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Influences of Quinoid Structures on Stability and Photovoltaic Performance of Nonfullerene Acceptors
Author(s) -
Lv Ruizhi,
Geng Shizhe,
Li Shuixing,
Wu Fei,
Li Yaokai,
Andersen Thomas Rieks,
Li Yuhao,
Lu Xinhui,
Shi Minmin,
Chen Hongzheng
Publication year - 2020
Publication title -
solar rrl
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.544
H-Index - 37
ISSN - 2367-198X
DOI - 10.1002/solr.202000286
Subject(s) - acceptor , polymer , molecule , photovoltaic system , photochemistry , mass spectrometry , materials science , desorption , ionization , chemistry , organic chemistry , adsorption , ion , ecology , physics , chromatography , biology , condensed matter physics
Although benzoazole‐fused rings with strong quinoid character have successfully been used to construct high‐performance small‐molecule non‐fullerene acceptors (NFAs), studies into how these units influence the stabilities of NFAs and their corresponding device performances are few to date. To address it, four new NFAs, SSTI, SNTI, NTI and NTTI, which adopt BBT, TBZ, and BTAZ as the cores, respectively, are designed and investigated. It is found that SSTI and SNTI based on BBT and TBZ cores with stronger quinoid resonance effects show features of more red‐shifted absorptions and deeper energy levels, but worse thermal and light stabilities than NTI and NTTI with a BTAZ core, especially in solutions and/or films blended with polymer donors. Through matrix‐assisted laser desorption ionization time of flight mass spectrometry analysis of the degradation products, it is disclosed that the CC double bond cleavage would be accelerated by stronger quinoid effects. Therefore, NTI and NTTI with relatively weaker quinoid characteristics show improved photovoltaic properties. Especially, NTTI based devices yield a good efficiency of 8.61% as the side chains on sp3‐hybrid C atoms can prevent the formation of large aggregates. These findings can provide invaluable knowledge for the molecular design of NFAs with both high‐efficiency and high‐stability