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Research Article | Open Access

Electronic structure and absorption mechanism of Fe-doped Y0.9Sr0.1CoO3 perovskite microwave absorbers

Jialing Wang1Haochen Qu1Xiangyu Ye1Shujuan Tan1( )Xin Yan1Pengze Li1Weizhi Tian2Guangbin Ji1 ( )
College of Materials Science and Technology, Nanjing University of Aeronautics and Astronautics, Nanjing 211100, China
Beijing Xinghang Electromechanical Equipment Co., Ltd., Beijing 100074, China
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Abstract

YCoO3 has unique advantages in functional applications owing to its exceptional lattice stability, valence adaptability, and environmental resistance; however, its potential for microwave absorption remains largely unexplored. In this study, Y0.9Sr0.1Co1−xFexO3 (x = 0–0.2) perovskite absorbers were synthesized via a sol–gel method, which demonstrated superior microwave absorption performance. Oxygen vacancy engineering facilitates Co redox cycling, significantly enhancing oxygen ion mobility and conductivity loss. First-principles calculations revealed that Fe3+doping not only intensifies crystal polarization but also improves magnetic properties, thereby synergistically optimizing dipole polarization and magnetic losses. Additionally, the nanoscale particle morphology enhances the interfacial polarization effects. The optimal composition (x = 0.1) achieves an effective absorption bandwidth (EAB) of 5.71 GHz with a reflection loss (RL) of −47.18 dB at a thickness below 1.8 mm, demonstrating a significant enhancement over that of the undoped material. This work provides new insights into the design of ultrathin, high-performance absorbers while elucidating the fundamental loss mechanisms in perovskite-based systems.

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Journal of Advanced Ceramics
Article number: 9221191

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Cite this article:
Wang J, Qu H, Ye X, et al. Electronic structure and absorption mechanism of Fe-doped Y0.9Sr0.1CoO3 perovskite microwave absorbers. Journal of Advanced Ceramics, 2025, 14(12): 9221191. https://doi.org/10.26599/JAC.2025.9221191
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Received: 08 July 2025
Revised: 15 September 2025
Accepted: 09 October 2025
Published: 24 December 2025
© The Author(s) 2025.

This is an open access article under the terms of the Creative Commons Attribution 4.0 International License (CC BY 4.0, http://creativecommons.org/licenses/by/4.0/).