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dc.contributor.authorFakharuddin, Azhar
dc.contributor.authorSeybold, Michael
dc.contributor.authorAgresti, Antonio
dc.contributor.authorPescetelli, Sara
dc.contributor.authormatteocci, fabio
dc.contributor.authorHaider, Muhammad Irfan
dc.contributor.authorBirkhold, Susanne T.
dc.contributor.authorHu, Hao
dc.contributor.authorGiridharagopal, Rajiv
dc.contributor.authorSultan, Muhammad
dc.contributor.authorMora-Sero, Ivan
dc.contributor.authorDi Carlo, Aldo
dc.contributor.authorSchmidt-Mende, Lukas
dc.date.accessioned2018-12-05T08:43:20Z
dc.date.available2018-12-05T08:43:20Z
dc.date.issued2018
dc.identifier.citationFAKHARUDDIN, Azhar, et al. Perovskite-polymer blends influencing microstructure, non-radiative recombination pathways and photovoltaic performance of perovskite solar cells. ACS applied materials & interfaces, 2018, 10, 49, 42542–42551ca_CA
dc.identifier.issn1944-8244
dc.identifier.issn1944-8252
dc.identifier.urihttp://hdl.handle.net/10234/177890
dc.description.abstractSolar cells based on organic–inorganic halide perovskites are now leading the photovoltaic technologies because of their high power conversion efficiency. Recently, there have been debates on the microstructure-related defects in metal halide perovskites (grain size, grain boundaries, etc.) and a widespread view is that large grains are a prerequisite to suppress nonradiative recombination and improve photovoltaic performance, although opinions against it also exist. Herein, we employ blends of methylammonium lead iodide perovskites with an insulating polymer (polyvinylpyrrolidone) that offer the possibility to tune the grain size in order to obtain a fundamental understanding of the photoresponse at the microscopic level. We provide, for the first time, spatially resolved details of the microstructures in such blend systems via Raman mapping, light beam-induced current imaging, and conductive atomic force microscopy. Although the polymer blend systems systematically alter the morphology by creating small grains (more grain boundaries), they reduce nonradiative recombination within the film and enhance its spatial homogeneity of radiative recombination. We attribute this to a reduction in the density of bulk trap states, as evidenced by an order of magnitude higher photoluminescence intensity and a significantly higher open-circuit voltage when the polymer is incorporated into the perovskite films. The solar cells employing blend systems also show nearly hysteresis-free power conversion efficiency ∼17.5%, as well as a remarkable shelf-life stability over 100 days.ca_CA
dc.format.extent10 p.ca_CA
dc.language.isoengca_CA
dc.publisherAmerican Chemical Societyca_CA
dc.relation.isPartOfACS Applied Materials and Interfaces, 2018, 10, 49, 42542–42551ca_CA
dc.rightsCopyright © American Chemical Societyca_CA
dc.rights.urihttp://rightsstatements.org/vocab/InC/1.0/*
dc.subjectdefects in perovskitesca_CA
dc.subjectgrain boundaries and defectsca_CA
dc.subjectnon-radiative recombinationca_CA
dc.subjectpolymer scaffolds for perovskitesca_CA
dc.subjectspatially resolved characterizations of perovskitesca_CA
dc.titlePerovskite-Polymer Blends Influencing Microstructures, Nonradiative Recombination Pathways, and Photovoltaic Performance of Perovskite Solar Cellsca_CA
dc.typeinfo:eu-repo/semantics/articleca_CA
dc.identifier.doihttps://doi.org/10.1021/acsami.8b18200
dc.relation.projectIDAlexander von Humboldt; the ERANET project Hydrosol; Deutsche Forschungsgemeinschaft DFG for funding within the framework of the Collaborative Research Center SFB-1214 - project Z1 (Particle Analysis Center); Carl Zeiss Foundation; DOE (DE-SC0013957) ;European Research Council (ERC) via a Consolidator Grant (724424-No- LIMIT).
dc.rights.accessRightsinfo:eu-repo/semantics/openAccessca_CA
dc.relation.publisherVersionhttps://pubs.acs.org/doi/full/10.1021/acsami.8b18200ca_CA
dc.contributor.funderA.F. acknowledges financial support from Alexander von Humboldt and A.F. and L.S.M. from the ERANET project Hydrosol. The authors thank the Deutsche Forschungsgemeinschaft DFG for funding within the framework of the Collaborative Research Center SFB-1214 - project Z1 (Particle Analysis Center). S.T.B. acknowledges financial support from the Carl Zeiss Foundation. We thank David S. Ginger (University of Washington) for the use of AFM facilities for cAFM measurements. R.G. acknowledges support from DOE (DE-SC0013957). IMS acknowledges European Research Council (ERC) via a Consolidator Grant (724424-NoLIMIT).
dc.type.versioninfo:eu-repo/semantics/acceptedVersionca_CA


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