Gao Hao, Liu Cong, Hermann Andreas, Needs Richard J, Pickard Chris J, Wang Hui-Tian, Xing Dingyu, Sun Jian
National Laboratory of Solid State Microstructures, School of Physics and Collaborative Innovation Center of Advanced Microstructures, Nanjing University, Nanjing 210093, China.
Centre for Science at Extreme Conditions and The School of Physics and Astronomy, The University of Edinburgh, Edinburgh EH9 3FD, UK.
Natl Sci Rev. 2020 Apr 22;7(10):1540-1547. doi: 10.1093/nsr/nwaa064. eCollection 2020 Oct.
Helium and methane are major components of giant icy planets and are abundant in the universe. However, helium is the most inert element in the periodic table and methane is one of the most hydrophobic molecules, thus whether they can react with each other is of fundamental importance. Here, our crystal structure searches and first-principles calculations predict that a HeCH compound is stable over a wide range of pressures from 55 to 155 GPa and a HeCH compound becomes stable around 105 GPa. As nice examples of pure van der Waals crystals, the insertion of helium atoms changes the original packing of pure methane molecules and also largely hinders the polymerization of methane at higher pressures. After analyzing the diffusive properties during the melting of HeCH at high pressure and high temperature, in addition to a plastic methane phase, we have discovered an unusual phase which exhibits coexistence of diffusive helium and plastic methane. In addition, the range of the diffusive behavior within the helium-methane phase diagram is found to be much narrower compared to that of previously predicted helium-water compounds. This may be due to the weaker van der Waals interactions between methane molecules compared to those in helium-water compounds, and that the helium-methane compound melts more easily.
氦和甲烷是巨大冰行星的主要成分,且在宇宙中含量丰富。然而,氦是元素周期表中最惰性的元素,甲烷是最疏水的分子之一,因此它们是否能相互反应至关重要。在此,我们的晶体结构搜索和第一性原理计算预测,一种HeCH化合物在55至155吉帕的广泛压力范围内是稳定的,且一种HeCH化合物在约105吉帕时变得稳定。作为纯范德华晶体的良好示例,氦原子的插入改变了纯甲烷分子的原始堆积,并且在较高压力下也极大地阻碍了甲烷的聚合。在分析了HeCH在高压和高温下熔化过程中的扩散性质后,除了塑性甲烷相之外,我们还发现了一个不寻常的相,该相表现出扩散氦和塑性甲烷的共存。此外,发现氦 - 甲烷相图内扩散行为的范围与先前预测的氦 - 水化合物相比要窄得多。这可能是由于甲烷分子之间的范德华相互作用比氦 - 水化合物中的弱,以及氦 - 甲烷化合物更容易熔化。