Department of Physics and Astronomy, University of Glasgow, University Avenue, Glasgow, G12 8QQ, Scotland, United Kingdom.
Micron. 2010 Aug;41(6):547-53. doi: 10.1016/j.micron.2010.04.013. Epub 2010 May 7.
The electron energy loss near edge structure on the O K-edge from chromite spinels contains fine structure from the hybridisation of the O p-orbitals and the Cr d-orbitals. Unlike the aluminates, a non-spin polarised calculation of this fine structure differs significantly from experimental observations. This is due to the large magnetic moment on the Cr. Calculations using simplified collinear ordering of the spins and the local spin density approximation give much improved agreement. A real space multiple scattering formalism and a reciprocal space density functional formalism give results in substantial agreement. In general, the actual spin arrangement of these chromites is not known since they are typically frustrated magnetic systems with ordering temperatures in the 10-20K range. The calculations are based on the hypothesis that dynamic short range order persists to room temperature over the time scale of the interaction with the fast electron. However, it is possible that the observed effects are due to the strong paramagnetism present at room temperatures but which it is not possible to simulate accurately at present.
尖晶石铬铁矿 O K 边的近边电子能量损失结构包含 O p 轨道和 Cr d 轨道杂化的精细结构。与铝酸盐不同,这种精细结构的非自旋极化计算与实验观察结果有很大的不同。这是由于 Cr 上的磁矩很大。使用自旋的简化共线排序和局域自旋密度近似的计算给出了更好的一致性。实空间多次散射形式和倒空间密度泛函形式给出了非常一致的结果。一般来说,这些铬铁矿的实际自旋排列是未知的,因为它们通常是具有在 10-20K 范围内的有序温度的受挫磁体系统。这些计算基于这样的假设,即在与快速电子相互作用的时间尺度内,动态短程有序持续到室温。然而,也有可能观察到的效应是由于室温下存在的强顺磁性质,但目前还不可能准确地模拟。