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High-pressure crystal structures and superconductivity of Stannane (SnH4)

机译:锡烷(SnH4)的高压晶体结构和超导性

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摘要

There is great interest in the exploration of hydrogen-rich compounds upon strong compression where they can become superconductors. Stannane (SnH4) has been proposed to be a potential high-temperature superconductor under pressure, but its high-pressure crystal structures, fundamental for the understanding of superconductivity, remain unsolved. Using an ab initio evolutionary algorithm for crystal structure prediction, we propose the existence of two unique high-pressure metallic phases having space groups Ama2 and P63/mmc, which both contain hexagonal layers of Sn atoms and semimolecular (perhydride) H2 units. Enthalpy calculations reveal that the Ama2 and P63/mmc structures are stable at 96–180 GPa and above 180 GPa, respectively, while below 96 GPa SnH4 is unstable with respect to elemental decomposition. The application of the Allen-Dynes modified McMillan equation reveals high superconducting temperatures of 15–22 K for the Ama2 phase at 120 GPa and 52–62 K for the P63/mmc phase at 200 GPa.
机译:在富氢化合物在强压缩下可以成为超导体的过程中,人们对它们的研究引起了极大的兴趣。有人建议将Stannane(SnH4)在压力下用作高温超导体,但其高压晶体结构(对于理解超导性至关重要)仍未解决。使用从头算进化算法进行晶体结构预测,我们建议存在两个具有空间群Ama2和P63 / mmc的独特高压金属相,它们均包含六方层的Sn原子和半分子(全氢化物)H2单元。焓计算表明,Ama2和P63 / mmc结构分别在96–180 GPa和180 GPa以上稳定,而在96 GPa以下SnH4就元素分解而言是不稳定的。 Allen-Dynes修正的McMillan方程的应用揭示了120GPa时Ama2相的高温超导温度为15-22 K,200GPa时P63 / mmc相的超导温度为52-62 K.

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