Abstract
Rapid Spray Plasma Processing (RSPP) is a high throughput, scalable, and open-air route toward manufacturing perovskite solar modules. The plasma exposure is dosed such that the perovskite precursor solution is cured in milliseconds using a combination of rapid heating, reactive species, and UV photons. We implemented in situ wide angle X-ray scattering (WAXS) to characterize the crystal growth in multiple cation, mixed halide perovskite thin films - Csx(MAzFA1-z)1-xPb(Br0.17I0.83)3 for 0.05 ≤ x ≤ 0.25 - fabricated in open air. The use of synchrotron radiation and high detector speeds resolved the formation and dissolution of a transient intermediate crystalline phase during the tens of milliseconds when the perovskite crystallized. Increasing the mole fraction of cesium and methylammonium resulted in a decrease in the intermediate phase and an increase in the average grain diameter. Increasing the cesium fraction suppressed phase segregation, as observed in photoluminescence. Calculations showed the refractive index decreased and the extinction coefficient increased with cesium fraction. Based on the rapid crystallization kinetics, RSPP perovskite films exhibit residual stress values >5× lower than spin coated films. Understanding the kinetics of perovskite formation enables the design of perovskite films with improved thermomechanical and operational stability.
Original language | English |
---|---|
Pages (from-to) | 169-176 |
Number of pages | 8 |
Journal | Journal of Materials Chemistry A |
Volume | 8 |
Issue number | 1 |
DOIs | |
State | Published - Jan 7 2020 |
Bibliographical note
Publisher Copyright:© 2019 The Royal Society of Chemistry.
Funding
This material is based upon work supported by the U.S. Department of Energy's Office of Energy Efficiency and Renewable Energy (EERE) under Solar Energy Technologies Office (SETO) Agreement Number DE-EE0008559. Part of this work was performed at the Stanford Nano Shared Facilities (SNSF), supported by the National Science Foundation under award ECCS-1542152. Additional support was provided by the National Science Foundation Graduate Research Fellowship, awarded to N. Rolston under award DGE-1656518. Use of the Stanford Synchrotron Radiation Lightsource SLAC National Accelerator Laboratory, is supported by the U.S. Department of Energy, Office of Science, Office of Basic Energy Sciences under Contract No. DE-AC02-76SF00515. We also thank Ron Marks for helpful discussions and experimental assistance at Beamline 10-2 at SSRL.
Funders | Funder number |
---|---|
National Science Foundation Integrated Graduate Education and Research Training | DGE-1656518 |
Office of Basic Energy Sciences | |
Stanford Nano Shared Facilities | |
National Science Foundation Arctic Social Science Program | ECCS-1542152 |
Office of Science Programs | |
Office of Energy Efficiency and Renewable Energy | |
Solar Energy Technologies Office | DE-EE0008559 |
ASJC Scopus subject areas
- General Chemistry
- Renewable Energy, Sustainability and the Environment
- General Materials Science