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    Semimetal He-rich compounds at terapascal pressures

    Shengchao Qiu1,*, Hairui Ding1,*, Haixu Cui2, Shiyang Liu1, Xiang-Feng Zhou3,†, and Xiao Dong1,‡

    • 1Key Laboratory of Weak-Light Nonlinear Photonics and School of Physics, Nankai University, Tianjin 300071, China
    • 2College of Physics and Materials Science, Tianjin Normal University, Tianjin 300387, China
    • 3Center for High Pressure Science, State Key Laboratory of Metastable Materials Science and Technology, School of Science, Yanshan University, Qinhuangdao 066004, China

    • *These authors contributed equally to this work
    • †Contact author: xfzhou@ysu.edu.cn
    • ‡Contact author: xiao.dong@nankai.edu.cn

    Phys. Rev. B 114, 034114 – Published 27 July, 2026

    DOI: https://doi.org/10.1103/fb4n-y594

    Abstract

    Helium, which is on par with neon, is one of the most inert elements and most difficult elements for metallization in the periodic table. It requires more than 30 TPa to transit to an indirect metal. Here, via an ab initio evolutionary algorithm, we predict a semimetal helium–oxygen compound, He3O, which stabilizes at 5.74 TPa with topological nodal lines in its band structure. Further analysis revealed definite chemical bonding between the He and O atoms. Since helium and oxygen exist widely in the white dwarfs, He3O is quite important for understanding and modeling celestial bodies.

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