Hydrocarbons under pressure: phase diagrams and surprising new compounds in the C-H system
arXiv:1904.03135 · doi:10.1021/acs.jpcc.9b01353
Abstract
Understanding the high-pressure behavior of C-H system is of great importance due to its key role in organic, bio-, petroleum and planetary chemistry. We have performed a systematic investigation of the pressure-composition phase diagram of the C-H system at pressures up to 400 GPa using evolutionary structure prediction coupled with ab initio calculations and discovered that only saturated hydrocarbons are thermodynamically stable. Several stable methane-hydrogen co crystals are predicted: 2CH4 * H2, earlier obtained experimentally, is predicted to have I4/m space group and 2-90 GPa stability range at 0 K, and two new thermodynamically stable compounds 2CH4 * 7H2 (P-3m1 space group) and CH4 * 9H2 (Cm space group), as potential energy storage materials. P21/c phase of methane is predicted to be stable at pressures < 8 GPa; bulk graphane (CH) was shown to be thermodynamically stable at 7-18 and 18-50 GPa and 0 K in the P-3m and Cmca phases, respectively; polyethylene is shown to have a narrow field of stability. We report the p-T-x phase diagram of the C-H system and p-T phase diagram of CH4.
References in corpus (6)
- Van der Waals density functionals applied to solids
- Control of graphene's properties by reversible hydrogenation
- SCAN+rVV10: A promising van der Waals density functional
- The Melting Line of Hydrogen at High Pressures
- Bulk graphanes synthesized from benzene and pyridine
- The role of temperature and Coulomb correlation in stabilization of CsCl-phase in FeS under pressure
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