journal article·2016-09-09

Grain-Size-Limited Mobility in Methylammonium Lead Iodide Perovskite Thin Films

Obadiah G. Reid, Mengjin Yang, Nikos Kopidakis, Kai Zhu, Garry Rumbles

ACS Energy Letters· Volume 1· Issue 3
Publisher page

Abstract

We report a systematic study of the gigahertz-frequency charge carrier mobility found in methylammonium lead iodide perovskite films as a function of average grain size using time-resolved microwave conductivity and a single processing chemistry. Our measurements are in good agreement with the Kubo formula for the AC mobility of charges confined within finite grains, suggesting (1) that the surface grains imaged via scanning electron microscopy are representative of the true electronic domain size and not substantially subdivided by twinning or other defects not visible by microscopy and (2) that the time scale of diffusive transport across grain boundaries is much slower than the period of the microwave field in this measurement (∼100 ps). The intrinsic (infinite grain size) minimum mobility extracted form the model is 29 ± 6 cm 2 V –1 s –1 at the probe frequency (8.9 GHz).
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Research context

OpenAlex topics: Perovskite Materials and Applications · Organic and Molecular Conductors Research · Solid-state spectroscopy and crystallography

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

Affiliations

Chemistry and Nanoscience Center, National Renewable Energy Laboratory, 15013 Denver West Parkway, Golden, Colorado 80401, United States

Renewable and Sustainable Energy Institute, University of Colorado at Boulder, Boulder, Colorado 80309, United States

Department of Chemistry and Biochemistry, University of Colorado at Boulder, Boulder, Colorado 80309, United States

Funding

Basic Energy Sciences

References (32)

Show source-provided references
1. 10.1002/anie.20130871910.1002/anie.201308719 ↗
2. 10.1126/science.aad101510.1126/science.aad1015 ↗
3. 10.1126/science.aaa272510.1126/science.aaa2725 ↗
4. 10.1126/science.125476310.1126/science.1254763 ↗
5. 10.1126/science.122860410.1126/science.1228604 ↗
6. 10.1126/science.125830710.1126/science.1258307 ↗
7. 10.1038/nenergy.2016.4810.1038/nenergy.2016.48 ↗
8. 10.1038/nature1250910.1038/nature12509 ↗
9. 10.1021/acsenergylett.6b0006910.1021/acsenergylett.6b00069 ↗
10. 10.1038/nnano.2014.14910.1038/nnano.2014.149 ↗
11. 10.1038/nphoton.2016.6210.1038/nphoton.2016.62 ↗
12. 10.1038/nnano.2015.9010.1038/nnano.2015.90 ↗
13. 10.1039/C5NR08622A10.1039/C5NR08622A ↗
14. 10.1021/jp406706u10.1021/jp406706u ↗
15. 10.1126/science.aaa533310.1126/science.aaa5333 ↗
16. 10.1021/acs.jpclett.5b0136110.1021/acs.jpclett.5b01361 ↗
17. 10.1021/acs.jpclett.6b0026910.1021/acs.jpclett.6b00269 ↗
18. 10.1021/acs.jpclett.5b0248510.1021/acs.jpclett.5b02485 ↗
19. 10.1143/JPSJ.12.57010.1143/JPSJ.12.570 ↗
20. 10.1103/RevModPhys.72.87310.1103/RevModPhys.72.873 ↗
21. 10.1021/jp501087410.1021/jp5010874 ↗
22. 10.1002/pssb.20056271910.1002/pssb.200562719 ↗
23. 10.1103/PhysRevLett.96.14660110.1103/PhysRevLett.96.146601 ↗
24. 10.1021/jz201229a10.1021/jz201229a ↗
25. 10.1002/cphc.20130102210.1002/cphc.201301022 ↗
26. 10.1039/C5EE02503F10.1039/C5EE02503F ↗
27. 10.1038/ncomms890310.1038/ncomms8903 ↗
28. 10.1021/acs.accounts.5b0054010.1021/acs.accounts.5b00540 ↗
29. 10.1021/nl403514x10.1021/nl403514x ↗
30. 10.1021/ja506936f10.1021/ja506936f ↗
31. 10.1063/1.494834410.1063/1.4948344 ↗
32. 10.1002/adma.20150258610.1002/adma.201502586 ↗