La3Ni2O7的缠绕电荷和自旋不稳定性

IF 7.5 1区 物理与天体物理 Q1 PHYSICS, MULTIDISCIPLINARY
Guiwen Jiang, Chenye Qin, Kateryna Foyevtsova, Liang Si, Mona Berciu, George A. Sawatzky, Mi Jiang
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引用次数: 0

摘要

镍基超导体的研究已经从无限层LaNiO2发展到有限层La6Ni5O12,以及最近的Ruddlesden-Popper相La3Ni2O7,该相被发现在~ 80k和~ 16 GPa的压力下表现出超导性。本文利用密度泛函计算和多轨道、多原子团簇精确对角化(包括局域交换和库仑相互作用),分析了La3Ni2O7双层相中Ni2O9团簇的压力依赖性低能电子态。我们量化了Ni2O9团簇的各种可能的自旋态,并通过\({\rm{Ni}}-3d_{3z^2-r^2}\)轨道和原子Hund规则交换、顶端桥接O-2pz轨道以及参与局部类张- rice单重态形成的轨道的参与量化了Ni2O9团簇的交换和超交换机制。我们发现,对于标称价态和局部电荷波动,导致团簇基态的主要构型都不涉及顶端氧的占据;相反,他们倾向于在O配体空穴和Ni \(3d_{z^2-y^2}\)轨道之间形成平面内的张-赖斯单重态。我们还强调了由我们的簇结果提出的两种可能的电荷和自旋有序状态,它们在我们的模型中的所有相关压力下几乎是简并的。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Intertwined charge and spin instability of La3Ni2O7

Research on nickel-based superconductors has progressed from infinite-layer LaNiO2 to finite-layer La6Ni5O12, and most recently to the Ruddlesden-Popper phase La3Ni2O7, which was found to exhibit onset of superconductivity at ∼80 K under a pressure of ∼16 GPa. Using density functional calculations and multi-orbital, multi-atom cluster exact diagonalization that includes local exchange and Coulomb interactions, here we analyze the pressure dependent low-energy electronic states of the Ni2O9 cluster, relevant for the bilayer phase of La3Ni2O7. We quantify the various possible spin states and the exchange and superexchange mechanisms of the Ni2O9 cluster are quantified through the involvement of the \({\rm{Ni}}-3d_{3z^2-r^2}\) orbitals and the atomic Hund’s rule exchange, the apical bridging O-2pz orbitals, and the orbitals involved in the formation of local Zhang-Rice singlet like states. We find that the leading configurations contributing to the cluster ground-states both for nominal valence and also with local charge fluctuations, do not involve occupation of the apical oxygen; instead, they favor the formation of in-plane Zhang-Rice singlet-like states between an O ligand hole and the Ni \(3d_{z^2-y^2}\) orbital. We also highlight two possible charge and spin ordered states suggested by our cluster results, that are nearly degenerate at all relevant pressures within our modeling.

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来源期刊
Science China Physics, Mechanics & Astronomy
Science China Physics, Mechanics & Astronomy PHYSICS, MULTIDISCIPLINARY-
CiteScore
10.30
自引率
6.20%
发文量
4047
审稿时长
3 months
期刊介绍: Science China Physics, Mechanics & Astronomy, an academic journal cosponsored by the Chinese Academy of Sciences and the National Natural Science Foundation of China, and published by Science China Press, is committed to publishing high-quality, original results in both basic and applied research. Science China Physics, Mechanics & Astronomy, is published in both print and electronic forms. It is indexed by Science Citation Index. Categories of articles: Reviews summarize representative results and achievements in a particular topic or an area, comment on the current state of research, and advise on the research directions. The author’s own opinion and related discussion is requested. Research papers report on important original results in all areas of physics, mechanics and astronomy. Brief reports present short reports in a timely manner of the latest important results.
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