<HashMap><database>biostudies-literature</database><scores/><additional><submitter>Hadke SS</submitter><funding>Ministry of Education - Singapore (MOE)</funding><pagination>8240</pagination><full_dataset_link>https://www.ebi.ac.uk/biostudies/studies/S-EPMC12417543</full_dataset_link><repository>biostudies-literature</repository><omics_type>Unknown</omics_type><volume>16(1)</volume><pubmed_abstract>The photovoltaic performance of Cu&lt;sub>2&lt;/sub>ZnSn(S,Se)&lt;sub>4&lt;/sub> is limited by open-circuit voltage losses (ΔV&lt;sub>OC&lt;/sub>) in the radiative (ΔV&lt;sub>OC&lt;/sub>&lt;sup>Rad&lt;/sup>) and non-radiative (ΔV&lt;sub>OC&lt;/sub>&lt;sup>Nrad&lt;/sup>) limits, due to sub-bandgap absorption and deep defects, respectively. Recently, several devices with power conversion efficiencies approaching 15% have been reported, prompting renewed interest in the possibility that the key performance-limiting factors have been addressed. In this work, we analyze the sources of ΔV&lt;sub>OC&lt;/sub> in these devices and offer directions for future research. We find that ΔV&lt;sub>OC&lt;/sub>&lt;sup>Rad&lt;/sup>, arising from bandgap fluctuations and Urbach tails, has been significantly suppressed, with values comparable to those of commercial Cu(In,Ga)(S,Se)&lt;sub>2&lt;/sub> solar cells. However, the recombination parameter J&lt;sub>0&lt;/sub>, which is more directly related to ΔV&lt;sub>OC&lt;/sub>&lt;sup>Nrad&lt;/sup>, shows only modest improvement and must be reduced by four to six orders of magnitude to compete with Cu(In,Ga)(S,Se)&lt;sub>2&lt;/sub>. To approach the theoretical efficiency limit, future work should focus on more directly addressing deep defects and ΔV&lt;sub>OC&lt;/sub>&lt;sup>Nrad&lt;/sup>.</pubmed_abstract><journal>Nature communications</journal><pubmed_title>Understanding efficiency losses from radiative and nonradiative recombination in Cu&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;ZnSn(S,Se)&amp;lt;sub&amp;gt;4&amp;lt;/sub&amp;gt; solar cells.</pubmed_title><pmcid>PMC12417543</pmcid><funding_grant_id>RG155/23</funding_grant_id><pubmed_authors>Liang G</pubmed_authors><pubmed_authors>Shao Z</pubmed_authors><pubmed_authors>Meng Q</pubmed_authors><pubmed_authors>Wu S</pubmed_authors><pubmed_authors>Su Z</pubmed_authors><pubmed_authors>Hadke SS</pubmed_authors><pubmed_authors>Xin H</pubmed_authors><pubmed_authors>Wong LH</pubmed_authors></additional><is_claimable>false</is_claimable><name>Understanding efficiency losses from radiative and nonradiative recombination in Cu&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;ZnSn(S,Se)&amp;lt;sub&amp;gt;4&amp;lt;/sub&amp;gt; solar cells.</name><description>The photovoltaic performance of Cu&lt;sub>2&lt;/sub>ZnSn(S,Se)&lt;sub>4&lt;/sub> is limited by open-circuit voltage losses (ΔV&lt;sub>OC&lt;/sub>) in the radiative (ΔV&lt;sub>OC&lt;/sub>&lt;sup>Rad&lt;/sup>) and non-radiative (ΔV&lt;sub>OC&lt;/sub>&lt;sup>Nrad&lt;/sup>) limits, due to sub-bandgap absorption and deep defects, respectively. Recently, several devices with power conversion efficiencies approaching 15% have been reported, prompting renewed interest in the possibility that the key performance-limiting factors have been addressed. In this work, we analyze the sources of ΔV&lt;sub>OC&lt;/sub> in these devices and offer directions for future research. We find that ΔV&lt;sub>OC&lt;/sub>&lt;sup>Rad&lt;/sup>, arising from bandgap fluctuations and Urbach tails, has been significantly suppressed, with values comparable to those of commercial Cu(In,Ga)(S,Se)&lt;sub>2&lt;/sub> solar cells. However, the recombination parameter J&lt;sub>0&lt;/sub>, which is more directly related to ΔV&lt;sub>OC&lt;/sub>&lt;sup>Nrad&lt;/sup>, shows only modest improvement and must be reduced by four to six orders of magnitude to compete with Cu(In,Ga)(S,Se)&lt;sub>2&lt;/sub>. To approach the theoretical efficiency limit, future work should focus on more directly addressing deep defects and ΔV&lt;sub>OC&lt;/sub>&lt;sup>Nrad&lt;/sup>.</description><dates><release>2025-01-01T00:00:00Z</release><publication>2025 Sep</publication><modification>2026-05-27T08:03:04.43Z</modification><creation>2026-05-24T03:06:55.347Z</creation></dates><accession>S-EPMC12417543</accession><cross_references><pubmed>40921765</pubmed><doi>10.1038/s41467-025-63345-x</doi></cross_references></HashMap>