Pomjakushin V
Laboratory for Neutron Scattering and Imaging, Paul Scherrer Institut (PSI), 5232 Villigen PSI, Switzerland.
Acta Crystallogr B Struct Sci Cryst Eng Mater. 2024 Oct 1;80(Pt 5):385-392. doi: 10.1107/S205252062400756X. Epub 2024 Sep 10.
The magnetic and crystal structures of manganese and nickel monoxides have been studied using high-resolution neutron diffraction. The known 1k-structures based on the single propagation vector [½ ½ ½] for the parent paramagnetic space group Fm3m are forced to have monoclinic magnetic symmetry and are not possible in rhombohedral symmetry. However, the monoclinic distortions from the rhombohedral crystal metric allowed by symmetry are very small, and the explicit monoclinic splittings of the diffraction peaks have not been experimentally observed. We analyse the magnetic crystallographic models metrically compatible with our experimental data in full detail by using isotropy subgroup representation approach, including rhombohedral solutions based on the propagation vector star {[½ ½ ½], [-½ ½ ½], [½-½ ½], [½ ½ -½]}. Although the full star rhombohedral R3c structure can equally well fit our diffraction data for NiO, we conclude that the best solution for the crystal and magnetic structures for NiO and MnO is the 1k monoclinic model with the magnetic space group C2/c (Belov-Neronova-Smirnova No. 15.90, UNI symbol C2/c.1'[C2/m]).
利用高分辨率中子衍射研究了一氧化锰和一氧化镍的磁性和晶体结构。基于顺磁空间群Fm3m的单传播矢量[½ ½ ½]的已知1k结构被迫具有单斜磁对称性,而在菱面体对称性中是不可能的。然而,由对称性允许的从菱面体晶体度量的单斜畸变非常小,并且尚未通过实验观察到衍射峰的明显单斜分裂。我们通过使用各向同性子群表示方法,详细分析了与我们的实验数据在度量上兼容的磁晶体学模型,包括基于传播矢量星{[½ ½ ½], [-½ ½ ½], [½ -½ ½], [½ ½ -½]}的菱面体解。尽管全星菱面体R3c结构同样能很好地拟合我们对NiO的衍射数据,但我们得出结论,对于NiO和MnO的晶体和磁性结构,最佳解决方案是具有磁空间群C2/c(别洛夫 - 涅罗诺娃 - 斯米尔诺娃编号15.90,通用符号C2/c.1'[C2/m])的1k单斜模型。