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压力诱导脱水和氨一水合物-II 的结构。

Pressure-induced dehydration and the structure of ammonia hemihydrate-II.

机构信息

SUPA, School of Physics and Astronomy, Centre for Science at Extreme Conditions, University of Edinburgh, Edinburgh EH9 3JZ, United Kingdom.

出版信息

J Chem Phys. 2012 Mar 7;136(9):094506. doi: 10.1063/1.3686870.

Abstract

The structure of the crystalline ammonia-bearing phase formed when ammonia monohydrate liquid is compressed to 3.5(1) GPa at ambient temperature has been solved from a combination of synchrotron x-ray single-crystal and neutron powder-diffraction studies. The solution reveals that rather than having the ammonia monohydrate (AMH) composition as had been previously thought, the structure has an ammonia hemihydrate composition. The structure is monoclinic with spacegroup P2(1)/c and lattice parameters a = 3.3584(5) Å, b = 9.215(1) Å, c = 8.933(1) Å and β = 94.331(8)° at 3.5(1) GPa. The atomic arrangement has a crowned hexagonal arrangement and is a layered structure with long N-D···N hydrogen bonds linking the layers. The existence of pressure-induced dehydration of AMH may have important consequences for the behaviour and differentiation of icy planets and satellites.

摘要

当一水合氨液体在环境温度下被压缩至 3.5(1) GPa 时,形成的含氨结晶相的结构已通过同步加速器 X 射线单晶和中子粉末衍射研究的组合来解决。该解决方案表明,该结构的氨一水合物(AMH)组成与之前的想法不同,而是具有氨半水合物组成。该结构为单斜晶系,空间群为 P2(1)/c,晶格参数为 a = 3.3584(5) Å, b = 9.215(1) Å, c = 8.933(1) Å 和 β = 94.331(8)°,在 3.5(1) GPa 下。原子排列呈冠状六方排列,是一种层状结构,长的 N-D···N 氢键将各层连接在一起。AMH 的压力诱导脱水的存在可能对冰态行星和卫星的行为和分化产生重要影响。

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