Department of Chemistry , North Carolina State University , Raleigh , North Carolina 27695 , United States.
State Key Laboratory of Structural Chemistry , Fujian Institute of Research on the Structure of Matter (FJIRSM), Chinese Academy of Sciences (CAS) , Fuzhou 350002 , China.
Inorg Chem. 2018 Aug 6;57(15):9260-9265. doi: 10.1021/acs.inorgchem.8b01274. Epub 2018 Jul 23.
Rare-earth indium oxides RInO (R = Gd, Tb, Dy) consist of spin-frustrated hexagonal spin lattices made up of rare-earth ions R, where R = Gd (f, L = 0), Tb (f, L = 3), and Dy (f, L = 5). We carried out DFT calculations for RInO, including on-site repulsion U with/without spin-orbit coupling (SOC), to explore if their low-temperature magnetic properties are related to the two nonequivalent nearest-neighbor (NN) spin exchanges of their hexagonal spin lattices. Our DFT + U + SOC calculations predict that the orbital moments of the Tb and Dy ions are smaller than their free-ion values by ∼2μ while the Tb spins have an in-plane magnetic anisotropy, in agreement with the experiments. This suggests that the f orbitals of each R (R = Tb, Dy) ion are engaged, though weakly, in bonding with the surrounding ligand atoms. The magnetic properties of GdInO with the zero orbital moment are adequately described by the spin exchanges extracted by DFT + U calculations. In describing the magnetic properties of TbInO and DyInO with nonzero orbital moments, however, the spin exchanges extracted by DFT + U + SOC calculations are necessary. The spin exchanges of RInO (R = Gd, Tb, Dy) are dominated by the two NN spin exchanges J and J of their hexagonal spin lattice, in which the honeycomb lattice of J forms spin-frustrated ( J, J, J) triangles. The J/ J ratios are calculated to be ∼3, ∼1.7, and ∼1 for GdInO, TbInO, and DyInO, respectively. This suggests that the antiferromagnetic (AFM) ordering of GdInO below 1.8 K is most likely an AFM ordering of its honeycomb spin lattice and that TbInO would exhibit low-temperature magnetic properties similar to those of GdInO while DyInO would not.
稀土铟氧化物 RInO(R = Gd、Tb、Dy)由稀土离子 R 组成的具有自旋阻挫的六方自旋晶格组成,其中 R = Gd(f,L = 0)、Tb(f,L = 3)和 Dy(f,L = 5)。我们对 RInO 进行了密度泛函理论(DFT)计算,包括考虑和不考虑自旋轨道耦合(SOC)的局域排斥 U,以探究其低温磁性质是否与其六方自旋晶格的两个非等效最近邻(NN)自旋交换有关。我们的 DFT + U + SOC 计算预测,Tb 和 Dy 离子的轨道磁矩比自由离子值小约 2μ,而 Tb 自旋具有面内各向异性磁各向异性,与实验结果一致。这表明每个 R(R = Tb、Dy)离子的 f 轨道尽管较弱,但与周围的配体原子发生了键合。具有零轨道磁矩的 GdInO 的磁性性质可以通过 DFT + U 计算提取的自旋交换来充分描述。然而,对于具有非零轨道磁矩的 TbInO 和 DyInO,需要使用 DFT + U + SOC 计算提取的自旋交换来描述其磁性性质。RInO(R = Gd、Tb、Dy)的自旋交换由其六方自旋晶格的两个 NN 自旋交换 J 和 J 主导,其中 J 的蜂窝晶格形成自旋阻挫的(J、J、J)三角形。计算得到的 J/J 比值分别约为 3、1.7 和 1,对于 GdInO、TbInO 和 DyInO。这表明 GdInO 在 1.8 K 以下的反铁磁(AFM)有序很可能是其蜂窝自旋晶格的 AFM 有序,而 TbInO 将表现出类似于 GdInO 的低温磁性质,而 DyInO 则不会。