Spektor Kristina, Crichton Wilson A, Konar Sumit, Filippov Stanislav, Klarbring Johan, Simak Sergei I, Häussermann Ulrich
ESRF, The European Synchrotron Radiation Facility , F-38000 Grenoble, France.
EaStChem School of Chemistry and Centre for Science at Extreme Conditions (CSEC), University of Edinburgh , Edinburgh EH9 3FJ, United Kingdom.
Inorg Chem. 2018 Feb 5;57(3):1614-1622. doi: 10.1021/acs.inorgchem.7b02968. Epub 2018 Jan 11.
The Mg-Mn-H system was investigated by in situ high pressure studies of reaction mixtures MgH-Mn-H. The formation conditions of two complex hydrides with composition MgMnH were established. Previously known hexagonal MgMnH (h-MgMnH) formed at pressures 1.5-2 GPa and temperatures between 480 and 500 °C, whereas an orthorhombic form (o-MgMnH) was obtained at pressures above 5 GPa and temperatures above 600 °C. The crystal structures of the polymorphs feature octahedral [Mn(I)H] complexes and interstitial H. Interstitial H is located in trigonal bipyramidal and square pyramidal interstices formed by Mg ions in h- and o-MgMnH, respectively. The hexagonal form can be retained at ambient pressure, whereas the orthorhombic form upon decompression undergoes a distortion to monoclinic MgMnH (m-MgMnH). The structure elucidation of o- and m-MgMnH was aided by first-principles density functional theory (DFT) calculations. Calculated enthalpy versus pressure relations predict m- and o-MgMnH to be more stable than h-MgMnH above 4.3 GPa. Phonon calculations revealed o-MgMnH to be dynamically unstable at pressures below 5 GPa, which explains its phase transition to m-MgMnH on decompression. The electronic structure of the quenchable polymorphs h- and m-MgMnH is very similar. The stable 18-electron complex [MnH] is mirrored in the occupied states, and calculated band gaps are around 1.5 eV. The study underlines the significance of in situ investigations for mapping reaction conditions and understanding phase relations for hydrogen-rich complex transition metal hydrides.
通过对反应混合物MgH-Mn-H进行原位高压研究,对Mg-Mn-H体系展开了探究。确定了两种组成成分为MgMnH的复杂氢化物的形成条件。先前已知的六方晶系MgMnH(h-MgMnH)在1.5-2 GPa的压力和480至500°C的温度下形成,而正交晶系形式(o-MgMnH)是在高于5 GPa的压力和高于600°C的温度下获得的。多晶型物的晶体结构具有八面体[Mn(I)H]络合物和间隙氢。间隙氢分别位于由h-MgMnH和o-MgMnH中的镁离子形成的三角双锥和四方锥间隙中。六方晶系形式在常压下可以保留,而正交晶系形式在减压时会发生畸变,转变为单斜晶系MgMnH(m-MgMnH)。第一性原理密度泛函理论(DFT)计算有助于对o-MgMnH和m-MgMnH的结构进行阐释。计算得出的焓与压力关系预测,在高于4.3 GPa时,m-MgMnH和o-MgMnH比h-MgMnH更稳定。声子计算表明,o-MgMnH在低于5 GPa的压力下动力学不稳定,这解释了其在减压时向m-MgMnH的相变。可猝灭多晶型物h-MgMnH和m-MgMnH的电子结构非常相似。稳定的18电子络合物[MnH]反映在占据态中,计算得出的带隙约为1.5 eV。该研究强调了原位研究对于绘制反应条件和理解富氢复杂过渡金属氢化物的相关系的重要性。