在BiCoO3中压力诱导的旋转状态转换
Kengo Oka1, Masaki Azuma, Wei-tin Chen
1Institute for Chemical Research, Kyoto University, Uji, Kyoto 611-0011, Japan. oka@issp.u-tokyo.ac.jp
Journal of the American Chemical Society
|June 24, 2010
概括
高压改变了甲氧化物 (BiCoO3) 结构,导致体积减少和电阻率下降. 这揭示了离子的自旋状态变化,对于理解其电子性质至关重要.
科学领域:
- 材料科学 材料科学 材料科学
- 固态物理 固态物理
- 晶体学 晶体学是指结晶学.
背景情况:
- 木氧化物 (BiCoO3) 具有复杂的结构和电子特性.
- 了解压力下的相变是新材料应用的关键.
研究的目的:
- 在高压下研究BiCoO3的结构和电子行为.
- 确定压力诱导的相变和相关的属性变化.
主要方法:
- 使用同步X射线和中子粉衍射来分析结构变化.
- 在不同压力条件下进行电阻测量.
- 使用X射线发射光谱来探测电子和自旋状态的过渡.
主要成果:
- 从极性PbTiO3型到中心对称的GdFeO3型的结构相位过渡发生在3GPa以上.
- 在室温下观察到13%的显著体积减少,与旋转状态的变化有关.
- 在第一阶段过渡过程中,电阻率急剧下降.
- 结构数据表明,高压下Co3+的旋转状态较低,而X射线发射光谱则表明旋转状态中等.
结论:
- 高压会在BiCoO3.3中引起明显的结构和电子转变.
- 观察到的离子的自旋状态变化是材料对压力的反应的一个关键因素.
- 构建的压力-温度相位图为材料的稳定性和过渡温度提供了洞察力.
相关概念视频
Colors and Magnetism
Color in Coordination Complexes
When atoms or molecules absorb light at the proper frequency, their electrons are excited to higher-energy orbitals. For many main group atoms and molecules, the absorbed photons are in the ultraviolet range of the electromagnetic spectrum, which cannot be detected by the human eye. For coordination compounds, the energy difference between the d orbitals often allows photons in the visible range to be absorbed and emitted, which is seen as colors by the human eye.
When atoms or molecules absorb light at the proper frequency, their electrons are excited to higher-energy orbitals. For many main group atoms and molecules, the absorbed photons are in the ultraviolet range of the electromagnetic spectrum, which cannot be detected by the human eye. For coordination compounds, the energy difference between the d orbitals often allows photons in the visible range to be absorbed and emitted, which is seen as colors by the human eye.
Valence Bond Theory
Coordination compounds and complexes exhibit different colors, geometries, and magnetic behavior, depending on the metal atom/ion and ligands from which they are composed. In an attempt to explain the bonding and structure of coordination complexes, Linus Pauling proposed the valence bond theory, or VBT, using the concepts of hybridization and the overlapping of the atomic orbitals. According to VBT, the central metal atom or ion (Lewis acid) hybridizes to provide empty orbitals of suitable...
Atomic Nuclei: Nuclear Spin State Overview
NMR-active nuclei have energy levels called 'spin states' that are associated with the orientations of their nuclear magnetic moments. In the absence of a magnetic field, the nuclear magnetic moments are randomly oriented, and the spin states are degenerate. When an external magnetic field is applied, the spin states have only 2 + 1 orientations available to them. A proton with = ½ has two available orientations. Similarly, for a quadrupolar nucleus with a nuclear spin value of one, the...
Spin–Spin Coupling Constant: Overview
In bromoethane, the three methyl protons are coupled to the two methylene protons that are three bonds away. In accordance with the n+1 rule, the signal from the methyl protons is split into three peaks with 1:2:1 relative intensities. The methylene protons appear as a quartet, with the relative intensities of 1:3:3:1.
Qualitatively, any spin plus-half nucleus polarizes the spins of its electrons to the minus-half state. Consequently, the paired electron in the hydrogen–carbon bond must have a...
Qualitatively, any spin plus-half nucleus polarizes the spins of its electrons to the minus-half state. Consequently, the paired electron in the hydrogen–carbon bond must have a...
Spin–Spin Coupling: One-Bond Coupling
Coupling interactions are strongest between NMR-active nuclei bonded to each other, where spin information can be transmitted directly through the pair of bonding electrons. While nuclei polarize their electrons to the opposite spins, the bonding electron pair has opposite spins. Configurations with antiparallel nuclear spins are expected to be lower in energy. When coupling makes antiparallel states more favorable, J is considered to have a positive value. The one-bond coupling constant, 1J,...
Atomic Nuclei: Nuclear Spin State Population Distribution
Near absolute zero temperatures, in the presence of a magnetic field, the majority of nuclei prefer the lower energy spin-up state to the higher energy spin-down state. As temperatures increase, the energy from thermal collisions distributes the spins more equally between the two states. The Boltzmann distribution equation gives the ratio of the number of spins predicted in the spin −½ (N−) and spin +½ (N+) states.


