The systematic study on the stability and superconductivity of Y-Mg-H compounds under high pressure
arXiv:2107.05498 · doi:10.1002/adts.202100364
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 -YMgH. A metastable sodalite-like face-centered cubic (FCC) structure is also found in YMgH. These four clathrate structures of -YMgH, -YMgH, -YMgH, and -YMgH is made up of H14, H18, H24, and H24 cages, respectively, in which the H-H pair exhibits weak covalent bonding. According to phonon calculations, -YMgH and -YMgH require a pressure of 300 GPa to maintain dynamic stability, however -YMgH and -YMgH can maintain dynamic stability at pressures of 200 GPa and 250 GPa, respectively. Electron-phonon coupling calculations indicate that they might be potential high-temperature superconductors, with superconductivity intimately linked to the H cage structure. The sodalite structure -YMgH has a value of 190 K and a strong electron-phonon coupling constant of 2.18.
7 pages, 5 figures, 1 Supplemental Material
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