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基于 3d 过渡金属原子的金属-有机配位网络的磁性。

Magnetic Properties of Metal⁻Organic Coordination Networks Based on 3d Transition Metal Atoms.

机构信息

Departamento de Física de Materiales UPV/EHU, 20018 Donostia-San Sebastián, Spain.

Donostia International Physics Center (DIPC), 20018 Donostia-San Sebastián, Spain.

出版信息

Molecules. 2018 Apr 20;23(4):964. doi: 10.3390/molecules23040964.

DOI:10.3390/molecules23040964
PMID:29677142
原文链接:https://pmc.ncbi.nlm.nih.gov/articles/PMC6017066/
Abstract

The magnetic anisotropy and exchange coupling between spins localized at the positions of 3d transition metal atoms forming two-dimensional metal⁻organic coordination networks (MOCNs) grown on a Au(111) metal surface are studied. In particular, we consider MOCNs made of Ni or Mn metal centers linked by 7,7,8,8-tetracyanoquinodimethane (TCNQ) organic ligands, which form rectangular networks with 1:1 stoichiometry. Based on the analysis of X-ray magnetic circular dichroism (XMCD) data taken at T = 2.5 K, we find that Ni atoms in the Ni⁻TCNQ MOCNs are coupled ferromagnetically and do not show any significant magnetic anisotropy, while Mn atoms in the Mn⁻TCNQ MOCNs are coupled antiferromagnetically and do show a weak magnetic anisotropy with in-plane magnetization. We explain these observations using both a model Hamiltonian based on mean-field Weiss theory and density functional theory calculations that include spin⁻orbit coupling. Our main conclusion is that the antiferromagnetic coupling between Mn spins and the in-plane magnetization of the Mn spins can be explained by neglecting effects due to the presence of the Au(111) surface, while for Ni⁻TCNQ the metal surface plays a role in determining the absence of magnetic anisotropy in the system.

摘要

研究了定位在二维金属-有机配位网络(MOCN)中 3d 过渡金属原子位置的自旋的磁各向异性和交换耦合,该网络生长在 Au(111)金属表面上。特别是,我们考虑了由 Ni 或 Mn 金属中心通过 7,7,8,8-四氰基对醌二甲烷(TCNQ)有机配体连接而成的 MOCN,它们以 1:1 的化学计量比形成矩形网络。基于在 T = 2.5 K 下采集的 X 射线磁圆二色性(XMCD)数据的分析,我们发现 Ni⁻TCNQ MOCN 中的 Ni 原子呈铁磁耦合,且不显示任何显著的磁各向异性,而 Mn⁻TCNQ MOCN 中的 Mn 原子呈反铁磁耦合,且表现出弱的面内磁化磁各向异性。我们使用基于平均场 Weiss 理论的模型哈密顿量和包括自旋-轨道耦合的密度泛函理论计算来解释这些观察结果。我们的主要结论是,Mn 自旋之间的反铁磁耦合和面内 Mn 自旋的磁化可以通过忽略由于存在 Au(111)表面而产生的效应来解释,而对于 Ni⁻TCNQ,金属表面在确定系统中不存在磁各向异性方面起着作用。

https://cdn.ncbi.nlm.nih.gov/pmc/blobs/6783/6017066/7064f31e076a/molecules-23-00964-g008.jpg
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https://cdn.ncbi.nlm.nih.gov/pmc/blobs/6783/6017066/344efaf5242c/molecules-23-00964-g002.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/6783/6017066/212a3d284ace/molecules-23-00964-g003.jpg
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https://cdn.ncbi.nlm.nih.gov/pmc/blobs/6783/6017066/7064f31e076a/molecules-23-00964-g008.jpg

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