Abstract

Titanium (Ti)-doped hematite (α-Fe2O3) films were grown in oxygen-depleted condition by using the spray pyrolysis technique. The impact of post-deposition annealing in oxygen-rich condition on both the conductivity and water splitting efficiency was investigated. The X-ray diffraction pattern revealed that the films are of rhombohedral α-Fe2O3 structure and dominantly directed along (012). The as-grown films were found to be highly conductive with electrons as the majority charge carriers (n-type), a carrier concentration of 1.09×1020 cm−3, and a resistivity of 5.9×10−2 Ω-cm. The conductivity of the films were reduced upon post-deposition annealing. The origin of the conductivity was attributed firstly to Ti4+ substituting Fe3+ and secondly to the ionized oxygen vacancies (VO) in the crystal lattice of hematite. Upon annealing the samples in oxygen-rich condition, VO slowly depleted and the conductivity reduced. The photocurrent of the as-grown samples was found to be 3.4 mA/cm−2 at 1.23 V vs. RHE. The solar-to-hydrogen efficiency for the as-grown sample was calculated to be 4.18% at 1.23 V vs. RHE. The photocurrents were found to be significantly stable in aqueous environment. A linear relationship between conductivity and water-splitting efficiency was established.

Highlights

  • The highest STH conversion efficiency for as-grown sample was calculated to be 4.18% at 1.23 V vs. RHE

  • The electrical conductivity was tuned as a function of post-deposition annealing temperature in oxygen-rich condition and we systematically investigated the origin of that change in conductivity by using spectroscopic measurements

  • It was concluded that ionized oxygen vacancies were induced in films that facilitated better conductivity as well as better STH efficiency in the samples

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Summary

Introduction

We have grown high quality and highly conductive n-type Ti-doped hematite films by spray pyrolysis. The electrical conductivity was tuned as a function of post-deposition annealing temperature in oxygen-rich condition and we systematically investigated the origin of that change in conductivity by using spectroscopic measurements.

Results
Conclusion

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