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Pyrene-Based Small-Molecular Hole Transport Layers for Efficient and Stable Narrow-Bandgap Perovskite Solar Cells

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Samenvatting

Lead–tin (Pb–Sn) hybrid perovskite materials possess ideal narrow bandgaps (1.2–1.4 eV) for efficient single-junction and tandem solar cells. Poly(3,4-ethylenedioxythiophene):polystyrene sulfonate (PEDOT:PSS) is commonly used as hole transport layer (HTL) for Pb–Sn perovskite solar cells (PSCs), despite its poor stability with these perovskites. Here, two new octacyclic heteroaromatic molecules, pyrenodiindole (PDI) and pyrenodi-(7-azaindole) (PDAI), are presented as the HTL for narrow-bandgap (1.23 eV) p–i–n Pb-Sn PSCs. The self-assembled reciprocal hydrogen-bonded solid-state structure of PDAI bestows robustness compared to PDI, making it less vulnerable in processing the perovskite film on top, and improves the reproducibility of device fabrication. Transient photocurrent measurements and light-intensity-dependent device characteristics indicate that PDI and PDAI possess similar hole extraction properties to PEDOT:PSS. As a result, similar open-circuit voltages and fill factors are obtained in the PSCs. Interestingly, the use of thin PDI and PDAI as HTL in PSCs changes the optical interference and reduces parasitic absorption in the near-infrared region, resulting in an improved short-circuit current density. Consequently, a higher power conversion efficiency of 16.1% is obtained for PDI and PDAI, compared to 15.1% for PEDOT:PSS. In addition, the self-assembled structure of PDAI led to a notable enhancement of device stability.

Originele taal-2Engels
Artikelnummer2100454
Aantal pagina's11
TijdschriftSolar RRL
Volume5
Nummer van het tijdschrift10
DOI's
StatusGepubliceerd - okt. 2021

Bibliografische nota

Publisher Copyright:
© 2021 The Authors. Solar RRL published by Wiley-VCH GmbH

Financiering

P.G. and J.W. contributed equally to this work. The authors thank Dr. Junyu Li for GIWAX measurements, Kunal Datta for XRD measurements, Bas van Gorkom for sub‐bandgap EQE experiments, Tom van der Pol for optical simulations, Riccardo Ollearo for transient photocurrent measurements, and Antonio García for DFT calculations. The authors acknowledge the financial support from the Ministry of Science, Innovation and Universities (Project RTI2018‐101092‐B‐I00) and Programa Estatal de Fomento de la Investigación Científica y Técnica de Excelencia (RED2018‐102815‐T). The authors are also grateful to Fundación Séneca–Agencia de Ciencia y Tecnología de la Región de Murcia for funding the Project 20959/PI/18 and M.M.‐M.'s postdoctoral contract from the “Saavedra Fajardo Program” (20406/SF/17). Further funding was received from the Netherlands Organization for Scientific Research via the NWO Spinoza grant and from the Ministry of Education, Culture and Science (Gravity program 024.001.035).

FinanciersFinanciernummer
Ministerio de Ciencia e InnovaciónRTI2018‐101092‐B‐I00
Ministerie van OCW024.001.035
Nederlandse Organisatie voor Wetenschappelijk Onderzoek

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