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层状镍酸盐在半填充时的反铁磁绝缘态。

Antiferromagnetic insulating state in layered nickelates at half filling.

作者信息

Jung Myung-Chul, LaBollita Harrison, Pardo Victor, Botana Antia S

机构信息

Department of Physics, Arizona State University, Tempe, AZ, 85287, USA.

Instituto de Materiais iMATUS, Universidade de Santiago de Compostela, 15782, Santiago de Compostela, Spain.

出版信息

Sci Rep. 2022 Oct 25;12(1):17864. doi: 10.1038/s41598-022-22176-2.

DOI:10.1038/s41598-022-22176-2
PMID:36284152
原文链接:https://pmc.ncbi.nlm.nih.gov/articles/PMC9596485/
Abstract

We provide a set of computational experiments based on ab initio calculations to elucidate whether a cuprate-like antiferromagnetic insulating state can be present in the phase diagram of the low-valence layered nickelate family (R[Formula: see text]Ni[Formula: see text]O[Formula: see text], R= rare-earth, [Formula: see text]) in proximity to half-filling. It is well established that at [Formula: see text] filling the infinite-layer ([Formula: see text]) nickelate is metallic, in contrast to cuprates wherein an antiferromagnetic insulator is expected. We show that for the Ruddlesden-Popper (RP) reduced phases of the series (finite n) an antiferromagnetic insulating ground state can naturally be obtained instead at [Formula: see text] filling, due to the spacer RO[Formula: see text] fluorite slabs present in their structure that block the c-axis dispersion. In the [Formula: see text] nickelate, the same type of solution can be derived if the off-plane R-Ni coupling is suppressed. We show how this can be achieved if a structural element that cuts off the c-axis dispersion is introduced (i.e. vacuum in a monolayer of RNiO[Formula: see text], or a blocking layer in multilayers formed by (RNiO[Formula: see text])[Formula: see text]/(RNaO[Formula: see text])[Formula: see text]).

摘要

我们基于从头算计算提供了一组计算实验,以阐明在低价层状镍酸盐家族(R[化学式:见原文]Ni[化学式:见原文]O[化学式:见原文],R = 稀土,[化学式:见原文])接近半填充的相图中是否可以存在类似铜酸盐的反铁磁绝缘态。众所周知,在[化学式:见原文]填充时,无限层([化学式:见原文])镍酸盐是金属性的,这与预期为反铁磁绝缘体的铜酸盐形成对比。我们表明,对于该系列的Ruddlesden-Popper(RP)还原相(有限n),由于其结构中存在的间隔层RO[化学式:见原文]萤石板阻断了c轴色散,在[化学式:见原文]填充时反而可以自然地获得反铁磁绝缘基态。在[化学式:见原文]镍酸盐中,如果面外R-Ni耦合被抑制,也可以得到相同类型的解。我们展示了如果引入一个切断c轴色散的结构元素(即RNiO[化学式:见原文]单层中的真空,或由(RNiO[化学式:见原文])[化学式:见原文]/(RNaO[化学式:见原文])[化学式:见原文]形成的多层中的阻挡层),如何实现这一点。

https://cdn.ncbi.nlm.nih.gov/pmc/blobs/5c94/9596485/cd5bf2388a81/41598_2022_22176_Fig5_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/5c94/9596485/a73b43a5c909/41598_2022_22176_Fig1_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/5c94/9596485/472acc62d73f/41598_2022_22176_Fig2_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/5c94/9596485/9e907fc07a70/41598_2022_22176_Fig3_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/5c94/9596485/d58936c0aabb/41598_2022_22176_Fig4_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/5c94/9596485/cd5bf2388a81/41598_2022_22176_Fig5_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/5c94/9596485/a73b43a5c909/41598_2022_22176_Fig1_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/5c94/9596485/472acc62d73f/41598_2022_22176_Fig2_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/5c94/9596485/9e907fc07a70/41598_2022_22176_Fig3_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/5c94/9596485/d58936c0aabb/41598_2022_22176_Fig4_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/5c94/9596485/cd5bf2388a81/41598_2022_22176_Fig5_HTML.jpg

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本文引用的文献

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