Ab initio prediction of ground-state magnetic ordering and high-pressure magnetic phase transition of uranium mononitride

The ground-state magnetic ordering of uranium mononitride (UN) remains a contentious topic due to the unexpected lack of crystallographic distortion in the traditionally accepted 1 k antiferromagnetic (AFM) state. This discrepancy casts doubt on the validity of the 1 k magnetic ordering of UN. Here,...

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Published inChinese physics B Vol. 34; no. 8; pp. 87101 - 87111
Main Authors Zheng, Jing-Jing, Chen, Yuxi, Zhao, Chengxiang, Zhang, Junfeng, Zhang, Ping, Wang, Bao-Tian, Ma, Jiang-Jiang
Format Journal Article
LanguageEnglish
Published Chinese Physical Society and IOP Publishing Ltd 01.08.2025
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Summary:The ground-state magnetic ordering of uranium mononitride (UN) remains a contentious topic due to the unexpected lack of crystallographic distortion in the traditionally accepted 1 k antiferromagnetic (AFM) state. This discrepancy casts doubt on the validity of the 1 k magnetic ordering of UN. Here, we investigate the crystal structure, high-pressure phase transitions, and dynamical and mechanical properties of UN in its 1 k and 3 k AFM ground states using density functional theory (DFT). Our results reveal that the undistorted 3 k AFM state of F m 3 ¯ m within the DFT + U + SOC scheme is more consistent with experimental results. The Hubbard U and spin–orbit coupling (SOC) are critical for accurately capturing the crystal structure, high-pressure structural phase transition, and dynamical properties of UN. In addition, we have identified a new high-pressure magnetic phase transition from the nonmagnetic (NM) phase of R 3 ¯ m to the P 6 3 / mmc AFM state. Electronic structure analysis reveals that the magnetic ordering in the ground state is primarily linked to variations in partial 5f orbital distributions. Our calculations provide valuable theoretical insights into the complex magnetic structures of a typical strongly correlated uranium-based compound. Moreover, they provide a framework for understanding other similar actinide systems.
ISSN:1674-1056
2058-3834
DOI:10.1088/1674-1056/add4e6