4.7 Article Proceedings Paper

Exploring the role of the spacers and acceptors on the triphenylamine-based dyes for dye-sensitized solar cells

Journal

INTERNATIONAL JOURNAL OF HYDROGEN ENERGY
Volume 43, Issue 9, Pages 4691-4705

Publisher

PERGAMON-ELSEVIER SCIENCE LTD
DOI: 10.1016/j.ijhydene.2017.10.183

Keywords

Triphenylamine; Bis(styryl)benzene; Red shift; Lowest unoccupied molecular orbital; Open-circuit voltage; Dye-sensitized solar cell

Funding

  1. IIT Madras
  2. SERB-N-PDF [PDF/2016/002201]
  3. DST-SERI [CHY/1314/310/DSTX/EDAM]

Ask authors/readers for more resources

Six triphenylamine-based dyes were explored for their application in dye-sensitized solar cells (DSSCs). Dyes 1-3 and dyes 4-6 possess cyanoacrylic acid (C-acceptor) and rhodanine-3-acetic acid (R-acceptor), respectively. Stilbene (in dyes 2 and 5) and bis(styryl)benzene (in dyes 3 and 6) were used as pi-spacers. There is no pi-spacer in the dye 1 and 4. To elucidate the role of pi-spacers, optical, electrochemical, and photovoltaic properties of the dyes were studied. Among C-acceptor dyes, dye 2 exhibits the highest light-to-electricity conversion efficiency of 4.45%, followed by dye 3 (4.16%). Similarly, among R-acceptor dyes, dye 5 is the best. These results indicate that stilbene is a better pi-spacer over bis(styryl) benzene. Although bis(styryl)benzene could extend the light absorption range (in dye adsorbed TiO2 film), its tendency to promote intermolecular pi-pi stacking is possibly the reason for its poor performance in DSSCs. Furthermore, the conjugation break in the R-acceptor moiety attached to the TiO2 surface limits the electron injection of R-acceptor dyes poorer than C-acceptor dyes. Density functional theory calculations were performed for the dye-(TiO2)(8) cluster, assuming a bidentate chelation of a carboxylic acid group with Ti4+ of TiO2 anatase. The natural bond orbital (NBO) analysis indicated relatively more electron-accepting ability of cyanoacrylic acid over rhodanine-3-acetic acid. (C) 2017 Hydrogen Energy Publications LLC. Published by Elsevier Ltd. All rights reserved.

Authors

I am an author on this paper
Click your name to claim this paper and add it to your profile.

Reviews

Primary Rating

4.7
Not enough ratings

Secondary Ratings

Novelty
-
Significance
-
Scientific rigor
-
Rate this paper

Recommended

No Data Available
No Data Available