A Terpolymer Acceptor Enabling All-Polymer Solar Cells with a Broad Donor:Acceptor Composition Tolerance and Enhanced Stability

Bin Liu, Junwei Wang, Huiliang Sun*, Ziang Wu, Chao Yao, Qiaogan Liao, Zixiang Wei, Wanli Yang, Xianhe Zhang, Hong Meng, Han Young Woo*, Xugang Guo*

*Corresponding author for this work

    Research output: Contribution to journalArticlepeer-review

    9 Citations (Scopus)

    Abstract

    Achieving a broad donor:acceptor (D:A) composition tolerance in efficient organic solar cells (OSCs) is important for printing large-area solar cell modules. Herein, all-polymer solar cells (all-PSCs) based on new terpolymer acceptors and a well-known polymer donor PTB7-Th are fabricated to explore the effect of D:A ratio on morphology and photovoltaic performances. The all-PSCs show a promising power conversion efficiency (PCE) of 7.23% with an optimum D:A ratio of 1:2 and retain over 40% of its optimal PCE with ultrabroad D:A composition tolerance from 1:30 to 10:1. In addition, the all-PSCs can maintain 90% of its original PCE after 400 h of storage despite such broad range of D:A ratio, which is much better than those of other types of OSCs and even better than the benchmark all-polymer system with N2200 as the acceptor under the same condition. The results show the superiority of the all-PSCs in terms of D:A ratio tolerance and performance stability, which should be conducive to practical applications of all-PSCs.

    Original languageEnglish
    Article number2000436
    JournalSolar RRL
    Volume4
    Issue number11
    DOIs
    Publication statusPublished - 2020 Nov

    Bibliographical note

    Publisher Copyright:
    © 2020 Wiley-VCH GmbH.

    Keywords

    • all-polymer solar cells
    • film morphology
    • high donor:acceptor ratio tolerance
    • n-type terpolymers

    ASJC Scopus subject areas

    • Electronic, Optical and Magnetic Materials
    • Atomic and Molecular Physics, and Optics
    • Energy Engineering and Power Technology
    • Electrical and Electronic Engineering

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