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Phenyltrimethylammonium as an Interlayer Spacer for Stable Formamidinium-Based Quasi-2D Perovskite Solar Cells
Quasi-2D perovskite materials possess great potential in improving the stability of perovskite solar cells due to their superior chemical and structural stableness compared to 3D counterparts. Here, commonly-used 3D formamidinum lead iodide (FAPbI 3 ) perovskite is alloyed by addition of quaternary...
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Published in: | Electronic materials letters 2024, 20(6), , pp.791-798 |
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Main Authors: | , , |
Format: | Article |
Language: | English |
Subjects: | |
Citations: | Items that this one cites |
Online Access: | Get full text |
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Summary: | Quasi-2D perovskite materials possess great potential in improving the stability of perovskite solar cells due to their superior chemical and structural stableness compared to 3D counterparts. Here, commonly-used 3D formamidinum lead iodide (FAPbI
3
) perovskite is alloyed by addition of quaternary cation phenyltrimethylammonium (PTMA) up to 33% (
n
= 5), which forms quasi-2D perovskite phase that acts beneficial to charge transport and stability. Since the detailed structural analyses regarding this quaternary ammonium salt is still lacking, we attempt to provide how the presence of 2D perovskite affects the crystal structure based on x-ray diffraction techniques. It is shown that PTMA cations directs FAPbI
3
to have textured orientation and reduced strains. This led to enhanced extraction of photogenerated carriers and reduced defects, making it promising material for solar cell applications. The champion device remains stable under 60 °C or 1 sun for 700 h, demonstrating its potential for optoelectronic devices requiring long-term stability.
Graphical Abstract
Highlights
•
PTMA can be successfully alloyed in FAPbI
3
up to ~ 33%.
•
PTMA-alloyed FAPbI
3
demonstrates reduced strains and more textured perovskite layer.
•
Addition of PTMA results in improved PL yield and reduced trap density.
•
Solar cells with PTMA-alloyed FAPbI
3
shows excellent stability under heat or light. |
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ISSN: | 1738-8090 2093-6788 |
DOI: | 10.1007/s13391-024-00497-w |