Density matrix renormalization group study of a three-orbital Hubbard model with spin-orbit coupling in one dimension
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Density matrix renormalization group study of a three-orbital Hubbard model with spin-orbit coupling in one dimension

机译:一维自旋轨道耦合的三轨道哈伯德模型的密度矩阵重整化群研究

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摘要

Using the density matrix renormalization group technique we study the effect of spin-orbit coupling on a three-orbital Hubbard model in the (t_(2g))~4 sector and in one dimension. Fixing the Hund coupling to a robust value compatible with some multiorbital materials, we present the phase diagram varying the Hubbard U and spin-orbit coupling λ, at zero temperature. Our results are shown to be qualitatively similar to those recently reported using the dynamical mean-field theory in higher dimensions, providing a robust basis to approximate many-body techniques. Among many results, we observe an interesting transition from an orbital-selective Mott phase to an excitonic insulator with increasing A. at intermediate U. In the strong U coupling limit, we find a nonmagnetic insulator with an effective angular momentum 〈(J~(eff))~2〉≠ 0 near the excitonic phase, smoothly connected to the 〈(J~(eff))~2〉 = 0 regime. We also provide a list of quasi-one-dimensional materials where the physics discussed in this paper could be realized.
机译:使用密度矩阵重归一化群技术,我们研究了自旋轨道耦合对(t_(2g))〜4扇区和一维三轨道Hubbard模型的影响。将Hund耦合固定为与某些多轨道材料兼容的稳健值,我们给出了在零温度下改变Hubbard U和自旋轨道耦合λ的相图。我们的结果显示出在质量上与最近使用动力学平均场理论在更高维度上报道的结果相似,为近似多体技术提供了可靠的基础。在许多结果中,我们观察到在中间U处随着A.的增加,从轨道选择Mott相到激子绝缘子的有趣转变。在强U耦合极限下,我们发现了具有有效角动量〈(J〜( eff))〜2〉≠0在激子相附近,平滑地连接到〈(J〜(eff))〜2〉 = 0态。我们还提供了准一维材料的清单,可以实现本文中讨论的物理学。

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  • 来源
    《Physical review. B, Condensed Matter And Materals Physics》 |2017年第15期|155111.1-155111.10|共10页
  • 作者单位

    Department of Physics and Astronomy, The University of Tennessee, Knoxville, Tennessee 37996, USA,Materials Science and Technology Division, Oak Ridge National Laboratory, Oak Ridge, Tennessee 37831, USA;

    Department of Physics and Astronomy, The University of Tennessee, Knoxville, Tennessee 37996, USA,Materials Science and Technology Division, Oak Ridge National Laboratory, Oak Ridge, Tennessee 37831, USA;

    Department of Physics and Astronomy, The University of Tennessee, Knoxville, Tennessee 37996, USA,Materials Science and Technology Division, Oak Ridge National Laboratory, Oak Ridge, Tennessee 37831, USA;

    Center for Nanophase Materials Sciences, Oak Ridge National Laboratory, Oak Ridge, Tennessee 37831, USA,Computational Science and Engineering Division, Oak Ridge National Laboratory, Oak Ridge, Tennessee 37831, USA;

    Department of Physics and Astronomy, The University of Tennessee, Knoxville, Tennessee 37996, USA,Materials Science and Technology Division, Oak Ridge National Laboratory, Oak Ridge, Tennessee 37831, USA;

    Materials Science and Technology Division, Oak Ridge National Laboratory, Oak Ridge, Tennessee 37831, USA;

    Department of Physics and Astronomy, The University of Tennessee, Knoxville, Tennessee 37996, USA,Materials Science and Technology Division, Oak Ridge National Laboratory, Oak Ridge, Tennessee 37831, USA;

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