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Volume 11 Issue 1
Jan.  2026
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Article Contents
Chen Bo, Zeng Qiyu, Yu Xiaoxiang, Chen Jiahao, Zhang Shen, Kang Dongdong, Dai Jiayu. Three-step formation of diamonds in shock-compressed hydrocarbons: Dissociation, species separation, and nucleation[J]. Matter and Radiation at Extremes, 2026, 11(1): 017603. doi: 10.1063/5.0273729
Citation: Chen Bo, Zeng Qiyu, Yu Xiaoxiang, Chen Jiahao, Zhang Shen, Kang Dongdong, Dai Jiayu. Three-step formation of diamonds in shock-compressed hydrocarbons: Dissociation, species separation, and nucleation[J]. Matter and Radiation at Extremes, 2026, 11(1): 017603. doi: 10.1063/5.0273729

Three-step formation of diamonds in shock-compressed hydrocarbons: Dissociation, species separation, and nucleation

doi: 10.1063/5.0273729
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  • Corresponding author: a)Author to whom correspondence should be addressed: jydai@nudt.edu.cn
  • Received Date: 2025-04-01
  • Accepted Date: 2025-10-30
  • Available Online: 2026-01-01
  • Publish Date: 2026-01-01
  • The accumulation and circulation of carbon and hydrogen contribute to the chemical evolution of ice giant planets. Species separation and diamond precipitation have been reported in carbon–hydrogen systems and have been verified by static and shock compression experiments. Nevertheless, the dynamic formation processes underlying these phenomena remain insufficiently understood. In combination with a deep learning model, we demonstrate that diamonds form through a three-step process involving dissociation, species separation, and nucleation processes. Under shock conditions of 125 GPa and 4590 K, hydrocarbons decompose to give hydrogen and low-molecular-weight alkanes (CH4 and C2H6), which escape from the carbon chains, resulting in C/H species separation. The remaining carbon atoms without C–H bonds accumulate and nucleate to form diamond crystals. The process of diamond growth is associated with a critical nucleus size at which the dynamic energy barrier plays a key role. These dynamic processes of diamond formation provide insight into the establishment of a model for the evolution of ice giant planets.
  • The authors have no conflicts to disclose.
    Conflict of Interest
    Bo Chen: Conceptualization (lead); Data curation (lead); Formal analysis (equal); Investigation (lead); Methodology (lead); Validation (equal); Visualization (lead); Writing – original draft (lead); Writing – review & editing (equal). Qiyu Zeng: Conceptualization (equal); Data curation (equal); Formal analysis (supporting); Investigation (supporting); Methodology (equal); Validation (equal); Visualization (equal); Writing – review & editing (equal). Xiaoxiang Yu: Conceptualization (supporting); Formal analysis (equal); Validation (equal); Visualization (equal); Writing – review & editing (supporting). Jiahao Chen: Formal analysis (equal); Validation (supporting); Visualization (supporting); Writing – review & editing (supporting). Shen Zhang: Formal analysis (supporting); Methodology (supporting); Validation (supporting); Writing – review & editing (supporting). Dongdong Kang: Formal analysis (supporting); Funding acquisition (supporting); Validation (supporting); Writing – review & editing (supporting). Jiayu Dai: Conceptualization (equal); Data curation (equal); Funding acquisition (lead); Project administration (lead); Resources (lead); Supervision (lead); Writing – review & editing (lead).
    Author Contributions
    The data that support the findings of this study are available from the corresponding author upon reasonable request.
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