Abstract
The search for more efficient visible light materials for solar-driven hydrogen production has brought metal oxides into the light of renewed scientific attention due to its high stability. Traditionally various n-type metal oxides have been studied for the photoelectrochemical cell (PEC) application as a photoanode such as TiO2, because of its low cost, high-corrosion resistance, and suitable band structure (for UV light). More and more efforts are focused on the development of visible active n-type semiconducting metal oxides, while very few p-type semiconducting oxides are known for the solar-to-fuel conversion. The fact that p-type semiconductor actually acting as the photocathode in the photoelectrochemical cell, which generates hydrogen, encourages us to investigate new p-type semiconducting oxides and challenges associated with it. The emphasis of this chapter will be on the strategies to make p-type semiconducting oxides for solar-to-fuel conversion. The main focus will be on copper-based p-type metal oxides (copper niobates and copper tantalates), with respect to the structure–property relationship, dopant effect, and electronic structure calculations using density of state (DOS).
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Joshi, U.A. (2014). New Cu(I)-Based p-Type Semiconducting Metal Oxides for Solar-to-Fuel Conversion: Investigation and Challenges. In: Viswanathan, B., Subramanian, V., Lee, J. (eds) Materials and Processes for Solar Fuel Production. Nanostructure Science and Technology, vol 174. Springer, New York, NY. https://doi.org/10.1007/978-1-4939-1628-3_5
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DOI: https://doi.org/10.1007/978-1-4939-1628-3_5
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