The systematic study on the stability and superconductivity of Y-Mg-H compounds under high pressure
Peng Song, Zhufeng Hou, Pedro Baptista de Castro, Kousuke Nakano,, Kenta Hongo, Yoshihiko Takano, Ryo Maezono

TL;DR
This study uses computational methods to explore the stability and superconductivity of Y-Mg-H compounds under high pressure, revealing stable structures and potential high-temperature superconductivity around 190 K.
Contribution
It systematically investigates the structural stability and superconducting properties of YMgH$_{x}$ compounds at high pressures, identifying new stable and metastable phases with high $T_c$ values.
Findings
Hydrogen-rich YMgH$_{x}$ compounds require pressures above 200 GPa for stability.
The $Fd\bar{3}m$-YMgH$_{12}$ structure exhibits a $T_c$ of 190 K.
Stable structures include YMgH$_{2}$ and YMgH$_{3}$ at lower pressures.
Abstract
Motivated by recent discovery of yttrium-based high-temperature ternary superconducting hydrides (e.g., CaYH, LaYH, and ScYH), we have employed evolutionary algorithm and first-principles calculations to comprehensively examine the structural stability and superconductivity of the YMgH system at high pressure. The hydrogen content and the pressure are both important factors in the stability of these candidate structures. We find that the stability of hydrogen-rich materials frequently necessitates higher pressure. For instance, the pressures to stabilize -YMgH and -YMgH are both more than 250 GPa. Hydrogen-less materials, such as -YMgH and -YMgH, can be stable at pressures as low as 100 GPa. In addition, we find a metastable structure for YMgH with the same space group as the…
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