journal article·2025-06-19

Direct Observation of Orbital Hybridization Evolution in BAs

Jingwei Dong, Yingxin Zhang, Yunbo Wu, Zhe Sun, Zhongwei Chen

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Abstract

Boron arsenide (BAs) has a coefficient of thermal expansion comparable to that of common semiconductor materials like silicon, which helps prevent device damage or performance degradation due to thermal expansion mismatch. Understanding the evolution of electron orbital hybridization near the Fermi level as temperature varies is vital for elucidating the thermal and electrical properties of BAs crystals. Despite its significance, this topic has not been reported until now. In this study, ultraviolet photoelectron spectroscopy (UPS) was employed to measure the occupied electronic states near the Fermi level in BAs. The compositional ratio of the σ and π bands comprising the electronic states, as well as their binding energies, was found to vary with temperature. Density functional theory (DFT) calculations reveal that temperature-dependent orbital hybridization can be attributed to the evolution of phonon scattering strength.
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Research context

OpenAlex topics: Thermal properties of materials · Boron and Carbon Nanomaterials Research · Advanced Thermoelectric Materials and Devices

SciVX discovery tags are terminology-based. OpenAlex topics are source-provided classifications.

Affiliations

Power Battery & Systems Research Center, Dalian Institute of Chemical Physics

Chinese Academy of Sciences

State Key Laboratory of Catalysis, Dalian Institute of Chemical Physics

State Key Laboratory of Superhard Materials, Key Laboratory of Automobile Materials of MOE, and School of Materials Science and Engineering

Jilin University

National Synchrotron Radiation Laboratory

University of Science and Technology of China

Funding

Natural Science Foundation of Liaoning Province · National Natural Science Foundation of China · Chinese Academy of Sciences · Yulin Innovation Institute of Clean Energy

References (26)

Show source-provided references
1. 10.1063/1.510316610.1063/1.5103166 ↗
2. 10.3390/app1314830110.3390/app13148301 ↗
3. 10.1016/j.diamond.2023.11005510.1016/j.diamond.2023.110055 ↗
4. 10.1039/D3RA00898C10.1039/D3RA00898C ↗
5. 10.1088/1402-4896/abe0f110.1088/1402-4896/abe0f1 ↗
6. 10.1103/PhysRevApplied.11.06407010.1103/PhysRevApplied.11.064070 ↗
7. 10.1103/PhysRevLett.111.02590110.1103/PhysRevLett.111.025901 ↗
8. 10.1126/science.aat552210.1126/science.aat5522 ↗
9. 10.1126/science.abn472710.1126/science.abn4727 ↗
10. 10.1126/science.aat793210.1126/science.aat7932 ↗
11. 10.1126/science.115972510.1126/science.1159725 ↗
12. 10.1002/anie.20200394610.1002/anie.202003946 ↗
13. 10.1002/aelm.20160001910.1002/aelm.201600019 ↗
14. 10.1016/j.mtphys.2020.10029810.1016/j.mtphys.2020.100298 ↗
15. 10.1021/jacs.5b1327610.1021/jacs.5b13276 ↗
16. 10.1016/j.commatsci.2020.10988710.1016/j.commatsci.2020.109887 ↗
17. 10.1063/1.505813410.1063/1.5058134 ↗
18. 10.1002/admt.20240214610.1002/admt.202402146 ↗
19. 10.1063/1.506284510.1063/1.5062845 ↗
20. 10.1103/PhysRevB.89.02430810.1103/PhysRevB.89.024308 ↗
21. Li S. · SPECTROSC SPECT ANAL · 2022 · 42 · 454
22. 10.1103/PhysRevLett.132.11630110.1103/PhysRevLett.132.116301 ↗
23. 10.1103/PhysRevB.77.03542710.1103/PhysRevB.77.035427 ↗
24. Liu J. · J. Synth. Cryst. · 2021 · 391
25. 10.1088/0953-8984/14/11/30110.1088/0953-8984/14/11/301 ↗
26. 10.1103/PhysRevLett.77.386510.1103/PhysRevLett.77.3865 ↗