Carbon-Doped Sulfur Hydrides as Room-Temperature Superconductors at 270 GPa

Abstract

To understand the most-recent experiment on room-temperature superconductivity in carbonaceous sulfur hydride (CSH) systems under high pressure, we have performed extensive stoichiometry and structure searches of ternary CSH compounds using generic evolutionary algorithms. Judged from the formation enthalpy of different CSH compounds, our studies conclude that certain levels of carbon doping (~5%-6%) in sulfur hydride (H${}_3$S) in its R3m and phases gives rise to the most-stable structure (second to the H${}_3$S itself) among the various CSH systems found. The replacement of a small amount of sulfur atoms by carbon in compounds like C${}_1$S${}_{15}$H${}_{48}$ and C${}_1$S${}_{17}$H${}_{54}$ results in a stronger electron-phonon coupling and a higher averaged phonon frequency that increases with pressure, thereby leading to room-temperature superconductivity at ~270 GPa. The calculated superconducting transition temperature T${}_c$ of C${}_1$S${}_{15}$H${}_{48}$ and C${}_1$S${}_{17}$H${}_{54}$ as a function of pressure shows reasonably good agreement with experimental measurements. Before transition to superconducting states at ~80 GPa, the CSH system is predicted to have a stoichiometry of C${}_2$S${}_2$H${}_{10}$ with a stable structure of P1 symmetry, which is supported by the direct comparison of its Raman spectrum with experiment.

23 pages with 8 figures (with Supplementary Material)

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