Cs x FA1- xPb(I1- yBr y)3 Perovskite Compositions : The Appearance of Wrinkled Morphology and its Impact on Solar Cell Performance
(2018) In Journal of Physical Chemistry C 122(30). p.17123-17135- Abstract
We report on the formation of wrinkle-patterned surface morphologies in cesium formamidinium-based CsxFA1-xPb(I1-yBry)3 perovskite compositions with x = 0-0.3 and y = 0-0.3 under various spin-coating conditions. By varying the Cs and Br contents, the perovskite precursor solution concentration and the spin-coating procedure, the occurrence and characteristics of the wrinkle-shaped morphology can be tailored systematically. Cs0.17FA0.83Pb(I0.83Br0.17)3 perovskite layers were analyzed regarding their surface roughness, microscopic structure, local and overall composition, and optoelectronic properties. Application of these films... (More)
We report on the formation of wrinkle-patterned surface morphologies in cesium formamidinium-based CsxFA1-xPb(I1-yBry)3 perovskite compositions with x = 0-0.3 and y = 0-0.3 under various spin-coating conditions. By varying the Cs and Br contents, the perovskite precursor solution concentration and the spin-coating procedure, the occurrence and characteristics of the wrinkle-shaped morphology can be tailored systematically. Cs0.17FA0.83Pb(I0.83Br0.17)3 perovskite layers were analyzed regarding their surface roughness, microscopic structure, local and overall composition, and optoelectronic properties. Application of these films in p-i-n perovskite solar cells (PSCs) with indium-doped tin oxide/NiOx/perovskite/C60/bathocuproine/Cu architecture resulted in up to 15.3 and 17.0% power conversion efficiency for the flat and wrinkled morphology, respectively. Interestingly, we find slightly red-shifted photoluminescence (PL) peaks for wrinkled areas and we are able to directly correlate surface topography with PL peak mapping. This is attributed to differences in the local grain size, whereas there is no indication for compositional demixing in the films. We show that the perovskite composition, crystallization kinetics, and layer thickness strongly influence the formation of wrinkles which is proposed to be related to the release of compressive strain during perovskite crystallization. Our work helps us to better understand film formation and to further improve the efficiency of PSCs with widely used mixed-perovskite compositions.
(Less)
- author
- publishing date
- 2018-08-02
- type
- Contribution to journal
- publication status
- published
- in
- Journal of Physical Chemistry C
- volume
- 122
- issue
- 30
- pages
- 13 pages
- publisher
- The American Chemical Society (ACS)
- external identifiers
-
- scopus:85049915528
- ISSN
- 1932-7447
- DOI
- 10.1021/acs.jpcc.8b06459
- language
- English
- LU publication?
- no
- id
- 7a3ceee0-527c-4e38-b2ed-dc2fe646cd7a
- date added to LUP
- 2020-01-19 14:53:31
- date last changed
- 2022-04-18 20:15:43
@article{7a3ceee0-527c-4e38-b2ed-dc2fe646cd7a, abstract = {{<p>We report on the formation of wrinkle-patterned surface morphologies in cesium formamidinium-based Cs<sub>x</sub>FA<sub>1-x</sub>Pb(I<sub>1-y</sub>Br<sub>y</sub>)<sub>3</sub> perovskite compositions with x = 0-0.3 and y = 0-0.3 under various spin-coating conditions. By varying the Cs and Br contents, the perovskite precursor solution concentration and the spin-coating procedure, the occurrence and characteristics of the wrinkle-shaped morphology can be tailored systematically. Cs<sub>0.17</sub>FA<sub>0.83</sub>Pb(I<sub>0.83</sub>Br<sub>0.17</sub>)<sub>3</sub> perovskite layers were analyzed regarding their surface roughness, microscopic structure, local and overall composition, and optoelectronic properties. Application of these films in p-i-n perovskite solar cells (PSCs) with indium-doped tin oxide/NiO<sub>x</sub>/perovskite/C<sub>60</sub>/bathocuproine/Cu architecture resulted in up to 15.3 and 17.0% power conversion efficiency for the flat and wrinkled morphology, respectively. Interestingly, we find slightly red-shifted photoluminescence (PL) peaks for wrinkled areas and we are able to directly correlate surface topography with PL peak mapping. This is attributed to differences in the local grain size, whereas there is no indication for compositional demixing in the films. We show that the perovskite composition, crystallization kinetics, and layer thickness strongly influence the formation of wrinkles which is proposed to be related to the release of compressive strain during perovskite crystallization. Our work helps us to better understand film formation and to further improve the efficiency of PSCs with widely used mixed-perovskite compositions.</p>}}, author = {{Braunger, Steffen and Mundt, Laura E. and Wolff, Christian M. and Mews, Mathias and Rehermann, Carolin and Jošt, Marko and Tejada, Alvaro and Eisenhauer, David and Becker, Christiane and Guerra, Jorge Andres and Unger, Eva and Korte, Lars and Neher, Dieter and Schubert, Martin C. and Rech, Bernd and Albrecht, Steve}}, issn = {{1932-7447}}, language = {{eng}}, month = {{08}}, number = {{30}}, pages = {{17123--17135}}, publisher = {{The American Chemical Society (ACS)}}, series = {{Journal of Physical Chemistry C}}, title = {{Cs <sub>x</sub> FA<sub>1- x</sub>Pb(I<sub>1- y</sub>Br <sub>y</sub>)<sub>3</sub> Perovskite Compositions : The Appearance of Wrinkled Morphology and its Impact on Solar Cell Performance}}, url = {{http://dx.doi.org/10.1021/acs.jpcc.8b06459}}, doi = {{10.1021/acs.jpcc.8b06459}}, volume = {{122}}, year = {{2018}}, }