Abstract
Hierarchically structured aggregates, consisting of TiO2 nanoparticles were produced via one-step solvothermal syntheses with a mixed solvent system containing both acetic acid and ethanol. Two of the resulting structures, one ~700 nm and the other ~300 nm in diameter, were found to be comprised of 8.5 nm and 10.5 nm anatase crystals, and possess specific surface areas of 138 and 106 m2 g−1 respectively. These particles were incorporated into Dye-sensitized Solar Cells (DSCs) as high surface area scattering layers, along with a layer of a transparent material. Solar-to-electric conversion efficiencies (PCE) of 9.1% and 8.2% were recorded using these aggregated particles as compared to those of commonly used large particles scattering layer 7.4%.
Introduction
Since the breakthrough report by O’Regan and Gratzel in 1991, Dye-sensitized Solar Cells (DSCs) have attracted a great deal of research attention, due to their anticipated low-cost, simple manufacturing processes and promising photocurrent conversion efficiency1–4. A DSC consists of a number of components. Firstly, light is absorbed by a sensitizer to generate an excited state dye, which is capable of injecting electrons into the conduction band of wide band gap metal oxide, with these electrons being then transported through the metal oxide to an external circuit. After charge injection, the cationic sensitizer is reduced back to its neutral form by electrons donated from a redox mediator. Balance in this mediator is maintained by the catalytic counter electrode. The most commonly used materials in DSC for the above four components are organometallic ruthenium complexes, titanium oxide (TiO2), iodide/triiodide redox couple (I3-/I-) and platinum nanoparticles respectively5, 6. To date, the highest efficiencies of DSC have been recorded using TiO2 anatase nanoparticle photoanodes3, 4 due to excellent optoelectronic properties7–9, albeit with different sensitizers and redox electrolyte as compared to the above-mentioned system.
Meta-analysis shows that over 40% of research towards enhancing DSC performance has looked at modifying or developing an efficient photoanode nanostructure6, 10–12. In these studies it has been established that materials for efficient photoanodes should have (1) a large surface area to facilitate high dye loading, leading to high light harvesting efficiency, (2) have a well-connected network of pores for electrolyte diffusion13, (3) facilitate electron transfer (4) have a minimum of defects (both surface and bulk), including those formed at grain boundaries, to limit charge recombination energy losses14. These considerations are however somewhat contradictory. For instance, while decreasing the size of TiO2 nanoparticles increases the surface area, the average pore size is also decreased, limiting diffusion as well as leading to increased numbers of grain boundaries based defects15.
Another strategy to enhance the light harvesting efficiency is the use of light scattering effects as increasing the average path length of light as it travels through the TiO2 film, improving the probability of it being captured by a dye molecule (particularly in the wavelength range where the dye extinction coefficient is the lowest). According to Mie theory, the size of the scattering particle will determine the wavelengths of light which will be scattered efficiently16.
This is typically exploited by employing a bi-layer photoanode structure consisting of a transparent (weakly scattering), underlayer comprised of small particles and a layer of larger (scattering) particles on the top12. Sub-micrometre sized TiO2 spheres have been prepared by sol-gel methods by controlling the hydrolysis reaction and crystallized by subsequent calcination. This procedure has successfully obtained spherical TiO2 structures. However, their low surface area limits their application in DSCs17–19. Recently there has been a trend towards the production of hierarchical TiO2 structures, with large dimensions (effective scattering) consisting of nanoparticles (high dye loading)15, 20–22. Such previous solvothermal approaches used to synthesize hierarchically aggregated TiO2 nanoparticles had long synthesis procedures to control the morphology and/or crystalline phase15, 17, 21, 23–25.
These recent studies motive us to synthesize hierarchical mesoporous structures, with different aggregate sizes (300 ± 65 nm and 700 ± 150 nm, TiO2−300 and TiO2−700 respectively) composed TiO2 nanoparticles (~10.5 nm and ~8.5 nm respectively) in a facile solvothermal approach. We report a new and facile one-step solvothermal approach using titanium isopropoxide (TTIP) as a precursor in a solvent mixture containing acetic acid (AA) and ethanol (EtOH). Subsequently, we investigate their performance in DSCs, which is enhanced as compared to the commonly used, commercially available, light scatting layer (WER2-O). This is explained in terms of high surface area and relatively high light scattering, along with efficient electrolyte penetration through the highly interconnected mesoporous structure.
Results and Discussion
The morphologies and internal structures of the aggregated particles were characterized by scanning electron microscopy (SEM) and transmission electron microscopy (TEM). As shown in the high and low magnification (SEM) images (Fig. 1a,b,e and f). Hierarchical mesoporous structures, with different aggregate size (700 nm and 300 nm designated TiO2-700 and TiO2-300 respectively) composed TiO2 nanoparticles, were formed using mixtures of acetic acid and ethanol as a mixed solvent. SEM images also confirmed that (TiO2-700) and (TiO2-300) show highly connected mesoporous structure as a result of assembling TiO2 nanoparticles into hierarchical spheres and clusters shapes.
Figure 1.
Structural (internal and morphological) characterizations of the calcined TiO2-300 and TiO2-700: (a–d) low and high magnification SEM and TEM images of TiO2-300; (e–h) low and high magnification SEM and TEM images of TiO2-700.
TEM images (Fig. 1c,d,g and h) show that both (TiO2-700) and (TiO2-300) have mesoporous structures, consisting of tightly interconnected and highly crystallized TiO2 nanoparticles with average sizes of (~8.5 nm) and (~10.5 nm) respectively.
X-ray diffraction patterns (XRD) for the two aggregate materials are shown in (Fig. 2a). Both possess polycrystalline tetragonal anatase phase without any impurities or other phases (JCPDS no. 21–1272, a = 3.785 Å, b = 3.785 Å, and c = 9.514 Å) [Fig. S1 shows, this is even true before calcination]. The average crystallite sizes of TiO2-700 and TiO2-300 were ~8.5 nm and ~10.5 nm respectively, based on the Scherrer equation26. The high-resolution TEM (HRTEM) images [Fig. S2] confirmed that (TiO2-700) and (TiO2-300) are composed of nanocrystalline TiO2 with a fringe spacing of approximately (3.5 Å), corresponding to the (101) plane of the TiO2 anatase phase which is consistent with XRD analysis.
Figure 2.

(a) X-ray diffraction patterns. (b) Nitrogen adsorption-desorption isotherms measurements. (c) Pore size distribution calculated from the adsorption branch of a nitrogen isotherm by the Barrett-Joyner-Halenda (BJH) method.
XRD, SEM and TEM analyses clearly demonstrated that both (TiO2-700) and (TiO2-300) have a hierarchical structure consisting of nano-sized TiO2 anatase nanoparticles, providing a highly interconnected mesoporous structure. This is verified by nitrogen adsorption/desorption measurements in (Fig. 2b and Table 1), which showed a type IV isotherm and H3 hysteresis loops at high relative pressures (P/P0 = 0.60–0.95). This indicates the presence of significant mesoporous structures in both (TiO2-700) and (TiO2-300) compared to (WER2-O) and is comparable with that of (18NR-T). Moreover, the hysteresis loops observed for the isotherms, even higher relative pressures (P/P0 = 0.85–0.95), indicate more condensed N2 in the pores and large voids of (TiO2-700) and (TiO2-300) compared to those of (WER2-O) and (18NR-T) leading to the conclusion that the overall surface area is larger for the aggregated particles. Barrett-Joyner-Halenda (BJH) analysis of pore size distribution (Fig. 2c) showed that the internal pore size (formed by aggregation nanoparticles) of (TiO2-700) and (TiO2-300) are (6.2 nm and 9.2 nm) respectively which are smaller than that of transparent layer (18NR-T) due to the smaller nano-size of their primary nanoparticles. However, the observed peak pore size of the Dyesol scattering layer (WER2-O) is around (2.7 nm). Due to the solid structure, this is assumed to arise from surface roughness. The external pore size related to the voids among (WER2-O) and (TiO2-300) particles are around 180 nm and 120 nm respectively due to owing approximately similar particle size. The external pore size of (TiO2-700) is expected to be around 350 nm, however, it is not observed here due to equipment limitations. Brunauer-Emmett-Teller (BET) calculations were conducted and summarized in Table 1. It is therefore expected that (TiO2-700) and (TiO2-300) would be capable of hosting a larger amount of dye, which can lead to higher photocurrent compared to those of (WER2-O). The internal and external pores of (TiO2-700) and (TiO2-300) can provide facile channels for the efficient electrolyte diffusion15, 27.
Table 1.
Porosity (P), Specific surface area (SA) and Surface roughness factor (RF) of 18NR-T, WER2-O, TiO2-700 and TiO2-300 particles.
| Sample | Porosity (%)a | Specific surface area (m2 g−1) | Roughness factor (µm−1)b |
|---|---|---|---|
| TiO2-300 | 63 | 106 | 154 |
| TiO2-700 | 56 | 138 | 235 |
| WER2-O | 35 | 15 | 38 |
| 18NR-T | 67 | 79 | 103 |
aThe porosity calculated as: P = PV/(ρ−1 + PV), where PV is the cumulative pore volume (cm3 g−1) and ρ−1 is the inverse of the density of anatase TiO2 (ρ−1 = 0.257 cm3 g−1). bThe estimated value of the surface roughness factor (RF) is calculated by RF = ρ(1−P)SA 32.
In addition, the aggregate size of around 700 nm and 300 nm, provide good scattering, while having high surface area true in undyed films, however, light travels in the film, hence increasing the probability of absorption light by the dye especially at wavelengths where the dye extinction coefficient is lower.
DSCs based on a bi-layer photoanode structure, incorporating a 18NR-T transparent layer, with either WER2-O, TiO2-700 or TiO2-300 as scattering layers, designated as (18NR-T/WER2-O), (18NR-T/TiO2-700) and (18NR-T/TiO2-300) respectively, along with a single layer (transparent only) (18NR-T) were prepared to investigate the effect of the scattering layers on the photovoltaic properties of the DSC. The current density-voltage characterisations (J-V) and key photovoltaic parameters are summarized in (Table 2) with representative J-V curves in Fig. 3a. DSC based on (18NR-T/TiO2-300) and (18NR-T/TiO2-700) photoanodes showed a significant enhancement in the photocurrent conversion efficiency compared to these using (18NR-T) or (18NR-T/WER2-O) photoanodes, with efficiencies of 8.2%, 9.1%, 7.2%, and 7.4% respectively. The higher efficiency of DSC devices based on (18NR-T/TiO2-300) and (18NR-T/TiO2-700) photoanodes is mainly due to enhanced J sc while FF and V oc are fairly consistent (Table 2). Dye loading on the (TiO2-700 and TiO2-300) films is significantly higher than that of (WER2-O) and comparable to that of Dyesol transparent layer (18NR-T) as seen from desorption experiments (Fig. 3b and Table 3). The hierarchical mesoporous structure of (TiO2-700) and (TiO2-300) based on high surface area aggregated nanoparticles can host more dye molecules, leading to higher J sc while the very low surface area of (WER2-O) can result in lower J sc due to the poor dye loading.
Table 2.
J-V characterizations of DSC devices.
| Device | J sc (mA cm−2) | V oc (V) | FF (%) | PCE (%) |
|---|---|---|---|---|
| 18NR-T/TiO2-300 | 14.1 ± 0.4 | 0.79 ± 0.01 | 69 ± 1 | 8.2 ± 0.2 |
| 18NR-T/ TiO2-700 | 16.1 ± 0.1 | 0.80 ± 0.01 | 71 ± 1 | 9.1 ± 0.1 |
| 18NR-T/WER2-O | 13.8 ± 0.3 | 0.79 ± 0.01 | 67 ± 1 | 7.4 ± 0.3 |
| 18NR-T | 12.3 ± 0.7 | 0.83 ± 0.01 | 70 ± 1 | 7.2 ± 0.4 |
Figure 3.
(a) J-V characteristics of DSC devices measured under 1 sun illumination with an area of 0.16 cm2; (b) absorbance spectra of the dye solution desorbed on the different scattering layers; (c) Incident photon to current conversion efficiency (IPCE) curves of DSCs.
Table 3.
The amount of dye on TiO2-300, TiO2-700, WER2-O and 18NR-T films.
| Film | Dye loading (10−7 mol cm−2) | Dye loading (10−5 mol cm−3) |
|---|---|---|
| TiO2-300 | 0.55 | 14 |
| TiO2-700 | 0.63 | 16 |
| WER2-O | 0.32 | 4 |
| 18NR-T | 0.61 | 15 |
Electrochemical Impedance Spectroscopy (EIS) measurements were carried out to compare electron transfer and lifetime of devices based on bi-layer photoanodes. Nyquist plots of all the devices showed similar electrochemical interface impedance response. However, device based on (18NR-T/WER2-O) showed a more depressed arc in the second semicircle (lower frequencies) which is related to electron transfer at the TiO2 interface with FTO and the electrolyte (Fig. S3a and Table S1). Fittings for all these deives use CPE, as opposed to capacitive elements, in the model as the double layer interfaces between the electrolyte/photoanode are non-ideal and act as a leakage capacitor28.
Bode plots were used to estimated lifetime (τ = 1/2πf max)29 of injected electrons from dye through photoanode to the charge collector (FTO). (Fig. S3b) showed that the maximum value of frequency of devices based on (18NR-T/TiO2-700) and (18NR-T/TiO2-300) photoanodes were located at (20 Hz) and (25 Hz) respectively which is lower than that of (18NR-T/WER2-O) (38 Hz), implying that the lifetimes of electron transfer through (18NR-T/TiO2-700) and (18NR-T/TiO2-300) photoanodes are longer than in (18NR-T/WER2-O) due to reduced electron recombination and/or faster electron diffusion through high surface area hierarchical crystalline structure (there are more boundaries in the aggregates and increased surface area).
The enhancement in photocurrent densities and its relationship to enhanced light harvesting efficiency was also further investigated with an incident photon to current conversion efficiencies (IPCE) measurements. In Fig. 3c. devices based on (18NR-T/TiO2-300) and (18NR-T/TiO2-700) showed higher IPCE values in the entire measured wavelength range (300–800 nm) along with a broader shape around than those of (18NR-T) and (18NR-T/WER2-O), (Fig. 3c and Fig. S4), even though (WER2-O) itself was more scattering than the aggregates. Peak IPCE values were nearly identical, while more marked differences in the red part of the spectrum were seen, where the dye absorption is lower.
The light-scattering effect can be evaluated by measuring the diffuse reflection of photoanode films. Figure 3d shows the reflectance spectra of different photoanode films in the range of (400–800 nm). (18NR-T/WER2-O) photoanode showed the strongest diffuse reflection (65–85%) which is higher than that of (18NR-T/TiO2-700) and (18NR-T/TiO2-300) photoanodes respectively which are in turn, have higher diffuse reflection (40–60%) than that of transparent layer (18NR-T) (20–30%). The lower diffuse reflection of (18NR-T/TiO2-700) and (18NR-T/TiO2-300) (40–60%) compared to (18NR-T/WER2-O), is probably due to owning high porosity structure resulting in the less dense film (not being solid particles) (Table 1) and (Fig. 4).
Figure 4.
Schematic of DSC devices based on (18NR-T/WER2-O), (18NR-T/TiO2-700) and (18NR-T/TiO2-300) photoanodes with their multifunctional properties including dye loading, scattering light, and electrolyte diffusion trough mesoporous structure.
Conclusion
High PCE has been realized through the use of aggregated TiO2 structure as scattering layers. The sub-micro size hierarchical mesoporous spheres TiO2-700 comprised of 8.5 nm TiO2 nanoparticles, prepared by a simple one-step solvothermal method, provided the highest PCE of 9.1% in conjunction with a transparent TiO2 layer. This resulted from combined effects of higher dye loading, efficient electrolyte diffusion through the highly connected mesoporous structure and good light scattering properties. To the best of our knowledge, this is the highest efficiency for aggregated nanoparticles hierarchical microsphere as scattering layers with a commercial transparent TiO2 layer22, 24, 30, 31.
Experimental
Synthesis of TiO2-700 and TiO2-300
TiO2-700 and TiO2-300 were synthesized by a facile one-step solvothermal process. Briefly, Titanium isopropoxide (TTIP) (0.5 ml) was added dropwise to an acetic acid-ethanol mixed solvent under vigorous stirring for (1 h) at room temperature. A clear solution was formed which was transferred into a Teflon-lined stainless steel autoclave, 45 mL (Parr Instrument Company) heated to 180 °C (ramp time of 1 °C/min) for 9 h, after cooling down to room temperature the resulting white precipitate was collected and washed with distilled water and ethanol three times and then dried overnight at 90 °C. Finally, the samples were calcined at 400 °C (ramp time of 1 °C/min) in air for three hours. The morphologies, particle size and surface area of TiO2-700 and TiO2-300, were controlled by adjusting the acetic acid-ethanol volume ratio (AA:EtOH v/v) with keeping other solvothermal reaction conditions constant. The typical volume ratio of (AA: EtOH v/v) were used to synthesize TiO2-700, and TiO2-300 were (1:5 in ml) and (1:3 in ml) respectively.
Preparation of photoanodes and DSCs assembly
Fluorine-doped tin oxide (FTO) glass was sequentially cleaned using soapy water, acetone, and ethanol in an ultrasonic bath for 20 min per solvent. A blocking layer of TiO2 was deposited on the cleaned FTO substrate using spray pyrolysis of titanium (IV) diisoproxide-bis-acetylacetonate (75 wt.% in isopropanol, Aldrich) solution (1:9 v/v in ethanol) at 450 °C. Scattering pastes (WER2-O, Dyesol Australia, TiO2-700 and TiO2-300 or as described below) were printed on the top of a single transparent layer (18NR-T, Dyesol Australia) using a Keywell screen printer with a custom mesh (43 T) to form 4 mm × 4mm (0.16 cm2) photoanodes. The printed transparent layer (18NR-T) was dried at 125 °C before scattering layers were deposited. Pastes of TiO2-700 and TiO2-300 were prepared using 1.0 g of TiO2 ground in a mixture of ethanol (25 ml), distilled water (1 ml), and acetic acid (0.2 ml). After that terpineol (5 g) and ethyl cellulose (0.5 g) were added to form a slurry which was sonicated and stirred for (2 h)32, 33. A viscous white paste was finally obtained after an evaporation process to remove water and ethanol. TiO2-700 and TiO2-300 scattering pastes were printed (thickness = 5.5 µm) on the top of a single transparent layer (18NR-T, Dyesol Australia) (thickness = 6.5 µm). For comparison, the photoanode including a single transparent layer (18NR-T) and a commercial scattering layer [Dyesol Australia WER2-O reflective Titania paste (thickness = 5.5 µm)] was printed. After that, the printed photoanodes were sintered using a multi-step program (up to 550 °C). Finally, the photoanodes were surface treated by soaking the photoanodes in (20 mM) aqueous solution of TiCl4 (Sigma) for 30 min at 70 °C, then washed and re-sintered at (500 °C for 30 min).
After cooling down to 110 °C, the photoanodes were immersed in an N719 dye solution (0.5 mM, Solaronix). The dye solution was a mixture of tert-butanol (LR, Ajax Chemicals) and acetonitrile (HPLC, Lab-scan) [1:1 v/v], the photoanodes were taken out from dye solution after 24 h and washed with acetonitrile and then dried. Counter electrodes were prepared by first drilling holes in a separate piece of FTO glass, to be used as a filling port for the electrolyte solution. One drop of (10 mM) H2PtCl6 solution (in ethanol) was smeared on the cleaned pre-FTO counter electrode and heating to 400 °C for 20 min. The counter electrodes are cooled before being sandwiched together with the photoanode, using a 25 µm Surlyn (Solaronix) spacer, by a hot press. The electrolyte solution [acetonitrile/Valeronitrile (85:15 vol %), iodine (I2) (0.03 M), 4-tertbutyl pyridine (4-tBP) (0.5 M), 1-butyl-3-methylimidazolium iodide (BMII) (0.6 M), and guanidinium thiocyanate (GuSCN) (0.1 M)] was introduced into the filling port by the vacuum back-filling technique, and the filling port was then closed with a piece of Surlyn laminated to aluminium foil.
Material Characterizations
The crystalline structures of TiO2-700 and TiO2-300 were examined using X-ray diffractometer (Bruker Advance, 40 kV, 30 mA) (Cu Kα, λ = 1.5406 Å) in range (2θ = 20°–80° with scan rate (1°/min). The morphology and internal structure of samples were examined by field-emission scanning electron microscopy (FE-SEM) (JEOL JSM-7500) and transmittance electron microscopy TEM (JEOL JEM-2010). Brunauner-Emmet-Teller (BET) surface area, as well as BHJ porosity and pore volume values, were determined from data collected on (Microtrac Belsorp-mini) nitrogen adsorption-desorption equipment. The amount of dye on the different scattering layers was calculated by measuring the absorbance of dye desorbed from the films (thickness = 4 µm, area = 1 cm2) in (4 ml) of (0.1 M) NaOH solution (distilled water: ethanol 1:1 v/v) using a Shimadzu UV-3600 spectrophotometer. The light scattering properties (diffuse reflectances) were measured using an integrating sphere (ISR-3100) and the above spectrophotometer. A Veeco Dektak 150 Surface Profiler was used for the film thickness measurements. Photocurrent density-voltage (J-V) measurements were measured using a solar simulator with AM1.5 filter; set to 1 sun (100 mW/cm2, PV Measurements, Colorado). A QEX10 system from (PV Measurements) was used for the incident to photocurrent conversion efficiency (IPCE) measurements in 5 nm steps. The measured currents were referenced to a calibrated Si photodiode. A Reference 600 Potentiostat (GAMRY instrument) was used for electrochemical impedance spectroscopy measurements (EIS) which were carried out for DSCs based on different photoanodes under 1 sun illumination at V oc in a frequency range (0.1–106 Hz) and AC voltage 10 mV.
Electronic supplementary material
Acknowledgements
This work is supported by Australian Research Council Discovery Projects (ARC). The authors would like to thank the Australian National Fabrication Facility (ANFF) and Electron Microscope Center (EMC) for access to equipment. Dr. Andrew Nattestad would like to acknowledge the ARC for funds (DE160100504) and (DP160102627). Kadhim Al-Attafi would like to acknowledge the Higher Committee for Education Development in Iraq (HCED) for financial support.
Author Contributions
K.Al-Attafi, A.N., and J.H.K designed experiments. K.Al-Attafi performed synthesis experiments, TEM, SEM and DSC measurements. Y.Y. performed BET measurements. K.Al-Attafi, A.N., and J.H.K analyzed the data and wrote the manuscript. A.N., J.H.K, and S.X.D supervised the work. All authors discussed the results and contributed to revisions.
Competing Interests
The authors declare that they have no competing interests.
Footnotes
Electronic supplementary material
Supplementary information accompanies this paper at doi:10.1038/s41598-017-09911-w
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Contributor Information
Andrew Nattestad, Email: anattest@uow.edu.au.
Jung Ho Kim, Email: jhk@uow.edu.au.
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