Copper oxides are promising photocathodes for solar hydrogen production, but the role of the metastable intermediate phase, paramelaconite (Cu 4 O 3 ), remains obscure due to its narrow thermodynamic stability window. Herein, we report the controllable synthesis of pure Cu 2 O, Cu 4 O 3 and CuO thin films via radio-frequency reactive magnetron sputtering by precisely manipulating the oxygen partial pressure. A systematic phase diagram was established to isolate the challenging Cu 4 O 3 phase, facilitating comprehensive comparative studies of the inherent correlations between crystal structure, electronic properties, and photoelectrochemical (PEC) behaviors. Mott-Schottky plots and band alignment analysis reveal that Cu 2 O exhibits the most favorable electronic properties, featuring the highest hole carrier density (∼ 3.1 × 10 19 cm −3 ) and the most negative conduction band potential, providing the strongest thermodynamic driving force for hydrogen evolution. In contrast, although the Cu 4 O 3 also demonstrates a high carrier density (∼ 2.7 × 10 19 cm −3 ), comprehensive PEC evaluations identify its rapid surface recombination and significant photocorrosion. This stems from a high density of deep-level traps acting as recombination centers, which drives severe surface charge recombination and consequently triggers rapid photocorrosion. Conversely, the Cu 2 O phase shows superior kinetic stability with rectangular photoresponses and distinctive self-activation behavior. This work unravels the trade-off between conductivity and stability, affirming that the defect tolerance and phase purity of Cu 2 O render it as the optimal candidate material for durable solar water splitting.
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Wang et al. (2026) studied this question.
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