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   	<dc:title>In silico investigation of Cu(In,Ga)Se2-based solar cells</dc:title>
   	<dc:creator>Mirhosseini, S. Hossein</dc:creator>
   	<dc:creator>Kormath Madam Raghupathy, Ramya</dc:creator>
   	<dc:creator>Sahoo, Sudhir K.</dc:creator>
   	<dc:creator>Wiebeler, Hendrik</dc:creator>
   	<dc:creator>Chugh, Manjusha</dc:creator>
   	<dc:creator>Kühne, Thomas</dc:creator>
   	<dc:description>Photovoltaics is one of the most promising and fastest-growing renewable energy technologies. Although the price-performance ratio of solar cells has improved significantly over recent years{,} further systematic investigations are needed to achieve higher performance and lower cost for future solar cells. In conjunction with experiments{,} computer simulations are powerful tools to investigate the thermodynamics and kinetics of solar cells. Over the last few years{,} we have developed and employed advanced computational techniques to gain a better understanding of solar cells based on copper indium gallium selenide (Cu(In{,}Ga)Se2). Furthermore{,} we have utilized state-of-the-art data-driven science and machine learning for the development of photovoltaic materials. In this Perspective{,} we review our results along with a survey of the field.</dc:description>
   	<dc:publisher>The Royal Society of Chemistry</dc:publisher>
   	<dc:date>2020</dc:date>
   	<dc:type>info:eu-repo/semantics/article</dc:type>
   	<dc:type>doc-type:article</dc:type>
   	<dc:type>text</dc:type>
   	<dc:type>http://purl.org/coar/resource_type/c_6501</dc:type>
   	<dc:identifier>https://ris.uni-paderborn.de/record/21112</dc:identifier>
   	<dc:source>Mirhosseini SH, Kormath Madam Raghupathy R, Sahoo SK, Wiebeler H, Chugh M, Kühne T. In silico investigation of Cu(In,Ga)Se2-based solar cells. &lt;i&gt;Phys Chem Chem Phys&lt;/i&gt;. 2020;22:26682-26701. doi:&lt;a href=&quot;https://doi.org/10.1039/D0CP04712K&quot;&gt;10.1039/D0CP04712K&lt;/a&gt;</dc:source>
   	<dc:language>eng</dc:language>
   	<dc:relation>info:eu-repo/semantics/altIdentifier/doi/10.1039/D0CP04712K</dc:relation>
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