The Oxygen Evolution Reaction Drives Passivity Breakdown for Ni–Cr–Mo AlloysShow others and affiliations
2023 (English)In: Advanced Materials, ISSN 0935-9648, E-ISSN 1521-4095, Vol. 35, no 39, article id 2304621Article in journal (Refereed) Published
Abstract [en]
Corrosion is the main factor limiting the lifetime of metallic materials, and a fundamental understanding of the governing mechanism and surface processes is difficult to achieve since the thin oxide films at the metal–liquid interface governing passivity are notoriously challenging to study. In this work, a combination of synchrotron-based techniques and electrochemical methods is used to investigate the passive film breakdown of a Ni–Cr–Mo alloy, which is used in many industrial applications. This alloy is found to be active toward oxygen evolution reaction (OER), and the OER onset coincides with the loss of passivity and severe metal dissolution. The OER mechanism involves the oxidation of Mo4+ sites in the oxide film to Mo6+ that can be dissolved, which results in passivity breakdown. This is fundamentally different from typical transpassive breakdown of Cr-containing alloys where Cr6+ is postulated to be dissolved at high anodic potentials, which is not observed here. At high current densities, OER also leads to acidification of the solution near the surface, further triggering metal dissolution. The OER plays an important role in the mechanism of passivity breakdown of Ni–Cr–Mo alloys due to their catalytic activity, and this effect needs to be considered when studying the corrosion of catalytically active alloys.
Place, publisher, year, edition, pages
Wiley , 2023. Vol. 35, no 39, article id 2304621
Keywords [en]
corrosion mechanisms, nickel alloys, Ni–Cr–Mo, oxygen evolution reaction, passivity breakdown, transpassive dissolution
National Category
Materials Chemistry
Identifiers
URN: urn:nbn:se:kth:diva-338521DOI: 10.1002/adma.202304621ISI: 001041483900001PubMedID: 37437599Scopus ID: 2-s2.0-85166340549OAI: oai:DiVA.org:kth-338521DiVA, id: diva2:1811848
Note
QC 20231114
2023-11-142023-11-142024-05-02Bibliographically approved