| Literature DB >> 30079206 |
Hao Zhang1, Yongzhen Wu1, Weiwei Zhang1, Erpeng Li1, Chao Shen1, Huiyun Jiang1, He Tian1, Wei-Hong Zhu1.
Abstract
The use of expensive hole transporting materials (HTMs), such as spiro-OMeTAD, inEntities:
Year: 2018 PMID: 30079206 PMCID: PMC6050542 DOI: 10.1039/c8sc00731d
Source DB: PubMed Journal: Chem Sci ISSN: 2041-6520 Impact factor: 9.825
Fig. 1(a) A schematic illustration of the shift of the HOMO energy level of D–π–D and D–A–D structured organic HTMs. (b) Chemical structures of D–A–D structured HTM TQ1 and TQ2 featuring a moderately electron deficient quinoxaline as the core.
Scheme 1The straightforward synthetic routes to TQ1 and TQ2.
Fig. 2(a) Absorption and emission spectra of TQ1 and TQ2 in CH2Cl2. (b) Absorption spectra of TQ1 and TQ2 in the thin film state. (c) CV spectra of TQ1, TQ2 and spiro-OMeTAD. (d) Energy-level diagram of perovskite solar cells with different HTMs (energy levels of the perovskite, TiO2 and Au are taken from ref. 8).
Photophysical and electrochemical properties of TQ1 and TQ2
| HTM |
|
|
|
|
|
|
| 326 454 | 629 | 2.38 | –5.32 | –2.94 |
|
| 313 336 420 469 | 639 | 2.32 | –5.30 | –2.98 |
Absorption maximum in CH2Cl2 solution.
Peak values of emission spectra in CH2Cl2 solution.
E g was calibrated from the intersection wavelength of normalized emission and absorption spectra by 1240/λ.
The EHOMO was obtained in CH2Cl2 with ferrocene (–5.1 eV vs. vacuum) as an external reference.
Calculated by Eg + EHOMO.
Fig. 3(a) Thermogravimetric analysis of TQ1 and TQ2 measured with a heating rate of 10 °C min–1. (b) The second DSC heating traces of HTMs previously heated and cooled with a scan rate of 10 °C min–1 under a nitrogen atmosphere. (c and d) Top-view AFM images of TQ1 and TQ2 thin films deposited on the perovskite layer, respectively.
Fig. 4(a) The J–V curves for the best-performing devices using TQ1, TQ2, and spiro-OMeTAD as HTMs. (b) IPCE spectra of the solar cell devices based on different HTMs. (c) Statistical distribution in efficiencies of the perovskite solar cells fabricated with TQ1, TQ2, and spiro-OMeTAD as the HTM, respectively.
Photovoltaic parameters for the best-performing devices based on TQ1, TQ2, and spiro-OMeTAD
| HTM | Scan direction |
|
|
| FF [%] | PCE [%] |
|
| Forward | 21.64 | 21.02 | 1.07 | 57.97 | 13.45 |
| Reverse | 21.79 | 1.09 | 60.16 | 14.27 | ||
|
| Forward | 22.52 | 22.09 | 1.11 | 76.80 | 19.20 |
| Reverse | 22.55 | 1.12 | 77.67 | 19.62 | ||
| Spiro-OMeTAD | Forward | 22.50 | 22.11 | 1.08 | 73.96 | 17.97 |
| Reverse | 22.58 | 1.09 | 75.32 | 18.54 |
The integrated current density from the IPCE spectra.
Fig. 5(a) Steady-state PL spectra of the MAPbI3 perovskite films with or without capping different HTMs. (b) Time resolved photoluminescence decay at 770 nm for the pristine perovskite film and the perovskite films capping different HTMs. (c) The space-charge-limited-current (SCLC) measurements of hole only devices with the configuration of ITO/PEDOT:PSS/HTM/Au. (d) The conductivity measurements of TQ1 and TQ2.
Fig. 6Molecular conformations and stacks of TQ1 (a–c) and TQ2 (d–f). The red, yellow, blue, and grey colored atoms represent O, S, N, and C, respectively (the hydrogen atoms have been omitted for clarity).
Fig. 7(a) The J–V curves for the optimized large area (1.02 cm2) devices using TQ2 as the HTM. (b) J–V curves measured from five different spots with an aperture area of 0.09 cm2 selected from the large area device.