Wide and ultra-wide bandgap oxides : where paradigm-shift photovoltaics meets transparent power electronics
Perez-Tomas, Amador (Institut Català de Nanociència i Nanotecnologia)
Chikoidze, Ekaterine (Université de Versailles Saint Quentin en Yvelines - CNRS)
Jennings, M. R. (University of Warwick)
Russell, Stephen A. O. (University of Warwick)
Teherani, Féréchteh Hosseini (Nanovation)
Bove, Philippe (Nanovation)
Sandana, Vinod E. (Nanovation)
Rogers, David J. (Nanovation)

Data:	2018
Resum:	Oxides represent the largest family of wide bandgap (WBG) semiconductors and also offer a huge potential range of complementary magnetic and electronic properties, such as ferromagnetism, ferroelectricity, antiferroelectricity and high-temperature superconductivity. Here, we review our integration of WBG and ultra WBG semiconductor oxides into different solar cells architectures where they have the role of transparent conductive electrodes and/or barriers bringing unique functionalities into the structure such above bandgap voltages or switchable interfaces. We also give an overview of the state-of-the-art and perspectives for the emerging semiconductor β- GaO, which is widely forecast to herald the next generation of power electronic converters because of the combination of an UWBG with the capacity to conduct electricity. This opens unprecedented possibilities for the monolithic integration in solar cells of both self-powered logic and power electronics functionalities. Therefore, WBG and UWBG oxides have enormous promise to become key enabling technologies for the zero emissions smart integration of the internet of things.
Ajuts:	Ministerio de Economía y Competitividad ENE2015-74275-JIN Ministerio de Economía y Competitividad SEV-2013-0295
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Llengua:	Anglès
Document:	Article ; recerca ; Versió sotmesa a revisió
Matèria:	Ultra Wide Bandgap Semiconductors ; Oxides ; Solar Cells ; Ferroelectricity ; Power Electronics
Publicat a:	Proceedings of SPIE, Vol. 10533 (February 2018) , art. 105331Q, ISSN 1996-756X

DOI: 10.1117/12.2302576

Preprint 15 p, 1.1 MB

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