Issue 47, 2025

Defect-enriched, active, self-supporting, coralline-like, high-entropy spinel oxide (FeNiCoMnCr)3O4 electrodes for high-stability oxygen evolution reaction

Abstract

High-entropy spinel oxides are promising catalysts for the oxygen evolution reaction due to their unique structures and high stability. However, developing defect-enriched, active, self-supporting, high-entropy spinel oxide electrodes is still a challenge. This study is the first to report defect-enriched, self-supporting, coralline-like, high-entropy spinel oxide (FeNiCoMnCr)3O4 electrodes (HEO-H500@NF) prepared using a synergistic approach integrating hydrothermal synthesis with hydrogen reduction. The optimized electrode exhibited excellent OER performance with an overpotential of 280 mV at 100 mA cm−2 and a small Tafel slope of 40.3 mV dec−1, superior to that of most high-entropy oxide catalysts reported so far. Additionally, the electrode maintained a stable overpotential of 280 mV at a current density of 100 mA cm−2 for 200 hours. Experimental and computational studies showed that the large number of oxygen vacancies on the surface of the HEO-H500@NF electrode was capable of enhancing the adsorption of the OER intermediates at active sites and reducing the energy barrier (formation of *O) of the rate-determining step, thus improving the OER performance. This study provides a new strategy for improving the OER performance of self-supporting, high-entropy oxide electrodes.

Graphical abstract: Defect-enriched, active, self-supporting, coralline-like, high-entropy spinel oxide (FeNiCoMnCr)3O4 electrodes for high-stability oxygen evolution reaction

Supplementary files

Article information

Article type
Paper
Submitted
28 Aug 2025
Accepted
29 Oct 2025
First published
30 Oct 2025

J. Mater. Chem. A, 2025,13, 41310-41320

Defect-enriched, active, self-supporting, coralline-like, high-entropy spinel oxide (FeNiCoMnCr)3O4 electrodes for high-stability oxygen evolution reaction

L. He, H. Zhao, H. Kang, H. Liu, K. Cui, J. Chen, W. Qin and X. Wu, J. Mater. Chem. A, 2025, 13, 41310 DOI: 10.1039/D5TA06995E

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