Abstract

The energy landscape of helium-nitrogen mixtures is explored by ab initio evolutionary searches, which predicted several stable helium-nitrogen compounds in the pressure range from 25 to 100 GPa. In particular, the monoclinic structure of HeN22_{22} consists of neutral He atoms, partially ionic dimers N2_{2}δ−^{δ-}, and lantern-like cages N20_{20}δ+^{δ+}. The presence of helium not only greatly enhances structural diversity of nitrogen solids, but also tremendously lowers the formation pressure of nitrogen salt. The unique nitrogen framework of (HeN20_{20})δ+^{δ+}N2_{2}δ−^{δ-} may be quenchable to ambient pressure even after removing helium. The estimated energy density of N20_{20}δ+^{δ+}N2_{2}δ−^{δ-} (10.44 kJ/g) is ∼\sim2.4 times larger than that of trinitrotoluene (TNT), indicating a very promising high-energy-density material.

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