Jian Tao Wang,
Xin Hua Zhong and
Jian Nong Wang*
Nanomaterials Research Center, School of Mechanical and Power Engineering and School of Chemistry and Molecular Engineering, East China University of Science and Technology, 130 Meilong Road, Shanghai, 200237, P. R. China. E-mail: jnwang@ecust.edu.cn; Tel: +86-21-64252360
First published on 8th June 2015
Current development of fluorine-doped tin oxide (FTO) films for application in solar cells is limited by tradeoffs among surface roughness related light trapping, optical transparency and electrical conductivity. Proposed methods for improving the surface roughness are usually dependent upon thickness increment or sacrificing the conductivity. In this study, we report a simple method for preparing FTO films with a flower-like grain morphology and thus a higher than ever mean roughness of 51.4–73.3 nm or mean-root-square roughness of 70.5–91 nm, by inclusion of HNO3 additive into the deposition system. The very rough films are 200–300 nm thick and also have maintained a high transparency of 80–85% in the visible region and a low sheet resistance of 14 Ω □−1 and resistivity of 4.2 × 10−4 Ω cm, perhaps resulting from the effects of HNO3 on heterogeneous nucleation and development of the (200) preferred orientation. The high roughness, combined with high transparency and low resistivity, would be beneficial to improving the light trapping of FTO films and thus the efficiency of solar cells.
Solar cell is a device which converts the solar energy into useful electrical energy. The main application of FTO thin films in this field is as the front electrical contact, which allows the solar spectrum in the visible region to pass through. A high optical transmittance is required for an efficient transport of light into the active stack, and a good electrical conductivity for a low transport loss of the generated electrical energy. In general, an excellent transparency (more than 80%) in the visible range and low electrical conductivity (<10−3 Ω cm) are essential for the front FTO films.9,10
In addition to transparency and conductivity, the light trapping ability of the film is another important factor to affect the efficiency of solar cells.11 A light trapping structure contributes to increase the light path length by reflecting and scattering the incident light at different angles. Since a high surface roughness is beneficial to diffuse transmission or total internal reflections of lights and reduce the optical losses in the film,12,13 roughness enhancement has been regarded as an effective method for enhancing light trapping12,14–16 and thus energy conversion efficiency of solar cells.17–22
For TCO thin films, some approaches have been used to enhance the surface roughness determined as either Ra, the mean roughness, or Rmrs, the mean root square roughness. The primary previous method for increasing roughness was increasing the film thickness.13,18 However, increasing film thickness always decreased the transparency. Alternatively, roughness was increased by adding additives into the deposition system, including alcohols and chelating reagents.3,13 However, the thickness effect was not eliminated. Recently, we reported a significant increase in roughness Ra from 13 to 60 nm, the highest ever reported, particularly at a low thickness of 300 nm by adding NH3 to the deposition process.23 However, the conductivity of the FTO film decreased noticeably, as evidenced by increases of sheet resistance from 14 to 35 Ω □−1 and resistivity from 4.2 × 10−4 to 10.5 × 10−4 Ω cm. The loss of conductivity could have a negative effect on photovoltaic applications, and thus should be suppressed.
Although great efforts have been made, effective methods for improving the roughness of FTO thin films without sacrificing transparency and conductivity are still lacking. In this study, we report the addition of HNO3 into the system of atmospheric pressure chemical vapor deposition (APCVD) for improving roughness. Corresponding to these roughness increases, the resistivity and the transmittance maintained at a high level. The roughness enhancement is illustrated to be related to the development of a flower-like grain morphology on the film surface.
The surface morphology of FTO films was examined with a Hitachi High-Technology S-4800 field emission scanning electron microscope (FE-SEM) at an accelerating voltage of 5 kV. Atomic force microscopy (AFM) measurement was performed with Nanoscope IIIa Multimode AFM with the roughness analysis being conducted by the software of Nanoscope 5.30. The structures of FTO thin films were investigated by X-ray diffraction (XRD) at room temperature with a Rigaku D/max 2550 VB/PC apparatus using Cu Kα radiation (λ = 0.15406 nm) and a graphite monochromator, operated at 40 kV and 100 mA. Diffraction patterns were recorded in the angular range of 20–80° with a step width of 0.02° s−1. An ION-TOF 5 Time of Flight Secondary Ion Mass Spectrometry (TOF-SIMS) instrument was used to obtain a compositional positive ion depth profile for several coatings. The analysis beam was Bi3+ and the sputter beam was 1 keV Cs+ with a beam current of 82+/−2 nA. The sputter beam was rastered over a 200 × 200 micron area, and the bismuth analysis beam was rastered over a 50 × 50 micron area at the centre of the sputtered region.
At the wavelength higher than 1200 nm, the transmittance began to decrease to be lower than 80% and decreased rapidly with increasing wavelength. The addition of HNO3 appeared to reduce such decrease. With increasing the feeding rate of HNO3, it was particularly evident that the decrease was slower than the one without HNO3.
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| Fig. 2 The amount of F doping in the baseline film (a), XRD pattern (b) and the texture coefficients of the main diffraction planes (c) for FTO thin films prepared with different additions of HNO3. | ||
XRD patterns for the baseline sample and those with addition of HNO3 are shown in Fig. 2b. It is illustrated that SnO2 crystals were polycrystalline with a rutile tetragonal structure. Peaks for SnO or Sn phases were not detected, indicating that the films were fully oxidized. No appreciable peak shift could be observed, which was reasonable considering that the doping level was relatively small for this system and the anionic radii were rather similar. This result also verified the small amount of F doping measured by TOF-SIMS. The major XRD peaks are associated with diffractions of (200), (110), and (211) planes, and the minor diffractions of (101), (301), and (310) planes are also indexed. The diffraction intensities of these planes varied with HNO3 feeding rate. For the baseline sample, the diffraction of (200) plane was dominant. With increasing HNO3 addition, the relative intensity of (200) plane showed an apparent increase first and then a decrease, but that of (211) plane a decrease first and then a gradual increase, suggesting a possible change in preferred orientation of the deposited film.
The feature of the preferred orientation of a thin film can be quantified by the texture coefficient (TC) which is calculated from the XRD of (hkl) plane as follows:24
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The TC values for the major diffraction planes are depicted in Fig. 2c. It is clearly shown that the TC for (200) increased to a high value with 1.5 mL min−1 HNO3 addition but then decreased with more addition. In contrast, the TC for (110) and particularly that for (211) declined first and then increased. Especially, with 2.25 mL min−1 HNO3 addition, the TCs for (110) and (211) were much larger than that for TC (200). This led to that (110) and (211) planes substituted for (200) plane as the preferred orientation with increasing HNO3 addition.
With more HNO3 addition the surface morphology changed significantly. In the case of 1.5 mL min−1 addition, flower-like grains appeared and dispersed on the surface of the film, while the background grains had no significant difference from the baseline sample except for smaller grain sizes (Fig. 3c–h). The size of the flower-like grains was around 300 nm in the lateral dimension, but the population of such grains appeared to decrease significantly in the films prepared with a thickness of 500 nm (Fig. 3e and f), compared with those prepared with a thickness of 200 nm (Fig. 3c and d) or 300 nm (Fig. 3e and f). The variation of the background grain size is attributed to the thickness change.
The surface morphology was also characterized by AFM measurements. Fig. 4 shows the AFM images for the films prepared with the same thickness of 300 nm but with different HNO3 additions. From these images, the surface of the film prepared with 1.5 mL min−1 HNO3 addition illustrates the presence of abundant high peaks which correspond to the flower-like grains observed in SEM images. Such film had a Ra roughness as high as 51.4 nm (Rmrs: 70.5 nm) (Table 1). All other film surfaces showed the absence or only a few high peaks, leading to a much smaller roughness.
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| Fig. 4 AFM images of FTO thin films of 300 nm thick prepared at different feeding rates of HNO3 (mL min−1). (a) 0, (b) 0.5, (c) 1, (d) 1.5, (e) 1.8, and (f) 2.25. | ||
| Feeding rate (mL min−1) | Film thickness (nm) | Sheet resistance (Ω □−1) | Resistivity × 10−4 (Ω cm) | Ra (nm) | Rmrs (nm) |
|---|---|---|---|---|---|
| 0 | 300 | 14 | 4.2 | 13 | 17 |
| 1 | 300 | 14 | 4.2 | 7.5 | 10.4 |
| 1.5 | 300 | 14 | 4.2 | 51.4 | 70.5 |
| 1.8 | 300 | 21 | 6.3 | 18.8 | 27.2 |
| 2.25 | 300 | 45 | 13.5 | 16.6 | 20.2 |
| 1.5 | 100 | 170 | 17 | 18.5 | 25.7 |
| 1.5 | 200 | 43 | 8.6 | 73.3 | 91.0 |
| 1.5 | 500 | 10 | 5 | 24.0 | 36.6 |
In order to investigate the growth process of the flower-like grains, the AFM surface morphologies of the films prepared with 1.5 mL min−1 HNO3 addition but with different thicknesses were examined (Fig. 5). It is revealed that the flower-like grains formed in the early stage of the deposition process. With increasing thickness, the size of such grains increased, but the number of such grains decreased beyond the thickness of 300 nm (Fig. 4d). Such a morphological variation generated a Ra roughness up to 73.3 nm (Rmrs: 91 nm) on the film of 200 nm thick but a Ra roughness of only 24 nm on the film of 500 nm (Table 1).
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| Fig. 5 AFM images of FTO thin films prepared at 1.5 mL min−1 of HNO3 with a thickness of 100 (a), 200 (b), and 500 nm (c). See Fig. 4d for the film prepared under the same condition with a thickness of 300 nm. | ||
Fig. 6a and b illustrates the variation of roughness with film thickness for typical previous and present FTO films. One of the unique features of the present roughness is that it was not only the highest among those ever reported but also it was observed for the films with a thickness of as low as 200 or 300 nm. This is different from the previous relatively high roughness within the range of 40–55 nm for the films (including commercial ones) with a thickness of >700 nm.13,15,18,25,26 The consequence is that the present very rough films had a transmittance value of 85–90% at the wavelength of 550 nm, which is much higher than those for previous thick films (<80%). Thus, improving the surface roughness was not in tradeoff with transmittance in the present study.
The further unique feature of the present roughness is that as a low amount of HNO3 was used as the additive, the sheet resistance of the rough film remained at a low level. For example, the very rough film of 300 nm thick had a resistivity of 4.2 × 10−4 Ω cm, one of the lowest resistivity ever reported for FTO films (Fig. 6c and d). This observation indicates that although the surface morphology and roughness were changed, the carrier concentration and mobility which are responsible for electrical conductivity did not change very much.
The unique features of the present rough film are apparently related to the use of HNO3 as the additive. Deposition of FTO thin films requires the presence of tin, fluorine and oxygen sources. It is the complex interplay between these components in the reactor that controls the film formation and deposition. The microstructures of thin films are determined in part by surface diffusion and nucleation processes on the growth interface. This in turn is affected by substrate temperature, reactor pressure, and gas-phase composition.27 Additives, when they are introduced in different amounts, modify the reaction chemistry and flow rate, which leads to the changes of film formation, growth rate, surface morphology and roughness.
The addition of HNO3 might have induced a special nucleation and crystal growth processes, which did not taken place with other additives before. HNO3 is well known being a strong oxidizing acid, especially at the high temperature of 600 °C. In the presence of HCl and/or HF from DMTDC and TFAA, respectively, HNO3 could have even caused corrosion of the substrate glass used for FTO film deposition. During nucleation, the heterogeneous nucleation was much more common than homogeneous nucleation. An uneven or corroded surface could certainly promote heterogeneous nucleation. The other factor to consider is that, in the deposition process, the organic impurities or precursors could be oxidized to lead to the formation of hydroxyl or carboxyl groups, which could cause the substrate surface more hydrophilic.28,29 Since the nucleation was determined by the nucleation barrier which was proportional to the surface area, when the surface became hydrophilic, the surface area decreased, resulting in the decrease of nucleation barrier. In this case, the heterogeneous nucleation was also much faster than homogeneous nucleation.
It may be the heterogeneous nucleation that governed the formation of flower-like grains and their further growth leading to a rough surface. Direct evidence comes from the observation of the formation of a heterogeneous and uneven surface structure at a thickness of as low as 100 nm (Fig. 5a). As the film thickness increased to 500 nm, such a surface structure tended to diminish, resulting in an even surface (Fig. 3g and 5c). Apparently, because the heterogeneous structure and flower-like grains formed at the early stage of film growth, a rough surface developed when the thickness of the film was still very thin in the present deposition. In contrast, in most previous studies, high roughness resulted from grain growth and thus was usually seen on the surfaces of very thick films.
The present film with a rough surface had a low resistivity. This may be related to the development of (200) preferred orientation during the process of film growth with the addition of HNO3 of up to 1.5 mL min−1 (Fig. 2). A clear beneficial effect of (200) preferred orientation on conductivity was also observed in some previous studies.8,15,30–33 The origin of preferred orientations can be explained by the periodic band chains (PBC) theory.23,34 According to this theory, the different faces of SnO2 can be classified into flat (F), stepped (S) and kinked (K) faces. For cassiterite SnO2, F{101} and K{110} faces are of great interest. F{101} and K{110} faces are polar, which consist of only tin atoms or oxygen atoms, while F{110} faces are less polar because they are comprised of both tin and oxygen atoms. For F{101} faces, there are two possible preferred orientations, namely, (110) and (001). Since the (001) orientation was not observed by XRD, the (110) preferred orientation formed by the crystalline pyramidal F(101)-faces. This may explain the major (110) preferred orientation observed in the baseline sample (Fig. 2).
Under the condition with inclusion of HNO3, F-faces having formed in the early stage may continue to grow, leading to prominent (200) growth perhaps for the following reason. HNO3 molecules have strong polarity, and could adsorb on polar F(101) planes. This could restrain the (110) plane growth, but give rise to the (200) plane growth, leading to the SnO2 crystals faceted exclusively by K faces with (200) preferred orientation, as previously reported for the favorable effect of the presence of halogen-rich gases on the development of (200) preferred orientation.8,31–33 But, with the addition of HNO3, the concentration of tin per unit volume was decreased, which was unfavorable for (200) growth which requires a high tin concentration.30 So excess HNO3 addition would slow down (200) plane growth, and benefit the growth of other planes. In addition, (211) plane also became the preferred orientation as the addition of HNO3 increased. The higher density of (211) direction was thought to be characterized by low growth rates and believed to be favoured during initial thin film formation.35 With HNO3 increasing, the concentration of precursors per unit volume decreased, which would lead to the decrease of growth rate. So (211) plane became the preferred orientation gradually.
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