Alderman O L G, Benmore C J, Neuefeind J, Tamalonis A, Weber R
Materials Development, Inc., Arlington Heights, IL 60004, United States of America.
J Phys Condens Matter. 2019 May 22;31(20):20LT01. doi: 10.1088/1361-648X/ab0939. Epub 2019 Feb 21.
The structure of molten BaTiO has been measured using laser heating, aerodynamic levitation and a combination of neutron diffraction with Ti isotope substitution, x-ray diffraction and spectroscopy. All measurements indicate a Ti-O coordination of n = 4.4(2), far lower than the perovskite or hexagonal crystalline forms. However, n > 4 suggests structural analogy with molten silicates at high pressures. We introduce methodology for ascertaining such analogies and demonstrate similarity with molten CaSiO at upper mantle pressures circa 5 GPa. Although some topological differences exist, we propose that planetary melt analogues provide rich insight into important processes relevant to hot exoplanets and Earth's early history.
利用激光加热、气动悬浮以及中子衍射与钛同位素取代、X射线衍射和光谱学相结合的方法,对熔融的BaTiO的结构进行了测量。所有测量结果均表明,Ti-O配位数n = 4.4(2),远低于钙钛矿或六方晶型。然而,n > 4表明在高压下与熔融硅酸盐具有结构相似性。我们介绍了确定此类相似性的方法,并证明了在约5 GPa的上地幔压力下与熔融CaSiO的相似性。尽管存在一些拓扑差异,但我们认为行星熔体类似物为与热系外行星和地球早期历史相关的重要过程提供了丰富的见解。