Issue 99, 2016, Issue in Progress

Molecular structure simplification of the most common hole transport materials in perovskite solar cells

Abstract

2,2′,7,7′-Tetrakis(N,N-di-p-methoxyphenylamine)-9,9′-spirobifluorene (spiro-OMeTAD) currently is the most common hole transport material (HTM) used in perovskite solar cells (PSCs). Whereas, the hole mobility of amorphous spiro-OMeTAD remains low and may result in severe charge recombination. In addition, the harsh conditions and high cost of spiro-OMeTAD synthesis are also disadvantageous for future large-scale applications. In this paper, we report the synthesis of a new, high-yielding spiro-type HTM, 2,7-di(N,N-di-p-methoxyphenylamine)-2′,7′-di-tert-butyl-9,9′-spirobifluorene (spiro-027). The replacement of two 4,4′-dimeoxyl-diphenylamine at the 2′ and 7′ positions of conventional spiro-OMeTAD with two tert-butyl in spiro-027 results in a greatly simplified molecular structure with unaffected thermal stability or highest occupied molecular orbital (HOMO) and lowest unoccupied molecular orbital (LUMO). In addition, enhanced hole mobility is observed in spiro-027. Thus, the PSC devices based on spiro-027 demonstrated a high power conversion efficiency (PCE) of 16.60%, which was higher than the 16.12% PCE achieved by those based on spiro-OMeTAD. By combining these results with theoretical calculations, our work confirmed the feasibility of simplifying the molecular structure of spiro-OMeTAD, which contributed to our knowledge of spiro-type optoelectronic functional materials. Moreover, our results offer a novel strategy for the replacement of expensive HTMs and the enhancement of PSCs performance.

Graphical abstract: Molecular structure simplification of the most common hole transport materials in perovskite solar cells

Supplementary files

Article information

Article type
Paper
Submitted
26 Aug 2016
Accepted
06 Oct 2016
First published
07 Oct 2016

RSC Adv., 2016,6, 96990-96996

Molecular structure simplification of the most common hole transport materials in perovskite solar cells

Y. Shi, Y. Xue, K. Hou, G. Meng, K. Wang, R. Chi, F. Chen, H. Ren, M. Pang and C. Hao, RSC Adv., 2016, 6, 96990 DOI: 10.1039/C6RA21448G

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