Optical and Electronic Losses Arising from Physically Mixed Interfacial Layers in Perovskite Solar Cells.

external quantum efficiency modeling interfacial layers optical and electronic losses optical properties perovskite solar cells spectroscopic ellipsometry

Journal

ACS applied materials & interfaces
ISSN: 1944-8252
Titre abrégé: ACS Appl Mater Interfaces
Pays: United States
ID NLM: 101504991

Informations de publication

Date de publication:
03 Feb 2021
Historique:
pubmed: 21 1 2021
medline: 21 1 2021
entrez: 20 1 2021
Statut: ppublish

Résumé

Perovskite solar cell device performance is affected by optical and electronic losses. To minimize these losses in solar cells, it is important to identify their sources. Here, we report the optical and electronic losses arising from physically mixed interfacial layers between the adjacent component materials in highly efficient two terminal (2T) all-perovskite tandem, single-junction wide-bandgap, and single-junction narrow-bandgap perovskite-based solar cells. Physically mixed interfacial layers as the sources of optical and electronic losses are identified from spectroscopic ellipsometry measurements and data analysis followed by comparisons of simulated and measured external quantum efficiency spectra. Parasitic absorbance in the physically mixed regions between silver metal electrical contacts and electron transport layers (ETLs) near the back contact and a physical mixture of commercial indium tin oxide and hole transport layers (HTL) near the front electrical contact lead to substantial optical loss. A lower-density void + perovskite nucleation layer formed during perovskite deposition at the interface between the perovskite absorber layer and the HTL causes electronic losses because of incomplete collection of photogenerated carriers likely originating from poor coverage and passivation of the initially nucleating grains.

Identifiants

pubmed: 33470116
doi: 10.1021/acsami.0c16364
doi:

Types de publication

Journal Article

Langues

eng

Sous-ensembles de citation

IM

Pagination

4923-4934

Auteurs

Biwas Subedi (B)

Department of Physics and Astronomy and the Wright Center for Photovoltaics Innovation and Commercialization, University of Toledo, Toledo 43606, Ohio, United States.

Zhaoning Song (Z)

Department of Physics and Astronomy and the Wright Center for Photovoltaics Innovation and Commercialization, University of Toledo, Toledo 43606, Ohio, United States.

Cong Chen (C)

Department of Physics and Astronomy and the Wright Center for Photovoltaics Innovation and Commercialization, University of Toledo, Toledo 43606, Ohio, United States.

Chongwen Li (C)

Department of Physics and Astronomy and the Wright Center for Photovoltaics Innovation and Commercialization, University of Toledo, Toledo 43606, Ohio, United States.

Kiran Ghimire (K)

Department of Physics and Astronomy and the Wright Center for Photovoltaics Innovation and Commercialization, University of Toledo, Toledo 43606, Ohio, United States.

Maxwell M Junda (MM)

Department of Physics and Astronomy and the Wright Center for Photovoltaics Innovation and Commercialization, University of Toledo, Toledo 43606, Ohio, United States.

Indra Subedi (I)

Department of Physics and Astronomy and the Wright Center for Photovoltaics Innovation and Commercialization, University of Toledo, Toledo 43606, Ohio, United States.

Yanfa Yan (Y)

Department of Physics and Astronomy and the Wright Center for Photovoltaics Innovation and Commercialization, University of Toledo, Toledo 43606, Ohio, United States.

Nikolas J Podraza (NJ)

Department of Physics and Astronomy and the Wright Center for Photovoltaics Innovation and Commercialization, University of Toledo, Toledo 43606, Ohio, United States.

Classifications MeSH