What superconducts in sulfur hydrides under pressure, and why
arXiv:1501.00196 · doi:10.1103/PhysRevB.91.060511
Abstract
The recent discovery of superconductivity at 190~K in highly compressed HS is spectacular not only because it sets a record high critical temperature, but because it does so in a material that appears to be, and we argue here that it is, a conventional strong-coupling BCS superconductor. Intriguingly, superconductivity in the observed pressure and temperature range was predicted theoretically in a similar compound HS. Several important questions about this remarkable result, however, are left unanswered: (1) Does the stoichiometry of the superconducting compound differ from the nominal composition, and could it be the predicted HS compound? (2) Is the physical origin of the anomalously high critical temperature related only to the high H phonon frequencies, or does strong electron-ion coupling play a role? We show that at experimentally relevant pressures HS is unstable, decomposing into HS and S, and that HS has a record high due to its covalent bonds driven metallic. The main reason for this extraordinarily high in HS as compared with MgB, another compound with a similar superconductivity mechanism, is the high vibrational frequency of the much lighter H atoms.
Supplementary material contains crystallographic information
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