- Open Access
Ternary H-C-N compounds at high pressure featuring -hybridized C-N networks
Phys. Rev. B 114, 034109 – Published 7 July, 2026
DOI: https://doi.org/10.1103/8252-rnzw
Abstract
Hydrogen, carbon, and nitrogen are amongst the most important light elements in the composition of the solar system. They form the organic molecules and atmospheric components of many outer planets. Under the extreme conditions within planets, exploring the H-C-N chemical space is central to understanding the abiotic chemistry and interior structure of icy planets and moons. Here, based on effective crystal structure searches and ab initio calculations, we report the ground state phase diagram of the H-C-N system at pressures up to 500 GPa. Two thermodynamically stable ternary compounds and are predicted to maintain their stability up to the pressure of the mantle-core boundary of Neptune. Upon compression, both and benefit from the formation of a dense tetrahedrally connected network formed from hybridized carbon and nitrogen, supported by hydrogen bonding. The simplest possible compound, hydrogen cyanide HCN, is found to be metastable. Amongst methane-ammonia mixtures, we identify five metastable compounds: (((, and (. Potential synthesis pathways for the metastable compounds are provided for further discussion on the formation of mixtures based on simple molecules.
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