journal article·2017-10-13Open access

High-Resolution Study of TiO2 Contact Layer Thickness on the Performance of Over 800 Perovskite Solar Cells

Laxman Gouda, Kevin J. Rietwyk, Jiangang Hu, Adi Kama, Adam Ginsburg, Maayan Priel, David A. Keller, Shay Tirosh, Simcha Meir, Ronen Gottesman, Arie Zaban

ACS Energy Letters· Volume 2· Issue 10

Abstract

In this Letter, we systematically explore the influence of TiO 2 thickness with nanometric variations over a range of 20–600 nm on the photovoltaic parameters (open-circuit voltage, short circuit current, fill-factor, and power conversion efficiency) of CH 3 NH 3 PbI 3 -based solar cells. We fabricate several sample libraries of 13 × 13 solar cells on large substrates with spatial variations in the thickness of the TiO 2 layers while maintaining similar properties for the other layers. We show that the optimal thickness is ∼50 nm for maximum performance; thinner layers typically resulted in short-circuited cells, whereas increasing the thickness led to a monotonic decrease in performance. Furthermore, by assuming a fixed bulk resistivity of TiO 2, we were able to correlate the TiO 2 thickness to the series and shunt resistances of the devices and model the variation in the photovoltaic parameters with thickness using the diode equation to gain quantitative insights.
Source: openalex_inverted_index · Quality: baseline

Research context

OpenAlex topics: Perovskite Materials and Applications · Chalcogenide Semiconductor Thin Films · Quantum Dots Synthesis And Properties

SciVX discovery tags are terminology-based. OpenAlex topics are source-provided classifications.

Affiliations

Department of Chemistry, Institute for Nanotechnology & Advanced Materials, Bar-Ilan University, Ramat Gan 5290000, Israel

Funding

H2020 Marie Sklodowska-Curie Actions · Seventh Framework Programme

References (29)

Show source-provided references
1. 10.1021/acsnano.6b0261310.1021/acsnano.6b02613 ↗
2. 10.1038/353737a010.1038/353737a0 ↗
3. 10.1021/jz401549e10.1021/jz401549e ↗
4. 10.1021/jp305026h10.1021/jp305026h ↗
5. 10.1126/science.122860410.1126/science.1228604 ↗
6. 10.1038/srep0059110.1038/srep00591 ↗
7. 10.1038/nature1234010.1038/nature12340 ↗
8. 10.1039/C5EE03874J10.1039/C5EE03874J ↗
9. 10.1039/C4RA03981E10.1039/C4RA03981E ↗
10. 10.1021/acs.jpcc.5b0278410.1021/acs.jpcc.5b02784 ↗
11. 10.1002/adma.20160374710.1002/adma.201603747 ↗
12. 10.1002/aenm.20140177510.1002/aenm.201401775 ↗
13. 10.1021/acs.jpclett.5b0028910.1021/acs.jpclett.5b00289 ↗
14. 10.1021/acs.jpcc.6b0423310.1021/acs.jpcc.6b04233 ↗
15. 10.1021/jz500059v10.1021/jz500059v ↗
16. 10.1016/j.orgel.2016.11.01710.1016/j.orgel.2016.11.017 ↗
17. 10.1016/j.jallcom.2016.10.10610.1016/j.jallcom.2016.10.106 ↗
18. 10.1246/cl.16005910.1246/cl.160059 ↗
19. 10.1002/adma.20150604910.1002/adma.201506049 ↗
20. 10.1016/j.mssp.2014.07.03910.1016/j.mssp.2014.07.039 ↗
21. 10.1002/admi.20150083710.1002/admi.201500837 ↗
22. 10.1021/acs.jpcc.6b0116410.1021/acs.jpcc.6b01164 ↗
23. 10.1021/co300158310.1021/co3001583 ↗
24. 10.1039/C5NR08658B10.1039/C5NR08658B ↗
25. 10.1039/C6TA05869H10.1039/C6TA05869H ↗
26. 10.1039/C5TA03686K10.1039/C5TA03686K ↗
27. 10.1260/1708-5284.11.2.11110.1260/1708-5284.11.2.111 ↗
28. 10.1063/1.486463810.1063/1.4864638 ↗
29. 10.1063/1.490151010.1063/1.4901510 ↗