MRS Meetings and Events

 

EN02.08.02 2023 MRS Spring Meeting

Zinc Phosphide: a Promising Material for the Next Generation of Solar Cell Absorbers

When and Where

Apr 12, 2023
4:00pm - 4:30pm

Moscone West, Level 2, Room 2002

Presenter

Co-Author(s)

Mirjana Dimitrievska1,2,Anna Fontcuberta i Morral2

Empa–Swiss Federal Laboratories for Materials Science and Technology1,École Polytechnique Fédérale de Lausanne2

Abstract

Mirjana Dimitrievska1,2,Anna Fontcuberta i Morral2

Empa–Swiss Federal Laboratories for Materials Science and Technology1,École Polytechnique Fédérale de Lausanne2
The path towards the next generation of inexpensive and high efficiency solar cells is based on the utilization of earth-abundant, environmentally-friendly, and chemically stable materials. One promising candidate is zinc-phosphide (Zn<sub>3</sub>P<sub>2</sub>), with a direct bandgap of 1.5 eV, high absorption coefficient ( &gt; 10<sup>5</sup> cm<sup>-1</sup>), and excellent air stability. This work will present an overview of recent key findings related to the engineering of Zn<sub>3</sub>P<sub>2</sub> absorbers for incorporation into high-efficiency solar cell devices.<br/><br/>First part of the talk will focus on three different approaches for synthesizing high crystal quality Zn<sub>3</sub>P<sub>2</sub> thin films. These will include monocrystalline layer growth using molecular beam epitaxy [1], selective area epitaxy [2] and Van der Waals epitaxial growth on graphene substrates [3].<br/><br/>The second part of the talk will showcase the tunability of zinc-phosphide functional properties achieved by variation in the compositional stoichiometry [4,5]. In this case, we will show how electron and X-ray diffraction and Raman spectroscopy, along with density functional theory calculations, point to the favorable creation of P interstitial defects over Zn vacancies in P-rich and Zn-poor compositional regions. Photoluminescence and absorption measurements show that these defects create additional energy levels at about 180 meV above the valence band. Furthermore, they lead to the narrowing of the bandgap, due to the creation of band tails in the region of around 10–20 meV above the valence and below the conduction band. These results are also corroborated with the transport measurements on Zn<sub>3</sub>P<sub>2</sub> devices.<br/><br/>Finally, we will discuss the device architecture for a polycrystalline Zn3P2 thin film solar cell on an InP substrate with a 4.4 % conversion efficiency. We will show the dominant recombination mechanisms in the device using different techniques and identify the key factors that limit the device efficiency. Additionally, we will provide a perspective on the next-generation Zn<sub>3</sub>P<sub>2</sub>-based solar cells.<br/><br/>[1] M. Zamani et al. J. Phys. Energy 3 034011 (2021)<br/>[2] S. Escobar Steinvall et al., Nanoscale Adv., 3, 326-332 (2021)<br/>[3] R. Paul et al., Cryst. Growth Des., 20, 6, 3816–3825 (2020)<br/>[4] E. Z. Stutz et al. Faraday Discuss., 239, 202-218 (2022)<br/>[5] M. Dimitrievska et al. Adv. Funct. Mater. 31, 2105426 (2021)

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