Material properties for longer-lasting, more efficient solar cells — ScienceDaily

Material properties for longer-lasting, more efficient solar cells — ScienceDaily

The designers of solar cells know their creations must contend with a wide range of temperatures and all sorts of weather conditions — conditions that can impact their efficiency and useful lifetime.

Florida State University Assistant Professor of Chemistry and Biochemistry Lea Nienhaus and former FSU postdoctoral researcher Sarah Wieghold are helping to understand the fundamental processes in a material known as perovskites, work that could lead to more efficient solar cells that also do a better job of resisting degradation. They found that small tweaks to the chemical makeup of the materials as well as the magnitude of the electrical field it is exposed to can greatly affect the overall material stability.

Their latest work is published in a pair of studies in Journal of Materials Chemistry C and Journal of Applied Physics.

Their research is focused on improving the potential of perovskites, a material with a crystal structure based on positively charged lead ions known as cations and negatively charged halide anions. In a cubic perovskite crystal structure, the octahedra formed by the lead and halide ions are surrounded by additional positively charged cations.

The first perovskite solar cells, which were developed in 2006, had a solar energy power conversion efficiency of about 3 percent, but cells developed in 2020 have a power conversion efficiency of more than 25 percent. That rapid increase in efficiency makes them a promising material for further research, but they have drawbacks for commercial viability, such as a tendency to degrade quickly.

“How can we make perovskites more stable under real-world conditions in which they’ll be used?” Nienhaus said. “What is causing the degradation? That’s what we’re trying to understand. Perovskites that don’t degrade quickly could be a valuable tool for obtaining more energy from solar cells.”

Perovskites are a so-called “soft material,” despite the ionic bonds of the crystal lattice that make up their structure. The halides or cations in the material can move through that lattice, which may increase their rate of degradation, resulting in a lack of long-term stability.

In the Journal of Materials Chemistry C paper, the researchers investigated the combined influence of light and elevated temperature on the performance of mixed-cation mixed-halide perovskites.

They found that adding a small amount of the element cesium to the perovskite film increases the stability of the material under light and elevated temperatures. Adding rubidium, on the other hand, led to worse performance.

“We found that depending on the choice of the cation, two pathways of degradation can be observed in these materials, which we then correlated to a decrease in performance,” said Wieghold, now an assistant scientist at the Center for Nanoscale Materials and the Advanced Photon Source at Argonne National Laboratory. “We also showed that the addition of cesium increased the film stability under our testing conditions, which are very promising results.”

They also found that a decrease in film performance for the less stable perovskite mixtures was correlated with the formation of the compound lead bromide/iodide and an increase in electron-phonon interactions. The formation of lead bromide/iodide is due to the unwanted degradation mechanism, which needs to be avoided to achieve long-term stability and performance of these perovskite solar cells.

In the Journal of Applied Physics paper, they explored the link between voltage and the performance of perovskite materials. This showed that the ion movement in the material changes the underlying electrical response, which will be a critical factor in the photovoltaic performance.

“Perovskites present a great opportunity for the future of solar cells, and it’s exciting to help move this science forward,” Nienhaus said.

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Materials provided by Florida State University. Original written by Bill Wellock. Note: Content may be edited for style and length.

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