MRS Meetings and Events

 

EN02.03.05 2023 MRS Spring Meeting

Chemical and Electronic Properties of the MgxZn1-xO/CuGa3Se5 Interface with a Cd2+-Treatment

When and Where

Apr 11, 2023
4:45pm - 5:00pm

Moscone West, Level 2, Room 2002

Presenter

Co-Author(s)

Mary Blankenship1,Brooklynne Jacobellis1,Dirk Hauschild1,2,Lothar Weinhardt1,2,Imran Khan3,Christopher Muzzillo3,Andriy Zakutayev3,Nicolas Gaillard4,Clemens Heske1,2

University of Nevada, Las Vegas1,Karlsruhe Institute of Technology2,National Renewable Energy Laboratory3,University of Hawai‘i at Mānoa4

Abstract

Mary Blankenship1,Brooklynne Jacobellis1,Dirk Hauschild1,2,Lothar Weinhardt1,2,Imran Khan3,Christopher Muzzillo3,Andriy Zakutayev3,Nicolas Gaillard4,Clemens Heske1,2

University of Nevada, Las Vegas1,Karlsruhe Institute of Technology2,National Renewable Energy Laboratory3,University of Hawai‘i at Mānoa4
Ordered-vacancy wide band gap CuGa<sub>3</sub>Se<sub>5</sub> is a promising candidate as absorber material for the top cell in tandem solar cells as well as in photoelectrochemical water-splitting devices. For wide band gap absorber materials, it is increasingly important to also use a wide band gap buffer layer to avoid absorption losses. Instead of the traditionally used CdS buffer layer, a conductive oxide Mg<sub>x</sub>Zn<sub>1-x</sub>O (MZO) was thus chosen in this study, deposited by RF sputtering on the absorber. To further improve the interface properties, a Cd<sup>2+</sup> partial electrolyte treatment (CdPE) can be applied to the CuGa<sub>3</sub>Se<sub>5</sub> surface prior to MZO layer deposition. Further optimization of the interface requires a more detailed understanding of the chemical and electronic properties at the MZO/absorber interface, such as the band edge positions, band gaps at the interface and, in particular, the band alignment.<br/><br/>In this contribution, we investigate the CuGa<sub>3</sub>Se<sub>5</sub> absorber after CdPE, as well as its interface with the MZO layer using a toolchest of electron spectroscopies, including laboratory-based x-ray and UV photoelectron spectroscopy (XPS and UPS), x-ray-excited Auger electron spectroscopy (XAES), and inverse photoemission spectroscopy (IPES). With this combination of techniques, a detailed electronic and chemical picture of the interface is painted and will be discussed in view of its impact on the performance of CuGa<sub>3</sub>Se<sub>5</sub> solar devices.

Keywords

electronic structure | interface | thin film

Symposium Organizers

Eric Colegrove, National Renewable Energy Laboratory
Jessica de Wild, imec
Byungha Shin, Korea Advanced Institute of Science and Technology
Colin Wolden, Colorado School of Mines

Publishing Alliance

MRS publishes with Springer Nature