2019
DOI: 10.1021/acsanm.8b01936
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Electronically-Coupled Phase Boundaries in α-Fe2O3/Fe3O4 Nanocomposite Photoanodes for Enhanced Water Oxidation

Abstract: Photoelectrochemical (PEC) water splitting reactions are promising for sustainable hydrogen production from renewable sources. We report here, the preparation of α-Fe 2 O 3 /Fe 3 O 4 composite films via a single-step chemical vapor deposition of [Fe(O t Bu) 3 ] 2 and their use as efficient photoanode materials in PEC setups. Film thickness and phase segregation was controlled by varying the deposition time and corroborated through cross-section Raman spectroscopy and scanning electron microscopy. The highest w… Show more

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Cited by 33 publications
(29 citation statements)
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“…According to previous reports, the peak position of Fe 2p 3/2 is between 710.6 and 711.2 eV, and the area of the Fe 2p 3/2 peak is greater than that of Fe 2p 1/2 . The Fe 2p 3/2 peak has also been associated with a satellite peak located approximately 8 eV higher than the main Fe 2p 3/2 peak for α-Fe 2 O 3 , and Fe 2p 3/2 of Fe 3 O 4 does not have a satellite peak. , Therefore, the presence of the satellite peak at 718.8 eV in Figure A confirms the existence of α-Fe 2 O 3 ; and after reaction, the weakening of the satellite peak implies the reduction of α-Fe 2 O 3 Furthermore, the peak position of Fe 2p 3/2 moves downward after reaction, which can be attributed to the formation of Fe 2+ 2p 3/2 of Fe 3 O 4 . The XPS spectra thus indicate the reduction of α-Fe 2 O 3 to Fe 3 O 4 during the reaction.…”
mentioning
confidence: 83%
See 1 more Smart Citation
“…According to previous reports, the peak position of Fe 2p 3/2 is between 710.6 and 711.2 eV, and the area of the Fe 2p 3/2 peak is greater than that of Fe 2p 1/2 . The Fe 2p 3/2 peak has also been associated with a satellite peak located approximately 8 eV higher than the main Fe 2p 3/2 peak for α-Fe 2 O 3 , and Fe 2p 3/2 of Fe 3 O 4 does not have a satellite peak. , Therefore, the presence of the satellite peak at 718.8 eV in Figure A confirms the existence of α-Fe 2 O 3 ; and after reaction, the weakening of the satellite peak implies the reduction of α-Fe 2 O 3 Furthermore, the peak position of Fe 2p 3/2 moves downward after reaction, which can be attributed to the formation of Fe 2+ 2p 3/2 of Fe 3 O 4 . The XPS spectra thus indicate the reduction of α-Fe 2 O 3 to Fe 3 O 4 during the reaction.…”
mentioning
confidence: 83%
“…19,20 Therefore, the presence of the satellite peak at 718.8 eV in Figure 3A confirms the existence of α-Fe 2 O 3 ; and after reaction, the weakening of the satellite peak implies the reduction of α-Fe 2 O 3 Furthermore, the peak position of Fe 2p 3/2 moves downward after reaction, which can be attributed to the formation of Fe 2+ 2p 3/2 of Fe 3 O 4 . 21 The XPS spectra thus indicate the reduction of α-Fe 2 O 3 to Fe 3 O 4 during the reaction.…”
mentioning
confidence: 94%
“…These factors lead to an enhancement of the photocurrent density up to 0.48 mA cm −2 at 1.23 V (vs RHE), despite a film thickness of 11 μm. [ 123 ]…”
Section: Morphologymentioning
confidence: 99%
“…After a long period of research, Al-Kuhaili et al [7] found that hematite α-Fe 2 O 3 had a 2.18 eV direct band gap, which theoretically allows the utilization of approximately 40% of the solar spectrum. However, the actual conversion efficiency of solar energy is not ideal due to poor performance, such as a very short excited-state lifetime [8][9][10], relatively poor absorptivity [11,12] and poor oxygen evolution reaction kinetics [13]. Therefore, improving the properties of α-Fe 2 O 3 becomes hard work.…”
Section: Introductionmentioning
confidence: 99%