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dc.contributor.authorRavishankar, Sandheep
dc.contributor.authorGarcía-Batlle, Marisé
dc.contributor.authorBisquert, Juan
dc.contributor.authorGarcia-Belmonte, Germà
dc.contributor.authorOdrobina, Jann
dc.contributor.authorSchiller, Carl-Albrecht
dc.date.accessioned2020-11-05T10:12:32Z
dc.date.available2020-11-05T10:12:32Z
dc.date.issued2020-06-29
dc.identifier.citationRAVISHANKAR, Sandheep, et al. Removing Instability-Caused Low-Frequency Features in Small Perturbation Spectra of Perovskite Solar Cells. The Journal of Physical Chemistry C, 2020, vol. 124, no 29, p. 15793-15799.ca_CA
dc.identifier.issn1932-7447
dc.identifier.urihttp://hdl.handle.net/10234/190221
dc.description.abstractSmall-perturbation frequency-domain techniques such as impedance spectroscopy and intensity-modulated photocurrent spectroscopy (IMPS) have become important methods for the investigation of the physical working mechanisms of the perovskite solar cell (PSC). The validity of these methods relies on assuming sample stability at the given steady state. Through a series of IMPS measurements, we identify that this assumption is invalid in certain cases for both iodide and bromide-based PSCs that show strong time drift in their IMPS response, noticeable in particular at low frequencies, which are usually connected with the kinetics of ionic motion and interaction with outer electrodes. Using time course interpolation and a corrective Z-HIT algorithm that connects the modulus of the IMPS transfer function and its phase, we identify that the low-frequency arc/tail is in certain cases an artifact generated by time drift of the sample. Since the low-frequency data in an IMPS measurement of the PSC provide important information regarding its differential external quantum efficiency, care must be taken to ascertain the origin and validity of the low-frequency phenomena. Validity test is performed by using a combination of corrective algorithms mentioned above and several measurements over time to obtain stabilized spectra virtually free of time drift.ca_CA
dc.format.extent17 p.ca_CA
dc.format.mimetypeapplication/pdfca_CA
dc.language.isoengca_CA
dc.publisherAmerican Chemical Societyca_CA
dc.relation.isPartOfJ. Phys. Chem. C 2020, 124, 29, 15793–15799ca_CA
dc.rights© 2020 American Chemical Societyca_CA
dc.rights.urihttp://rightsstatements.org/vocab/InC/1.0/*
dc.subjectoxidesca_CA
dc.subjectexternal quantum efficiencyca_CA
dc.subjectelectrical propertiesca_CA
dc.subjectsolar cellsca_CA
dc.subjectelectron correlationca_CA
dc.titleRemoving Instability-Caused Low-Frequency Features in Small Perturbation Spectra of Perovskite Solar Cellsca_CA
dc.typeinfo:eu-repo/semantics/articleca_CA
dc.identifier.doihttps://doi.org/10.1021/acs.jpcc.0c04050
dc.relation.projectIDS.R. acknowledges funding from the Helmholtz association via the PEROSEED project. M. G.-B. acknowledges Generalitat Valenciana for Grant GRISOLIAP/2018/073.ca_CA
dc.rights.accessRightsinfo:eu-repo/semantics/openAccessca_CA
dc.relation.publisherVersionhttps://pubs.acs.org/doi/10.1021/acs.jpcc.0c04050ca_CA
dc.date.embargoEndDate2021-06-30
dc.type.versioninfo:eu-repo/semantics/acceptedVersionca_CA


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