
- Journal of Semiconductors
- Vol. 42, Issue 6, 060501 (2021)
Abstract
Star nonfullerene acceptors like ITIC[
Figure 1.(Color online) (a) DTBT and DTBO building blocks, and DTBO-based copolymers P1 and P2. (b) Molecular models and corresponding frontier molecular orbitals and energy levels for D18, P1 and P2. (c)
We built the polymer models for D18, P1 and P2 (Fig. 1(b)). Each model has two repeating units, and the alkyl chains were replaced by methyl groups for saving the calculation time. All structures were optimized at the B3LYP/6-31G(d) level. The DFT-predicted frontier molecular orbitals and energy levels for D18, P1 and P2 are shown in Fig. 1(b). From D18 to P1, DTBT being replaced by DTBO, simultaneous decrease in HOMO and LUMO energy levels was observed. The HOMO and LUMO levels for P1 are –5.05 and –2.69 eV, respectively, which are ~0.1 eV lower than that of D18. A higher Voc was expected for P1-based solar cells since Voc is proportional to the energy difference between donor HOMO and acceptor LUMO[
The synthetic routes for P1 and P2 are shown in Scheme S1. The 5,8-dibromodithieno[3',2':3,4;2'',3'':5,6]benzo[1,2-c][1,2,5]oxadiazole (DTBO-Br) coupled with tributyl(4-(2-butyloctyl)thiophen-2-yl)stannane gave compound 1 in 62% yield. Bromination of compound 1 with NBS gave compound 2 in 80% yield. Copolymerization of compound 2 with (4,8-bis(5-(2-ethylhexyl)-4-fluorothiophen-2-yl)benzo[1,2-b:4,5-b']dithiophene-2,6-diyl)bis(trimethylstannane) (FBDT-Sn) and (4,8-bis(5-(2-ethylhexyl)thiophen-2-yl)benzo[1,2-b:4,5-b']dithiophene-2,6-diyl)bis(trimethylstannane) (BDT-Sn) gave P1 and P2 in 90% and 58% yield, respectively. The number-average molecular weights (Mn) for P1 and P2 are 38.0 and 47.0 kDa, respectively, with the polydispersity indexes (PDI) of 2.08 and 1.67, respectively. P1 and P2 are soluble in chloroform and chlorobenzene. The absorption spectra for P1, P2 and Y6 films are shown in Fig. S7. Both P1 and P2 show two absorption peaks, with a high-energy peak at 545 and 549 nm, respectively, and a low-energy peak at 582 and 590 nm, respectively. The absorption band for P1 and P2 lies in 400–620 nm region, which is complementary with that of Y6 (560–920 nm). The absorption onsets for P1 and P2 films are 626 and 633 nm, respectively, corresponding to optical bandgaps (Egopt) of 1.98 and 1.96 eV, respectively. Energy levels for P1 and P2 were estimated from CV measurements (Fig. S8). The HOMO and LUMO levels for P1 and P2 were calculated from the onset potentials of oxidation (Eonox) and reduction (Eonred), respectively, i.e., HOMO = –(Eonox + 4.8) and LUMO = –(Eonred + 4.8). The energy level diagram is presented in Fig. S9. P1 and P2 show deep HOMO levels of –5.61 and –5.45 eV, respectively, which are favorable for producing high Voc in solar cells. The HOMO level of P1 is 0.1 eV deeper than that of D18 (–5.51 eV)[
Solar cells with a structure of ITO/PEDOT:PSS/polymer:Y6/PDIN/Ag were made to evaluate the performance of P1 and P2. The D/A ratio, active layer thickness and additive (1-chloronaphthalene) content were optimized (Tables S1–S6). J–V curves and external quantum efficiency (EQE) spectra for the best cells are shown in Figs. 1(c) and 1(d), respectively. The best P1:Y6 cells gave a PCE of 10.92%, with a Voc of 0.91 V, a Jsc of 18.22 mA cm–2 and a FF of 65.7%. These cells have a D/A ratio of 1 : 1.6 (w/w), an active layer thickness of 110 nm and no additive. The best P2:Y6 cells gave a PCE of 15.64%, with a Voc of 0.83 V, a Jsc of 26.72 mA cm–2 and a FF of 70.6%. These cells have a D/A ratio of 1 : 1.6 (w/w), an active layer thickness of 120 nm and no additive. The Voc of P1:Y6 cells is 0.05 V higher than that of D18:Y6 cells[
In summary, a fused-ring acceptor unit DTBO was developed. Compared with previously reported DTBT unit, DTBO can lower the HOMO level of polymer donors, thus increasing the Voc of solar cells. DTBO-based copolymers delivered a maximum Voc of 0.91 V and a maximum PCE of 15.64%.
Acknowledgements
This work was supported by the National Key Research and Development Program of China (2017YFA0206600, SQ2020YFE010701), the National Natural Science Foundation of China (51773045, 21772030, 51922032, 21961160720, 51473053) and the Natural Science Foundation of Hunan Province (2019JJ50603).
Appendix A. Supplementary materials
Supplementary materials to this article can be found online at https://doi.org/1674-4926/42/6/060501.
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