Goncharov Alexander F, Struzhkin Viktor V, Jacobsen Steven D
Geophysical Laboratory, Carnegie Institution of Washington, 5251 Broad Branch Road, NW, Washington, DC 20015, USA.
Science. 2006 May 26;312(5777):1205-8. doi: 10.1126/science.1125622.
Optical absorption spectra have been measured at pressures up to 80 gigapascals (GPa) for the lower-mantle oxide magnesiowüstite (Mg,Fe)O. Upon reaching the high-spin to low-spin transition of Fe2+ at about 60 GPa, we observed enhanced absorption in the mid- and near-infrared spectral range, whereas absorption in the visible-ultraviolet was reduced. The observed changes in absorption are in contrast to prediction and are attributed to d-d orbital charge transfer in the Fe2+ ion. The results indicate that low-spin (Mg,Fe)O will exhibit lower radiative thermal conductivity than high-spin (Mg,Fe)O, which needs to be considered in future geodynamic models of convection and plume stabilization in the lower mantle.
已在高达80吉帕斯卡(GPa)的压力下测量了下地幔氧化物镁铁方铁矿(Mg,Fe)O的光吸收光谱。在约60 GPa时达到Fe2+的高自旋到低自旋转变时,我们观察到中红外和近红外光谱范围内的吸收增强,而可见光-紫外光范围内的吸收则降低。观察到的吸收变化与预测相反,归因于Fe2+离子中的d-d轨道电荷转移。结果表明,低自旋(Mg,Fe)O的辐射热导率将低于高自旋(Mg,Fe)O,这在未来关于下地幔对流和地幔柱稳定的地球动力学模型中需要予以考虑。