Recent Progress and Viability of PGM-Free Catalysts for Hydrogen Evolution Reaction and Hydrogen Oxidation Reaction

Wenjamin Moschkowitsch, Oran Lori, Lior Elbaz

Research output: Contribution to journalShort surveypeer-review

71 Scopus citations

Abstract

The field of precious metal group (PGM)-free hydrogen evolution reaction (HER) and hydrogen oxidation reaction (HOR) catalysts grew rapidly in recent years. There are several different approaches, from theoretical calculations and engineering of known materials. The mechanisms for HER and HOR can be broken down into distinct elemental steps. The difference between HER and HOR is the direction in which the reactions occur. In most PGM-free catalysts, the pathways may differ, the exact active site is not necessarily known and might consist of more than one atom or an edge site. Hence, it cannot be assumed that the mechanism will follow the exact same pathway, and more theoretical calculations and experiments are needed to determine the mechanism for each catalyst. PGM-free HOR catalysts in AEMFC can be divided into three classes, namely, metals and alloys; bioinspired macromolecules; and ceramics (mostly metal nitrides and oxides). A summary of PGM-free HER catalysts is provided. A true performance comparison of different catalysts is often difficult to attain especially when coming to ascertain the state-of-the-art, mostly due to lack of uniformity in reporting performance parameters and diversity in specific active site and site density estimation. Development of standard testing protocols, performance parameters, and benchmarks must be done to allow a fair comparison between PGM-free catalysts, which will surely help pave the way to their further development.

Original languageEnglish
Pages (from-to)1082-1089
Number of pages8
JournalACS Catalysis
Volume12
Issue number2
DOIs
StatePublished - 21 Jan 2022

Bibliographical note

Funding Information:
The authors would like to thank the Israeli Ministry of Science, The Israeli Ministry of Energy, and The Israeli Science Foundation for the financial support.

Funding

The authors would like to thank the Israeli Ministry of Science, The Israeli Ministry of Energy, and The Israeli Science Foundation for the financial support.

FundersFunder number
Israeli Ministry of Science
Israel Science Foundation
Ministry of Energy, Israel

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