Hole-Transporting Materials for Printable Perovskite Solar Cells
Abstract
:1. Introduction
2. Perovskite Solar Cells
2.1. Mesoscopic and Planar Architectures
2.2. Current Challenges of Perovskite Solar Cells Research
3. Hole-Transporting Materials
- prevent the direct contact between the perovskite and the metal contact, which minimizes charge recombination and avoids degradation at the metal-perovskite interface;
- extract positive charges (holes) from perovskite and transport them to the top-electrode.
- high costs: spiro-OMeTAD is prohibitively expensive (~500 $/g) [39] because of (a) its onerous multistep synthesis that requires a low temperature (−78 °C); (b) the sensitive (n-butyllithium or Grignard reagents) and aggressive (Br2) reagents involved in the synthetic scheme [40]; (c) the costly sublimation step required for purification [41].
- negative impact on stability: the use of spiro-OMeTAD limits the long-term stability of the devices [39], thus inhibiting the upscaling application in the photovoltaic industry.
- sub-optimal charge transport: when in pristine form, spiro-OMeTAD shows a modest hole-mobility and conductivity (1.67 × 10−5 cm2 V−1 s−1 and 3.54 × 10−7 S cm−1, respectively) [42], thus requiring additives and chemical p-dopants to enhance the hole conductivity by 10-fold and thus the conversion efficiency of PSCs.
3.1. Organic Hole-Transporting Materials
3.1.1. Small-Molecule-Based HTMs
3.1.2. Polymer-Based Hole-Transporters
3.2. Inorganic Hole-Transporting Materials
3.3. Hybrid Hole-Transporters
4. Concluding Remarks and Future Perspectives
- Appropriate ionization potentials are essential to guarantee efficient transfer of the photoexcited holes from the perovskite layer to the HTM.
- Low electron affinities are required to avoid electron recombination at the perovskite|HTM interface.
- HTMs should also be highly transparent, low-cost and present good film-forming properties at the same time, which ensure smooth and pinhole-free coverage.
- High mobility: Doping of the organic HTMs is in most cases necessary to ensure high cells performance, but it is usually responsible for significant degradation processes compared to pristine HTMs. To enhance the stability, it would be ideal to avoid any dopant to the pristine HTM. This requires the HTM to have high mobility. Research efforts in this direction must continue, starting from the promising achievements about the highly order columnar design concept as a strategy to facilitate the mobility of charge-carriers by face-on arrangement. This was the case of material Triazatrux-VII, which demonstrated how to enhance the hole-mobility to achieve exceptional device performance.
- If the use of dopants cannot be avoided because of the poor hole-mobility of the pristine HTM, hydrophobic dopants or air-stable additives should be chosen, as alternatives to the highly unstable dopants commonly used at present (LiTFSI, TBP, FK 209).
Acknowledgments
Author Contributions
Conflicts of Interest
References
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Category | HTM | PCE (%), HTM | PCE (%), Spiro-OMeTAD | Reference |
---|---|---|---|---|
Pyrene-based | PY-1 | 3.3 | 12.70 | [55] |
PY-2 | 12.3 | 12.70 | [55] | |
PY-3 | 12.4 | 12.70 | [55] | |
Truxene-core | Trux-I | 18.6 (10.2 [56]) | 16.0 (9.5 [56]) | [57] |
Trux-II | 13.4 | 9.50 | [56] | |
Triazatrux-I | 8.9 | 17.10 | [58] | |
Triazatrux-II | 17.7 | 17.10 | [58] | |
Triazatrux-III | 15.8 | 17.10 | [58] | |
Triazatrux-IV | 11.5 | 17.10 | [58] | |
Triazatrux-V | 8.88 | 19.01 | [59] | |
Triazatrux-VI | 14.87 | 19.01 | [59] | |
Triazatrux-VII | 19.03 | 19.01 | [59] | |
Phenothiazine-based | PH-I | 2.10 | 17.70 | [60] |
PH-II | 17.60 | 17.70 | [60] | |
Acridine-, thiophene-, biphenyl-, bithiophene-, tetrathiophene-, difluorobenzene, and phenyl-based | AC-I | 16.42 | 16.26 | [61] |
Thio-I | 9.05 | 8.83 (15.63) 1 | [62] | |
Thio-II | 15.13 | 8.83 (15.63) 1 | [62] | |
BPH-I | 13.27 | 16.81 | [63] | |
BPH-II | 16.42 | 16.81 | [63] | |
BTHIO | 19.40 | 18.80 | [64] | |
TETRATH-I | 18.13 | 17.80 | [65] | |
TETRATH-II | 17.3 | 17.80 | [65] | |
TETRATH-III | 15.7 | 17.80 | [65] | |
TETRATH-IV | 9.7 | 17.80 | [65] | |
DFTAB | 10.4 | 15 | [66] | |
Triazine-based | TRIAZ-I | 12.5 | 13.45 | [67] |
TRIAZ-II | 10.9 | 13.45 | [67] | |
TRIAZ-III | 13.2 | 13.8 | [68] | |
TRIAZ-IV | 12.6 | 13.8 | [68] | |
Benzotrithiophene- and squaraine-based | BZTR-I | 16 | 18.1 | [69] |
BZTR-II | 17 | 18.1 | [69] | |
BZTR-III | 18.2 | 18.1 | [69] | |
BZTR-IV | 19 | 18.9 | [70] | |
BZTR-VHYX | 18.2 | 18.9 | [70] | |
SQ-H | 14.74 | 15.33 | [71] | |
SQ-OC6H13 | 14.73 | 15.33 | [71] | |
Fluorene- and spiro-fluorene-based | FL-I | 17.8 | 18.4 | [72] |
FL-II | 16.73 | 14.84 | [73] | |
FL-III | 17.25 | 16.67 | [74] | |
FL-IV | 15.90 | 16.67 | [74] | |
FL-V | 14.52 | 17.88 | [75] | |
FL-VI | 15.09 | 17.88 | [75] | |
FL-VII | 9.15 | 17.88 | [75] | |
FL-VIII | 16.79 | 17.88 | [75] | |
FL-IX | 16.45 | 17.88 | [75] | |
Spiro-FL-I | 19.8 | 20.8 | [76] | |
Spiro-FL-II | 13.6 | 18.8 | [77] | |
Spiro-FL-III | 20.8 | 18.8 | [77] | |
XDB | 5.4 | 5.5 | [78] | |
XOP | 15.0 | 5.5 | [78] | |
XMP | 16.5 | 5.5 | [78] | |
XPP | 17.2 | 5.5 | [78] | |
FDT | 20.2 | 19.7 | [39] | |
SPI-BI | 17.77 | 18.25 | [79] | |
SPI-TH | 19.96 | 18.25 | [79] | |
SPI-TRI | 19.47 | 18.25 | [79] | |
SPI-FL-MM-3PA | 13.46 | 14.98 | [80] | |
SPI-FL-MP-3PA | 15.59 | 14.98 | [80] | |
SPI-FL-MM-2PA | 12.56 | 14.98 | [80] | |
SPI-FL-MP-2PA | 13.43 | 14.98 | [80] | |
Carbazole-based | CA-I | 12.3 | 12.17 | [81] |
CA-II | 8.5 | 10.2 | [82] | |
CA-III | 10.2 | 10.2 | [82] | |
CA-IV | 13.28 | 15.23 | [83] | |
CA-V | 14.79 | 15.23 | [83] | |
CA-VI | 13.86 | 15.23 | [83] | |
CA-VII | 4.53 | 5.10 | [84] | |
CA-VIII | 0.19 | 5.10 | [84] | |
CA-IX | 7.6 | 10.2 | [85] | |
CA-X | 9.8 | 10.2 | [85] | |
CA-XI | 10.96 | 13.76 | [86] | |
CA-XII | 12.61 | 13.76 | [86] | |
CA-XIII | 13.0 | 13.76 | [86] | |
CA-XIV | 11.4 | 12.0 | [87] | |
CA-XV | 13.1 | 12.0 | [87] | |
CA-XVI | 17.8 | 18.6 | [88] | |
CA-XVII | 17.81 | 18.59 | [89] | |
CA-XVIII | 12.42 | 14.32 | [90] | |
CA-XIX | 14.92 | 15.01 | [91] | |
CA-XX | 16.74 | 15.01 | [91] | |
CA-XXI | 0 | 15.01 | [91] | |
CA-XXII | 13.30 | 15.01 | [91] | |
CA-XXIII | 16.87 | 15.53 | [92] | |
Other small molecules (Naphthalene (NPH), di- and tetra-phenylmethane (DPA-TPM, TPA-TPM), and ethylene dioxythiophene (EDOT)) | NPH-I | 10.05 | 10.06 | [93] |
NPH-II | 8.66 | 10.06 | [93] | |
OMe-I | 18.34 | - | [94] | |
OMe-II | 16.14 | - | [94] | |
Thiazo-I | 10.60 | - | [95] | |
Thiazo-II | 4.37 | - | [95] | |
Thiazo-III | 8.63 | - | [95] | |
Ph-TPM | 4.62 | 15.49 | [96] | |
DPA-TPM | 9.33 | 15.49 | [96] | |
TPA-TPM | 15.06 | 15.49 | [96] | |
EDOT-AZO | 11.0 | 11.9 | [97] |
HTM | PCE (%), HTM | PCE (%), Reference | Reference |
---|---|---|---|
PTAA | 22.1 | - | [12] |
P3HT | 13.0 | [108] | |
PEDOT:PSS | 18.1 | [30] | |
PDPP3T | 12.32 | 12.34 | [112] |
PCDTBT | 15.9 | 16.6 | [113] |
PCPDTBT | 15.1 | - | [115] |
HB-CZ | 14.07 | 9.05 (P3HT), 6.60 (PCz) | [116] |
PDVT-10 | 13.4 | 11.28 (PTAA) | [117] |
PVCz-OMeDAD | 16.09 | 9.62 | [118] |
PBDTT-FTTE | 11.6 | 10.3 | [119] |
Scan Direction | VOC (V) | JSC (mA/cm2) | FF (%) | PCE (%) |
---|---|---|---|---|
Forward | 1.03 | 20.58 | 74.7 | 15.89 |
Reverse | 1.03 | 20.66 | 74.2 | 15.90 |
© 2017 by the authors. Licensee MDPI, Basel, Switzerland. This article is an open access article distributed under the terms and conditions of the Creative Commons Attribution (CC BY) license (http://creativecommons.org/licenses/by/4.0/).
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Vivo, P.; Salunke, J.K.; Priimagi, A. Hole-Transporting Materials for Printable Perovskite Solar Cells. Materials 2017, 10, 1087. https://doi.org/10.3390/ma10091087
Vivo P, Salunke JK, Priimagi A. Hole-Transporting Materials for Printable Perovskite Solar Cells. Materials. 2017; 10(9):1087. https://doi.org/10.3390/ma10091087
Chicago/Turabian StyleVivo, Paola, Jagadish K. Salunke, and Arri Priimagi. 2017. "Hole-Transporting Materials for Printable Perovskite Solar Cells" Materials 10, no. 9: 1087. https://doi.org/10.3390/ma10091087
APA StyleVivo, P., Salunke, J. K., & Priimagi, A. (2017). Hole-Transporting Materials for Printable Perovskite Solar Cells. Materials, 10(9), 1087. https://doi.org/10.3390/ma10091087