Abstract
An essential step in the development of a new photovoltaic (PV) technology is choosing appropriate electron and hole extraction layers to make an efficient device. We recently proposed the minerals enargite ( Cu 3 AsS 4) and bournonite ( CuPbSbS 3) as materials that are chemically stable with desirable optoelectronic properties for use as the absorber layer in a thin-film PV device. For these compounds, spontaneous lattice polarization with internal electric fields - and potential ferroelectricity - may allow for enhanced carrier separation and novel photophysical effects. In this work, we calculate the ionization potentials for non-polar surface terminations and propose suitable partners for forming solar cell heterojunctions by matching the electronic band edges to a set of candidate electrical materials. We then further screen these candidates by matching the lattice constants and identify those that are likely to minimise strain and achieve epitaxy. This two-step screening procedure identified a range of unconventional candidate junction partners including SnS 2, ZnTe, WO 3, and Bi 2 O 3.
Original language | English |
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Article number | 055703 |
Journal | Journal of Applied Physics |
Volume | 125 |
Issue number | 5 |
DOIs | |
Publication status | Published - 2019 Feb 7 |
Bibliographical note
Funding Information:We thank Jake Bowers, Elisabetta Arca, Ji-Sang Park, and Lee Burton for useful discussions. This work has been supported by the Engineering and Physical Sciences Research Council (EPSRC) (Grant Nos. EP/L016354/1 and EP/K016288/1). This work benefited from access to ARCHER, the UK’s national high-performance computing service, which is funded by the Office of Science and Technology through EPSRC’s High End Computing Programme (No. EP/L000202). This work was also supported by a National Research Foundation of Korea (NRF) the Korean government (MSIT) (No. 2018R1C1B6008728).This study used the MacroDensity
Funding Information:
We thank Jake Bowers, Elisabetta Arca, Ji-Sang Park, and Lee Burton for useful discussions. This work has been supported by the Engineering and Physical Sciences Research Council (EPSRC) (Grant Nos. EP/L016354/1 and EP/K016288/1). This work benefited from access to ARCHER, the UK’s national high-performance computing service, which is funded by the Office of Science and Technology through EPSRC’s High End Computing Programme (No. EP/L000202). This work was also supported by a National Research Foundation of Korea (NRF) grant funded by the Korean government (MSIT) (No. 2018R1C1B6008728).
Publisher Copyright:
© 2019 Author(s).
All Science Journal Classification (ASJC) codes
- Physics and Astronomy(all)