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Main Authors: Hußner, Markus, Richard, Pacalaj A., Müller-Dieckert, Olaf G., Liu, Chao, Zhou, Zhisheng, Majeed, Nahdia, Greedy, Steve, Ramirez, Ivan, Li, Ning, Hosseini, Seyed Mehrdad, Uhrich, Christian, Brabec, Christoph J., Durrant, James R., Deibel, Carsten, MacKenzie, Roderick C. I.
Format: Preprint
Published: 2023
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Online Access:https://arxiv.org/abs/2309.03644
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author Hußner, Markus
Richard, Pacalaj A.
Müller-Dieckert, Olaf G.
Liu, Chao
Zhou, Zhisheng
Majeed, Nahdia
Greedy, Steve
Ramirez, Ivan
Li, Ning
Hosseini, Seyed Mehrdad
Uhrich, Christian
Brabec, Christoph J.
Durrant, James R.
Deibel, Carsten
MacKenzie, Roderick C. I.
author_facet Hußner, Markus
Richard, Pacalaj A.
Müller-Dieckert, Olaf G.
Liu, Chao
Zhou, Zhisheng
Majeed, Nahdia
Greedy, Steve
Ramirez, Ivan
Li, Ning
Hosseini, Seyed Mehrdad
Uhrich, Christian
Brabec, Christoph J.
Durrant, James R.
Deibel, Carsten
MacKenzie, Roderick C. I.
contents Over the last two decades the organic solar cell community has synthesised tens of thousands of novel polymers and small molecules in the search for an optimum light harvesting material. These materials were often crudely evaluated simply by measuring the current voltage curves in the light to obtain power conversion efficiencies (PCEs). Materials with low PCEs were quickly disregarded in the search for higher efficiencies. More complex measurements such as frequency/time domain characterisation that could explain why the material performed as it did were often not performed as they were too time consuming/complex. This limited feedback forced the field to advance using a more or less random walk of material development and has significantly slowed progress. Herein, we present a simple technique based on machine learning that can quickly and accurately extract recombination time constants and charge carrier mobilities as a function of light intensity simply from light/dark JV curves alone. This technique reduces the time to fully analyse a working cell from weeks to seconds and opens up the possibility of not only fully characterising new devices as they are fabricated, but also data mining historical data sets for promising materials the community has over looked.
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institution arXiv
publishDate 2023
record_format arxiv
spellingShingle Machine learning for ultra high throughput screening of organic solar cells: Solving the needle in the hay stack problem
Hußner, Markus
Richard, Pacalaj A.
Müller-Dieckert, Olaf G.
Liu, Chao
Zhou, Zhisheng
Majeed, Nahdia
Greedy, Steve
Ramirez, Ivan
Li, Ning
Hosseini, Seyed Mehrdad
Uhrich, Christian
Brabec, Christoph J.
Durrant, James R.
Deibel, Carsten
MacKenzie, Roderick C. I.
Applied Physics
Over the last two decades the organic solar cell community has synthesised tens of thousands of novel polymers and small molecules in the search for an optimum light harvesting material. These materials were often crudely evaluated simply by measuring the current voltage curves in the light to obtain power conversion efficiencies (PCEs). Materials with low PCEs were quickly disregarded in the search for higher efficiencies. More complex measurements such as frequency/time domain characterisation that could explain why the material performed as it did were often not performed as they were too time consuming/complex. This limited feedback forced the field to advance using a more or less random walk of material development and has significantly slowed progress. Herein, we present a simple technique based on machine learning that can quickly and accurately extract recombination time constants and charge carrier mobilities as a function of light intensity simply from light/dark JV curves alone. This technique reduces the time to fully analyse a working cell from weeks to seconds and opens up the possibility of not only fully characterising new devices as they are fabricated, but also data mining historical data sets for promising materials the community has over looked.
title Machine learning for ultra high throughput screening of organic solar cells: Solving the needle in the hay stack problem
topic Applied Physics
url https://arxiv.org/abs/2309.03644