Light Scattering and Current Enhancement for Microcrystalline Silicon Thin-Film Solar Cells on Aluminium-Induced Texture Glass Superstrates with Double Texture

Yin, Yunfeng; Sahraei, Nasim; Venkataraj, Selvaraj; Calnan, Sonya; Ring, Sven; Stannowski, Bernd; Schlatmann, Rutger; Aberle, Armin G.; Stangl, Rolf

doi:https://doi.org/10.1155/2015/358276

International Journal of Photoenergy

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Thin-Film Photovoltaics 2014

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Research Article | Open Access

Volume 2015 | Article ID 358276 | https://doi.org/10.1155/2015/358276

Light Scattering and Current Enhancement for Microcrystalline Silicon Thin-Film Solar Cells on Aluminium-Induced Texture Glass Superstrates with Double Texture

Yunfeng Yin,^1,2Nasim Sahraei,^1,2Selvaraj Venkataraj,¹Sonya Calnan,³Sven Ring,³Bernd Stannowski,³Rutger Schlatmann,³Armin G. Aberle,^1,2and Rolf Stangl¹

Academic Editor: Francesco Bonaccorso

Received26 Oct 2014

Accepted23 Dec 2014

Published08 Jun 2015

Abstract

Microcrystalline silicon (μc-Si:H) thin-film solar cells are processed on glass superstrates having both micro- and nanoscale surface textures. The microscale texture is realised at the glass surface, using the aluminium-induced texturing (AIT) method, which is an industrially feasible process enabling a wide range of surface feature sizes (i.e., 700 nm–3 μm) of the textured glass. The nanoscale texture is made by conventional acid etching of the sputter-deposited transparent conductive oxide (TCO). The influence of the resulting “double texture” on the optical scattering is investigated by means of atomic force microscopy (AFM) (studying the surface topology), haze measurements (studying scattering into air), and short-circuit current enhancement measurements (studying scattering into silicon). A predicted enhanced optical scattering efficiency is experimentally proven by a short-circuit current enhancement of up to 1.6 mA/cm² (7.7% relative increase) compared to solar cells fabricated on a standard superstrate, that is, planar glass covered with nanotextured TCO. Enhancing the autocorrelation length (or feature size) of the AIT superstrates might have the large potential to improve the μc-Si:H thin-film solar cell efficiency, by reducing the shunting probability of the device while maintaining a high optical scattering performance.

1. Introduction

Silicon thin-film solar cells are of industrial interest due to the fact that (1) the (hydrogenated) silicon layers are obtained directly from the gas phase (thus avoiding expensive crystallisation technologies and material consuming sawing technologies) and (2) the solar module production process can be directly integrated into the cell production process (“monolithic integration”). Hydrogenated microcrystalline silicon (μc-Si:H), a mixed-phase material containing both amorphous and crystalline silicon regions, is widely used as a material forming the bottom cell of tandem or multijunction thin-film solar cells [1, 2]. In order to reduce manufacturing cost and excess carrier recombination, the μc-Si:H absorber layer should be as thin as possible. However, due to the material’s finite absorption coefficient, it is difficult to generate a sufficiently high photogeneration rate within the μc-Si:H film for a single pass of the light through the film. Therefore, light scattering technologies have to be used to enhance the effective light path within the film [3–5]. With the help of light trapping methods, photogenerated currents of above 30 mA/cm² can be generated, using around 3 μm thick μc-Si:H films, and very high PV efficiency has been reported [6–8]. The conventional thin-film light trapping is achieved by either etching the front transparent conductive oxide (TCO) layer of the solar cell prior to the μc-Si:H deposition or growing the TCO layer with a self-organized surface texture [9]. This usually creates a nanotextured surface, with typical feature sizes ranging from several tens of nanometres to several hundred nanometres [3, 9, 10]. This surface texture generally provides good light trapping properties for wavelengths up to 650 nm, but the ability to scatter near-infrared light from 700 to 1100 nm is quite modest. To overcome this problem, surface textures with a larger feature size are needed [11]. Photolithography was used to create periodic honeycomb patterns with microscale size, and a significant improvement of near-infrared light absorption was shown for substrate-type n-i-p μc-Si:H thin-film solar cells [7, 12]. For superstrate-type p-i-n μc-Si:H thin-film solar cells, texturing of the glass superstrate (leading to a microtextured glass surface) has been proposed recently, that is, using imprint-textured glass [11], rough glass by 3D texture transfer by ion etching [13], or aluminium-induced texture (AIT) glass [14–16] in order to enhance light trapping. Besides, double-textured TCO, for example, using HCl and HF wet etching leading to microscale and nanoscale surface textures, respectively, was also proposed and demonstrated to improve the light trapping ability for the silicon thin-film solar cells [17, 18]. In the present study, we use a double texture, that is, aluminium-induced texture glass superstrates (microtexture) covered with etched TCO (nanotexture), and compare its light trapping ability to a standard single-textured reference superstrate (i.e., planar glass covered with etched TCO). The AIT method enables us to obtain an industrially feasible microtextured glass surface with typical feature sizes in the 1–3 μm range (“AIT glass”). It has already been theoretically proven, using numerical computer simulation, that a double-textured superstrate has an excellent light scattering potential for the entire wavelength range from 300 to 1100 nm because of the superimposed scattering behaviour [19]. Experimentally, a double-textured superstrate was investigated, using ion-etched textured glass in combination with a self-organised textured (MOCVD made) TCO growth, proving a short-circuit current enhancement of 1.5 mA/cm² compared to the planar glass/textured TCO reference superstrate [20]. Using AIT glass covered with etched TCO (double texture), we so far only investigated scattering into air (i.e., haze and angular resolved scattering), thereby highlighting the potential of a large enhancement using a double texture [16]. However, on a device level, this has not yet been proven. This demonstration is the scope of this paper.

In order to investigate the benefit of a double texture (i.e., the benefit of AIT glass when using TCO etching for light trapping), three different superstrates are used (see Figure 1): (1) planar glass covered with textured TCO (“single-textured” reference superstrate, REF), (2) AIT glass exhibiting a moderate correlation length covered with textured TCO, and (3) AIT glass exhibiting a large correlation length covered with TCO (i.e., two different “double-textured” AIT glass superstrates, AIT-1 and AIT-2). The surface morphologies of these superstrates are studied by means of atomic force microscopy (AFM) and subsequent image processing. Thin-film μc-Si:H solar cells are processed on these textured superstrates and the resulting short-circuit currents are investigated using current-voltage as well as external quantum efficiency (EQE) measurements, in order to determine the optical scattering enhancement into silicon, if a double-textured superstrate is used. Furthermore, the influence of different AIT glass morphologies on the and on the solar cell efficiency, compared to the single-textured reference superstrate, is discussed.

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(b)

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2. Experimental Details

Three pieces of 10 × 10 cm² soda lime glass sheets (3 mm thick) were used. Two of them were textured on one surface with the AIT method [14–16, 21], and the remaining one was not textured (reference). By changing the Al thickness, reaction time, and etching time, the surface morphology and the corresponding haze values of AIT glass sheets can be well controlled; see [16] for a detailed study. The surface morphology and visible light haze values were measured using an atomic force microscope (Veeco, model DI-3100 Nanoman) and a digital hazemeter (BYK haze guard, model AT-4725, light source: tungsten lamp). The spectrally resolved haze values (ranging from 400 to 1200 nm) were measured by UV-VIS spectroscopy (Perkin-Elmer, Lambda 950). All three glass sheets (planar and textured) were cleaned with DI water and then coated with an aluminium-doped zinc oxide film (ZnO:Al or “AZO”), using DC magnetron sputtering from a ceramic ZnO:Al₂O₃ tube target. Next, the AZO films were etched in a highly diluted HCl solution, leading to a nanoscale surface texture on the AZO films. Thus, one single-textured reference superstrate (planar glass covered with nanotextured TCO) and two double-textured AIT superstrates (microtextured glass covered with nanotextured TCO) were processed [16]. All glass sheets were then cut into two parts. Half of them were used as superstrates for thin-film solar cell fabrication, while half were used for surface morphology characterisation. For solar cell fabrication, the AZO coated glass sheets were cut into 5 × 5 cm² pieces. They were then attached to a 30 × 30 cm² stainless steel sample holder and loaded into a conventional RF (13.56 MHz) PECVD system (Applied Materials, AKT 1600) for silicon thin-film deposition. Doped μc-:H films, doped with either boron or phosphorus, were used as p-type or n-type hole/electron collecting layers of the p-i-n thin-film solar cells, with a target thickness in the range of 20–30 nm for the reference superstrate. The intrinsic μc-Si:H absorber layer (target thickness of 1.75 μm for the reference superstrate) was deposited at a temperature of 190°C. It is emphasised that the resulting absorber layer thickness for the AIT glass superstrates is significantly lower (~1.5 μm), despite the fact that the same deposition run was used. This large thickness difference indicates a strong influence of the surface morphology on the thin-film deposition by PECVD, as, for example, highlighted in [22]. Next, a thin AZO film (~80 nm) combined with a 150 nm thick silver layer was deposited onto the thin-film silicon diode, serving as back surface reflector and rear contact of the solar cell. Finally, laser patterning was applied to define isolated cells with an area of 1.0 × 1.0 cm². The - characteristics of the cells were measured under standard test conditions (AM1.5G spectrum, cell temperature 25°C), using a class AAA dual-light-source solar simulator (Wacom, WXS_156S_L2). Cross-sectional images of the solar cells were taken by field emission transmission electron microscopy (XTEM, JEOL-JEM, 2010F) to determine their thickness.

3. Results and Discussion

3.1. Surface Morphology and Haze of the Superstrates

The three different superstrates mentioned above were investigated by AFM. From the 20 × 20 μm² AFM images as shown in Figure 1, surface morphology information such as mean surface roughness, surface angle distribution, and autocorrelation length were extracted (see Table 1) using the methods described in [23]. As compared to the reference superstrate (planar glass coated with nanotextured TCO), the AIT glass superstrates (microtextured glass coated with nanotextured TCO) show quite different characteristics. As expected, the AIT samples have much higher surface roughness (RMS) than the reference sample (about 200 nm versus 36 nm). Also the mean feature size of the textured superstrates (i.e., the autocorrelation length , which is a good indicator for the mean lateral feature size of randomly textured surfaces and which can be obtained from the autocorrelation function which can be extracted from AFM image data processing [23]; see Figure 2) differs considerably: for the reference superstrate the autocorrelation length is as small as 150 nm, whereas the AIT-1 superstrate has a moderate autocorrelation length of about 750 nm and the AIT-2 superstrate has a large autocorrelation length of about 1050 nm; see Table 1. The autocorrelation function is an indicator of spatial persistency (or similarity) of the surface structure to itself at two positions of the surface. The distance between these two points is called lag length [24]. Assuming that the autocorrelation function can be presented by an exponential function, the autocorrelation length is defined as the lag length for which the autocorrelation function equals (0.3678); see Figure 2. As expected from the AFM images of the superstrates in Figure 1, the autocorrelation length (the mean feature size) of the reference superstrate is much smaller than that of the AIT samples.

Surface angle distributions were extracted from the AFM images, as described in [23], specifying the probability of encountering a specific surface angle between 0 degrees (flat surface) and 90 degrees (surface perpendicular to the substrate plane); see Figure 3. Interestingly, AIT-1 and AIT-2 have similar surface angle distributions; see Figure 3. Both superstrates exhibit an average surface angle of 40 degrees, with a pronounced maximum at 30 and 50 degrees, respectively. Based on the extracted surface morphology data, a simplified surface morphology model describing the three different superstrates is proposed; see Figure 4. Referring to this simplified surface morphology model, the reference superstrate is nanotextured with an autocorrelation length (mean self-repeating feature size) of 150 nm and an average surface angle about 20 degrees due to the texture. The AIT glass superstrates are double-textured (microtextured glass and nanotextured TCO). They have an autocorrelation length (mean self-repeating feature size) of 742 μm or 1050 μm, respectively, an average surface angle of 40 degrees due to the microstructured glass, and an additional average surface angle of ±10 degrees due to the superimposed nanotexture stemming from the etched TCO. Thus, the average surface angle in the nanotextured surface valleys (“kinks”) of the double-textured AIT glass superstrates is either 30 or 50 degrees; see Figure 4. Furthermore, the number of “kinks” as well as the surface roughness should correlate with the autocorrelation length of the AIT glass superstrates (i.e., fewer “kinks” and higher surface roughness for AIT superstrates with higher autocorrelation length ).

“Kinks” are often found to be the sources of microcracks and thus also sources for recombination active regions within microcrystalline silicon solar cells [25]. They can also be sources for local shunt formation [26]. The schematic model clearly reveals that, within a certain area, the AIT-1 superstrate (with moderate correlation length ) has a much higher density of “kinks” than the AIT-2 superstrate (with large correlation length ). This means that AIT glass superstrates with a larger autocorrelation length have a lower shunting probability for the fabricated μc-Si:H thin-film solar cells. The AIT-2 superstrate should therefore be less affected by local shunting, if used as a superstrate for μc-Si:H solar cell processing.

Haze measurements (diffuse scattering into air) for visible light (400–700 nm) were performed on the 3 superstrates, both before and after the application of the nanotextured TCO. Without TCO, the reference superstrate (planar bare glass) shows no haze at all, while the haze values of the two AIT superstrates vary significantly (50% for AIT-1 and 70% for AIT-2). After the application of nanotextured TCO, the haze values of the two AIT glass superstrates differ much less (65% versus 74%), despite the fact that the autocorrelation length of the two samples is significantly different (742 versus 1050 nm). Compared to the haze of the reference superstrate (12%), the haze of the AIT superstrates is much higher. Table 1 compiles the measured haze and surface morphology parameters of the three investigated superstrates.

Furthermore, the spectrally resolved haze was measured; see Figure 5. Considering μc-Si:H thin-film solar cells, the light scattering ability in the long-wavelength region (700–1100 nm) is most important. As can be seen in Figure 5, the haze values of the double-textured AIT superstrates improve significantly in the long-wavelength region (compared to the single-textured reference superstrate). Therefore a stronger scattering of long-wavelength photons and thus a higher short-circuit current enhancement after μc-Si:H thin-film solar cell processing can be expected for the AIT superstrates. Furthermore, it is expected that the AIT-2 superstrate will give a higher than the AIT-1 superstrate.

3.2. Microcrystalline Silicon Thin-Film Solar Cells Grown on the Different Superstrates Used

Several 1 cm² μc-Si:H thin-film solar cells were processed on the different superstrates discussed in the previous section. It is well known that the growth of μc-Si:H is surface morphology dependent [26, 27]. As expected, the growth behaviour of μc-Si:H was considerably different when deposited on the double-textured AIT glass superstrates (microtextured glass covered with nanotextured TCO) compared to depositing on the single-textured reference superstrate (planar glass covered with nanotextured TCO), that is, the resulting film thickness differs significantly. The μc-Si:H layers deposited onto AIT glass superstrates are thinner (1.4–1.5 μm) compared to the layers deposited on the single-textured reference superstrate (1.7 μm), keeping the deposition time constant (i.e., using the same deposition process); see Figure 6. This difference can be attributed to the fact that the AIT superstrates have a larger surface area (around 13%) than the reference superstrate, stemming from the larger average surface angle of the microstructured AIT glass. Furthermore, the effects of shadowing and reemission should also be taken into consideration when depositing the films onto highly textured substrates [28].

(a)

(b)

Figure 7 and Table 2 show the corresponding one-sun - curves and the extracted solar cell parameters of the best μc-Si:H solar cells obtained on the three investigated superstrates. As expected, processing on double-textured AIT superstrates does improve the light scattering within the solar cell: a significant increase of 1.2 and 1.6 mA/cm² (5.8% and 7.7% relative) was observed for the AIT-1 and AIT-2 superstrates, respectively, compared to processing on the single-textured reference superstrate. Please note that the absolute short-circuit current density obtained for all solar cells is quite low (~21 mA cm⁻²) compared to the current state of the art (up to 30 mA cm⁻²). This is due to three facts: (1) the processed μc-Si:H deposition used was optimized for micromorph tandem (a-Si:H/μc-Si:H) solar cell applications but not for single-junction μc-Si:H solar cells like those investigated in this study, (2) a comparatively thin μc-Si:H absorber layer thickness (1.4–1.5 μm) was used, compared to a 3 μm absorber thickness used in demonstrating an above 30 mA cm⁻² [6, 7], and (3) an industrial feasible 3 mm thick soda lime glass was used instead of, for example, a 1 mm thin Corning glass. As expected, the current enhancement is mainly ascribed to the better light absorption for the infrared light (700–1100 nm) (see the EQE curves in Figure 8) since the haze values in the long-wavelength region improved significantly by using AIT glass superstrates, as shown in Figure 5. Furthermore, given the fact that the μc-Si:H film thickness on the AIT glass superstrates is thinner than on the reference superstrate, an even higher increase can be expected if the film thickness is tuned to be identical. As expected, the AIT glass superstrate with the larger autocorrelation length (AIT-2) shows a higher increase (compared to AIT-1).

Thus, analysing only the measured using AIT glass superstrates clearly enhances the light scattering ability into silicon. However, analysing the resulting - curves, so far, all cells processed (even including the cells processed on the reference superstrate REF) do suffer from significant shunting. As expected, this shunting issue is much more severe with processing on AIT glass superstrates. Thus a shunt-induced steep slope in the - curves towards low voltages is observed (for all three superstrates), and in case of the AIT superstrates the low shunt resistance even affects the open-circuit voltage (and also the measured short-circuit current) of the solar cells; see Figure 7 and Table 2. In case of no shunting, the short-circuit current enhancement of the AIT superstrate would be even higher than reported. Again, in agreement with our expectations outlined above, the AIT superstrate with the larger autocorrelation length (AIT-2) does suffer less from shunting compared to AIT-1. Indeed, defective areas (“cracks”) were observed when depositing μc-Si:H films on AIT glass superstrates, that is, above deep valleys (“kinks”) which are induced by the AIT glass, as shown in Figure 9.

Further optimisation still needs to be done, that is, (1) extending the autocorrelation length of AIT samples as much as possible, thus experimentally determining the maximum due to the use of AIT superstrates and simultaneously reducing the shunting probability and (2) depositing different μc-Si:H thin-films on the microtextured AIT superstrates, which are better adapted to grow shunt-free on a microstructured texture, that is, using lower-crystallinity films. Generally, μc-Si:H films with crystallinity of 50–60% are considered to be the best suited material for μc-Si:H solar cells [29], when deposited on conventional superstrates (i.e., suitable for our reference superstrate, planar glass covered with nanotextured TCO). However, when deposited onto highly textured substrates (i.e., on AIT glass), it is proposed to use lower-crystallinity films (40–50%, with slightly poorer absorption of infrared wavelengths) or buffer layers [30]. Thus, it can be expected that by optimising the deposition conditions of μc-Si:H films on AIT glass superstrates, as well as the AIT process itself, it should be possible to significantly reduce, or even eliminate, the local shunting problems experienced in our present experiments.

Based on the above analysis, μc-Si:H thin-film solar cells processed on AIT superstrates show a large potential to improve the solar cell efficiency, since (1) the improved light trapping (a higher short-circuit current density compared to a standard reference superstrate) has been experimentally proven and (2) a reduction/elimination of the presently observed local shunt formation seems possible.

4. Conclusions

Microcrystalline silicon (μc-Si:H) thin-film solar cells were processed on aluminium-induced texture (AIT) glass superstrates. The influence of the surface topology on the optical scattering behaviour and on the μc-Si:H film growth was investigated, by using a conventional single-textured reference superstrate (planar glass with nanotextured TCO) and two differently double-textured AIT glass superstrates (microtextured AIT glass covered with nanotextured TCO, exhibiting a moderate or large autocorrelation length, resp.). Surface topology information, such as surface roughness, surface angle distribution, and autocorrelation length (indicating the mean surface feature size), was extracted from AFM images. Scattering was investigated via haze measurements (scattering into air) and via the measured short-circuit current enhancement compared to the reference superstrate (scattering enhancement into the silicon). A significant haze increase was observed when using AIT superstrates, resulting in a short-circuit current enhancement of 1.6 mA/cm² (7.7% relative increase). However, local shunt formation also emerged. A decreasing shunting probability was observed to correlate with an increasing autocorrelation length of the AIT superstrate. The experimental results predict that a further enhancement of the autocorrelation length (mean feature size) of the AIT superstrates shows a large potential for improving the solar cell efficiency, by reducing the shunting probability while maintaining (or even increasing) the light scattering abilities. Thus after optimization of the μc-Si:H thin-film deposition process on highly textured surfaces, the use of double-textured AIT glass superstrates has a large potential for improving the efficiency of μc-Si:H thin-film solar cells.

Conflict of Interests

The authors declare that there is no conflict of interests regarding the publication of this paper.

Acknowledgments

The Solar Energy Research Institute of Singapore (SERIS) is sponsored by the National University of Singapore (NUS) and Singapore’s National Research Foundation (NRF) through Singapore Economic Development Board (EDB). This work was partly supported by the PVcomB (Helmholtz-Zentrum Berlin), Germany.

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Copyright © 2015 Yunfeng Yin et al. This is an open access article distributed under the Creative Commons Attribution License, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.

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