Structure and composition of C-S-H compounds up to 143 GPa
Elena Bykova, Maxim Bykov, Stella Chariton, Vitali B. Prakapenka,, Konstantin Glazyrin, Andrey Aslandukov, Alena Aslandukova, Giacomo Criniti,, Alexander Kurnosov, Alexander F. Goncharov

TL;DR
This study investigates the high-pressure structural evolution of C-S-H compounds synthesized from carbon, sulfur, methane, and hydrogen, revealing complex phase behavior and structural differences from known superconducting hydrides.
Contribution
It provides new insights into the structure and composition of C-S-H compounds up to 143 GPa, highlighting their distinct differences from H3S superconductors.
Findings
Both samples exhibit Al2Cu type I4/mcm symmetry.
Hydrogen subsystem shows pressure-induced ordering and modifications.
Methane-bearing sample transitions to orthorhombic Pnma structure at high pressure.
Abstract
We synthesized two C-S-H compounds from a mixture of carbon and sulfur in hydrogen and from sulfur in mixed methane-hydrogen fluids at 4 GPa. X-ray synchrotron single-crystal diffraction and Raman spectroscopy have been applied to these samples up to 58 and 143 GPa, respectively. Both samples show a similar Al2Cu type I4/mcm basic symmetry, while the hydrogen subsystem evolves with pressure via variously ordered molecular and extended modifications. The methane bearing sample lowers symmetry to an orthorhombic Pnma structure after laser heating to 1400 K at 143 GPa. The results suggest that superconducting C-S-H compounds are structurally different from a common Im-3m H3S.
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