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Effect of thiourea/metal ratio on the properties of MOE based Cu2ZnSn(S,Se)4 thin films and solar cells

By optimizing the thiourea-to-metal ratio in the precursor solution to tailor film porosity, this study enhances the vertical crystallization uniformity and defect properties of MOE-based CZTSSe absorbers, thereby boosting solar cell efficiency from 8.1% to 12.1%.

Original authors: Yingxuan Cui, Yajie Shen, Yang Liu, Yanxin Huo, Cong Song, Wei Yu, Chao Gao

Published 2026-07-20
📖 6 min read🧠 Deep dive

Original authors: Yingxuan Cui, Yajie Shen, Yang Liu, Yanxin Huo, Cong Song, Wei Yu, Chao Gao

Original paper licensed under CC BY 4.0 (https://creativecommons.org/licenses/by/4.0/). This is an AI-generated explanation of the paper below. It is not written or endorsed by the authors. For technical accuracy, refer to the original paper. Read full disclaimer

Imagine the world of solar energy as a bustling city where sunlight is the currency. For decades, we've been trying to build better "banks" to catch and store this currency, but the materials we use are often too expensive or made from rare elements that are running out. Enter a new contender for the job: a material called CZTSSe. Think of it as a super-efficient, eco-friendly sponge made from common elements like copper, zinc, tin, sulfur, and selenium. It's cheap to make and abundant in the earth, making it a perfect candidate to power our future. However, making a perfect sponge is tricky. If the sponge is too dense, the "currency" (sunlight) can't get deep inside to be collected. If it's too full of holes, the structure falls apart. The secret to a great solar cell lies in the "precursor"—the liquid soup you use to build the sponge before it hardens. Scientists have long known that the recipe matters, but the exact balance of ingredients to create the perfect internal structure has been a bit of a mystery.

In this study, researchers at Hebei University decided to play with the recipe of this liquid soup, specifically focusing on how much of a chemical called thiourea they added compared to the metal ingredients. They used a solvent called 2-methoxyethanol (MOE), which is like a gentle, low-toxicity glue that helps everything mix well. Their goal was to see if changing the amount of thiourea could change the "porosity" (the number of tiny holes) in the film before it was baked. They found that by carefully adjusting this ratio, they could turn a dense, sluggish film into a loose, porous one that acted like a high-speed highway for the next step of the process: selenization. This is where selenium gas is introduced to turn the solid film into the final solar material. The results were striking: by finding the "Goldilocks" ratio, they didn't just make a better film; they boosted the solar cell's efficiency from a modest 8.1% to a much more impressive 12.1%, all without needing extra fancy coatings or doping tricks.

The Recipe for a Better Solar Sponge

The story begins with the "precursor," which is essentially the liquid mixture scientists spin onto a glass slide to create the thin film that will eventually become the solar cell. The researchers prepared four different batches of this liquid, each with a slightly different ratio of thiourea to metal. They called these batches S-1.6, S-1.8, S-2.0, and S-2.2, based on the specific ratio numbers. When they looked at these films under a microscope before baking them, they saw something fascinating. The films with lower amounts of thiourea (like S-1.6) were dense and compact, almost like a tightly packed brick wall. But as they added more thiourea, the films became looser and more porous, resembling a sponge with tiny, interconnected tunnels.

Why does this matter? Think of the selenization process (where the film is heated with selenium gas) as a race. The selenium gas needs to rush into the film to react with the metals and form the final crystal structure. If the film is a dense brick wall, the gas has to struggle to get through, leading to a slow, uneven reaction. But if the film is a porous sponge, the gas can zoom right into the center, ensuring the whole film transforms evenly and quickly. The researchers discovered that the S-2.0 batch, with its perfectly tuned porosity, created the ideal "highway" for the selenium gas.

The Transformation: From Soup to Crystal

Once the films were baked, the magic happened. The team watched the transformation using X-ray machines and microscopes to see how the crystals grew. The S-2.0 sample, which had the optimal porosity, turned into a beautiful, large-grained structure with very few gaps or cracks. It was like watching a messy pile of sand suddenly organize itself into a giant, smooth crystal. In contrast, the S-1.6 sample (the dense one) struggled to grow large crystals and ended up with many tiny, disconnected grains and voids.

The researchers also noticed a cool side effect of the porous structure. During the early stages of baking, a temporary phase called Cu2-xSe formed. Think of this as a "construction crew" that arrives early to help build the final structure. In the S-2.0 sample, this crew arrived faster and worked more efficiently because the porous film let them in easily. This early help resulted in a much higher quality crystal structure by the time the baking was finished.

The Electrical Payoff

A better crystal structure means a better solar cell, and the numbers prove it. The team built solar cells using these different films and tested how well they worked. The S-2.0 device was the clear winner. It managed to convert 12.1% of the sunlight hitting it into electricity, a significant jump from the 8.1% achieved by the S-1.6 device.

Why was S-2.0 so much better? The porous structure led to a film with fewer "defects." In the world of solar cells, defects are like potholes on a road that cause electrons (the electricity carriers) to crash and lose energy. The S-2.0 film had fewer potholes, meaning the electrons could flow smoothly. This reduced the amount of energy lost as heat and allowed the cell to generate a higher voltage. Furthermore, the improved structure lowered the resistance at the back of the cell, making it easier for the electricity to exit the device and power your gadgets.

The researchers also looked at the "barrier" at the back of the cell. In the S-1.6 sample, this barrier was high (80.1 meV), acting like a steep hill that electrons had to climb. In the S-2.0 sample, the barrier dropped to 60.3 meV, making it a gentle slope that electrons could glide down effortlessly. This improvement, combined with a reduction in internal recombination (where electrons and holes cancel each other out before doing any work), was the key to the efficiency boost.

The Takeaway

This study shows that sometimes, the secret to a high-tech breakthrough isn't adding more complex ingredients, but simply adjusting the balance of what you already have. By tweaking the thiourea-to-metal ratio to create a porous precursor film, the researchers allowed the selenium gas to penetrate deeper and faster, leading to a superior crystal structure. This simple adjustment improved the quality of the solar cell, reduced energy losses, and pushed the efficiency up to 12.1%. While this isn't the highest efficiency ever recorded for this type of solar cell, it demonstrates a powerful and straightforward strategy: if you want to build a better solar sponge, make sure it has the right amount of holes to let the magic happen.

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