Organic compounds in metallic hydrogen
arXiv:2410.21772 · doi:10.21203/rs.3.rs-4618413/v1
Abstract
Metallic hydrogen is the most common condensed material in the universe, comprising the centre of gas giant planets. However, experimental studies are extremely challenging, and most of our understanding of this material has been led by theory. Chemistry in this environment has not been probed experimentally, so here we examine hydrocarbon chemistry in metallic hydrogen using density functional theory calculations. We find that carbon and oxygen react with metallic hydrogen to produce an entirely new type of hydrocarbon chemistry based on sixfold coordinated carbon with organic-style molecules CH6, C2H8, C3H10 OH3 NH4 and CH4OH. These are charged molecules stabilised by the metallic environment. Their associated electric fields are screened, giving oscillation in the surrounding electron and proton densities. In view of the excess hydrogen we refer to them as hypermethane, hyperethane etc. The relationship to traditional chemistry is that the metallic background acts as an electron donor and stabilizes negatively charged ions. This enables the formation of six covalent bonds per carbon atom, or three per oxygen atom. This demonstrates that organic chemistry may take place in very different environments from those found on earth, and may be common throughout the universe.
11 pages, 3 figures, submitted to Nature Communications
References in corpus (30)
- Phonons and related properties of extended systems from density-functional perturbation theory
- Optimized norm-conserving Vanderbilt pseudopotentials
- Conventional superconductivity at 203 K at high pressures
- Optimization Algorithm for the Generation of ONCV Pseudopotentials
- Thermal Contraction and Disordering of the Al(110) Surface
- Observation of the Wigner-Huntington Transition to Solid Metallic Hydrogen
- A Comparison of the Interiors of Jupiter and Saturn
- Thermophysical properties of warm dense hydrogen
- Zero-Temperature Structures of Atomic Metallic Hydrogen
- Jupiter models with improved ab initio hydrogen EOS (H-REOS.2)
- Ab Initio Equation of State for Hydrogen-Helium Mixtures with Recalibration of the Giant-Planet Mass-Radius Relation
- Density functional theory study of phase IV of solid hydrogen
- Evidence for supercritical behavior of high-pressure liquid hydrogen
- Rocky core solubility in Jupiter and giant exoplanets
- Benchmark of Exchange-Correlation Functionals for High Pressure Hydrogen using Quantum Monte Carlo
- Structure and metallicity of phase V of hydrogen
- Phase transitions in MgSiO3 post-perovskite in super-Earth mantles
- Understanding Jupiter's Interior
- Conductivity and Dissociation in Metallic Hydrogen: Implications for Planetary Interiors
- Ab initio studies of structural instabilities in magnesium silicate perovskite
- Benchmarking Hydrogen-Helium Mixtures with QMC: Energetics, Pressures, and Forces
- High-pressure behavior of dense hydrogen up to 3.5 TPa from density functional theory calculations
- Thermodynamic anomalies and three distinct liquid-liquid transitions in warm dense liquid hydrogen
- Unusual chemistry of the C-H-N-O system under pressure and implications for giant planets
- The role of van der Waals and exchange interactions in high-pressure solid hydrogen
- Striking Isotope Effect on the Metallization Phase Lines of Liquid Hydrogen and Deuterium
- A simple thermodynamic model for the hydrogen phase diagram
- Predicted reentrant melting of dense hydrogen at ultra-high pressures
- Isotope quantum effects in the metallization transition in liquid hydrogen
- The Observed Vibron Shift in Helium-Hydrogen Mixtures are due to Quantum Nuclear and Localisation Effects, not bonding