Abstract

Bifacial solar cell is a specially designed solar cell for the production of electricity from both sides of the solar cell. It is an active field of research to make photovoltaics (PV) more competitive by increasing its efficiency and lowering its costs. We developed an n+pp+ structure for the bifacial solar cell. The fabrication used phosphorus-oxy-trichloride (POCl3) diffusion to form the emitter and Al diffusion using conventional screen printing to produce the back surface field (BSF). The n+pp+ bifacial solar cell was a sandwiched structure of antireflective coatings on both sides, Argentum (Ag) as a front contact and Argentum/Aluminum (Ag/Al) as a back contact. This paper reports the solar cell performance with different surface passivation or antireflecting coatings (ARC). Silicon nitride (SiN) deposited by Plasma-Enhanced Chemical Vapor Deposition (PECVD), thermally grown silicon dioxide (SiO2), PECVD-SiO2, and SiO2/SiN stack were used as ARC. The efficiency obtained for the best bifacial solar cell having SiN as the ARC is 8.32% for front surface illumination and 3.21% for back surface illumination.

1. Introduction

Bifacial solar cell is a specially designed solar cell for the production of electricity from both sides of the solar cell. In bifacial solar cell allowance has to be made to allow absorption of light entering from the front and back sides. Since under ordinary circumstances the junction is located close to the front side, for rear illumination quantum efficiency is mostly realized from long wavelength. Thus, passivation and reflective indices of the rear side are important to the performance of the bifacial solar cell.

Cueves [1] reported that H. Mori 1966 developed the first bifacial solar cell by introducing a collecting p-n junction on both sides of a silicon wafer. In order to compensate for the short minority carrier lifetime, Mori placed a second pn-junction closed to the rear surface. This improved the collection efficiency for long-wavelength photons. However, the need for a third metal contact makes such devices cumbersome. In 1972, Mandelkorn and Lamneck reported a bifacial solar cell with a homopolar pp+ or nn+ junction on the opposite surface of heteropolar pn junction [1]. The structure was known as bifacial Back Surface Field (BSF) cells. The origins of the original bifacial solar cell may be attributed to the drift field at the heavily doped rear surface which reduces recombination and improves open-circuit voltage (𝑉oc). Variations of bifacial BSF such as n+pp+ [24], p+nn+ [2, 5], p+np+ [6], n+np+ [7], and n+pn+ [8] have all been reported.

The research on bifacial solar cell has since expanded by other researchers using wide range of device configurations in order to achieve higher efficiency. These include triode and Rear-Floating Emitter (RFE) [9], passivated emitter rear type (PERT) [3], and double-sided buried contact (DSBC) structures [10]. Methods that have been used in fabrication of bifacial solar cells include lithography [8], plasma-enhanced chemical vapor deposition (PECVD) [4, 11], screen-printed aluminum emitter [7], screen-printed boron and phosphorus pastes [12], spin on emitter [5], and boron and phosphorus gas diffusion [13]. Other than the use of thinner wafers, bifacial solar cells have other advantages including superior high temperature performance, lower metal usage, and enhanced power generation. A large number of bifacial solar cell improvements were made through surface texturing [8], buried contact [13], laser grooving [14], and electroplating [15].

The illumination received by bifacial solar cell is increased from the single facial solar cell of the same dimension. Optimum device processing should make bifacial solar cell competitive to single-sided solar cell in terms of performance. Also, using thinner wafer helps decrease the cost of bifacial solar cell.

In this study, we design a bifacial solar cell with a simple fabrication process. We have modified our single facial solar cell design by incorporating aluminum firing and passivation on the rear side. In this way, we have included a p++ layer. We expect the extra heavy doping at the rear contact of the bifacial solar cell will keep the electron away from the high recombination region. Besides, we develop an alternative technique to remove fired Al paste. Common techniques to remove aluminum are potassium bath [7] or nitric and fluoric acid dipping [8]. The effectiveness of passivation and antireflection coatings of SiN, SiO2, and SiN/SiO2 stacks are accessed.

2. Materials and Methods

Bifacial solar cells with a configuration of n+pp+ with Aluminium Back Surface Field (Al-BSF) were designed. The cell has screen-printed front surface Ag and back surface Ag/Al contacts. Figure 1 is a schematic of the basic cell structure.

P-type <100> Si wafers with resistivity ranging between 1 ohm-cm and 10 ohm-cm (with a doping density between 1015 and 1016) were used. The Si wafer was initially cleaned by dipping into solution of hydrofluoric acid (HF) and nitric acid (HNO3) in a ratio of 1 : 100 for 10 minutes. After rinsing with deionized water, it was then dipped into HF and water (H2O) in a ratio of 1 : 50 for 1 minute. The wafer was then immersed in 10% potassium hydroxide (KOH) at a temperature of 70°C for 5 minutes. Subsequently, the wafer was repeatedly cleaned in HF : H2O. The texturing process followed the cleaning procedure. The wafers were textured using a solution of KOH, isopropyl alcohol (IPA), and water (H2O). After the texturing process, the wafers were subjected to the n-type diffusion using gas-source phosphorous oxychloride (POCl3) at a temperature of 908°C. The edges of the Si wafers were then mechanically diced to achieve edge isolation.

For bifacial solar cells with Al-BSF, Al pastes were screen-printed onto the back side of the Si wafer. The paste was annealed at 150°C for 10 minutes prior to firing at a temperature of 830°C in a rapid thermal annealing (RTA) furnace to form Al-diffused p+ layer. Excess Al was removed by soaking in 100% hydrochloric acid (HCl) solution. In this way the n+pp+ structure was successfully fabricated.

We investigated three antireflection coating (ARC) and passivation structures. These are given in Figures 2(a), 2(b), and 2(c). For bifacial solar cell A, the thermally grown silicon dioxide (SiO2) that was formed after the diffusion process was maintained on both sides as passivation and ARC, while, for cell B, we removed the thermal oxide with Buffer Etch Oxide (BEO), after which we deposited the Silicon Nitride (SiN) on both sides using PECVD at a temperature of 150°C. For cell C, we performed the SiO2/SiN stack process on the front and back sides. Besides the thermally grown SiO2, we also carried out a low-temperature SiO2 deposition using PECVD. We used a combination of silane and nitrous gas to obtain the PECVD-SiO2 thin film.

Finally, the metallization processes were carried out using screen printing of Ag and Ag/Al pastes by employing identical grid masks on the front and back surfaces, respectively. Screen-printed contacts were fired at ~830°C to form front and back contacts.

The finished solar cells were experimentally analyzed by Light Current-Voltage (LIV) and Quantum Efficiency measurement systems using Keithley 237 current source meter. The Surface photovoltage properties of the front side of the bifacial solar cell were also examined.

3. Results and Discussions

Passivated interface reflects minority carriers but allows majority carriers to pass. Also, both emitter and base passivating layer of a bifacial solar cell has to be transparent to light and has a wider bandgap than silicon. A back surface field (BSF) is usually formed at the back of a solar cell to reflect minority carriers from combining at the rear. One way to achieve this is by increasing the doping of the surface field layer. However, a BSF is ineffective if the rear surface defect states are not passivated. In the present bifacial solar cell the front (emitter side) and back (base side) passivations are carried out using thin layers of SiO2, SiN, and SiN/SiO2 stack. In addition a BSF of p+ region is also introduced at the back.

As mentioned above, SiN was deposited using PECVD and two depositions methods were used for SiO2: thermally grown SiO2 and PECVD-SiO2. For the front side, the film was deposited on the emitter layer. Overall, two thermal annealing processes were independently carried out at 830°C through rapid firing; the first is Al firing to form the BSF and the other is the firing to form the front and back contacts. The effect of thermal treatment is shown to be conducive to surface and bulk passivation [9].

Figure 3 shows the minority carrier lifetime spectra of deposited PECVD-SiN, thermally grown SiO2, PECVD-SiO2, and SiN/SiO2 stack on the emitter layer. The measurements were done under an operating voltage of 50 𝜇V. SPV measures the minority carriers (i.e., electrons for p-type silicon) collected on the surface of a thin film. From Figure 3, the respond amplitude for the ultraviolet region between 400 nm and 500 nm is seen to be small. Within these wavelengths, photons are absorbed in the emitter region. Electron in the emitter region is a majority carrier and for low-injection condition the Fermi level of the electron does not change much from the equilibrium position. Thus no photogenerated electron diffuses to the surface.

Between 500 nm and 700 nm photogenerated electrons that are produced in the junction and in the base close to the junction will diffuse to the surface. The quality of the passivation layer is measured by the increase in the number of electrons reaching the surface. The deposition induces passivation of silicon dangling bonds at the emitter surface and consequently the reduction of the interface state density that can trap electrons. Also, the existence of high positive fixed charge density at the surface causes a reduction in the majority hole carrier concentration at the surface by means of field-effect passivation. From Figure 3 it can be seen that SiN produces the best passivation followed by thermally grown SiO2, PECVD SiO2, and SiN/SiO2 stack in that order.

For wavelength greater than 700 nm the SPV respond amplitude decreases indicating less electrons reaching the surface. For absorption close to the back of the solar cell bulk recombination dominates if the diffusion length of the electrons is less than the thickness of the base.

It is informative to compare thermally grown SiO2 with PECVD-SiO2. In the visible-light range, both of them show similar performance, but they differ in the longer wavelength response. The thermally grown SiO2 has a faster decay rate in the wavelength 700–800 nm compared to PECVD-SiO2. The thermally grown process consists of the transportation of oxygen to the surface, diffusion of the oxygen through the already grown oxide, and finally the reaction of the oxygen with the silicon at the interface between silicon and silicon oxide. With growing oxide thickness, the growing rate slows down because the time of the diffusion through the oxide depends on its thickness. This process makes the degradation of thermally grown SiO2 faster than PECVD-SiO2.

Since thermally grown SiO2 and PECVD-SiO2 show similar response in the visible light, we decided to use only thermally grown SiO2. The simplicity of surface passivation process by using thermal oxide is an added value to silicon solar cell processing [16]. Besides that, the surface is well passivated with lightly diffused phosphorus layer together with high-quality thermal oxide. By eliminating the use of PECVD process to deposit SiO2 the cost of fabrication can be kept low.

Figure 4(a) shows SEM images of SiN with a magnification of 50,000. From the figure, we see that SiN is deposited on the pyramid textured of the Si wafer with a thickness of 53.78 nm. Figure 4(b) shows the cross-sectional image of Al on SiN film with a magnification of 1,000. This characterization is done to study the Energy Dispersive X-Ray (EDX) profile of Al after the firing process to validate the punching of Al through the SiN layer to obtain the p+ layer. From Table 1, we see that Al exists until Spectrum 4 of the profile. The deeper EDX spectrum shows less Al. Thus, Al is able to punch through the ARC and diffuses into the Si wafer to form highly doped region.

Figure 5 shows the reflectance measurement of the various ARCs on planar Si wafer. From the figure, we can conclude that all ARCs show low reflectance compared to planar wafer. The SiO2/SiN stack should show the lowest reflectance, but is actually higher than thermally grown SiO2 and PECVD-SiN due to nontextured surface. The combination of textured and ARC thin film should reduce reflection losses enhancing photon absorption.

For the bifacial solar cell the reflectivity does not differ much from the planar case shown in Figure 4. The reflectivity is derived from the IV measurement of the short-circuit current density and quantum efficiency measurement. These values are given in Table 2. The reflectivity ranges between 24% and 67%.

The percentage of photogeneration in solar cell can be determined by measuring the Quantum Efficiency (QE). Many factors affect the photogeneration. Figures 6(a) and 6(b) show the QE spectra for front and back illuminations of the bifacial solar cell having SiO2, SiN, and SiO2/SiN stack ARC layers.

As shown in Figures 6(a) and 6(b) generally photogeneration decreases with increasing wavelength for both front and back illuminations. Also for front illumination the number of carriers generated is far less than one except for region in the lower part of the wavelength. Factors such as low absorption, high reflectivity of ARC, low field factor, high saturation current density, ineffective back surface field, and high bulk recombination all contribute to the degradation of the quantum efficiency. For front illumination the QE of SiO2 and SiN ARCs are about the same. For stack ARC the QE is lower.

For back illumination the QE for SiN ARC solar cell is better although for low wavelength the QE of stack ARC is higher than SiN. QE of SiO2 is the lowest. Thus, from the QE curve we have generated the photocurrent and this is given in Table 2. Together with the 𝐽sc obtained from the IV results reported below, the reflectivity was deduced. It is shown that the SiO2 and SiN ARCs for front illumination show low reflectivity.

We now report the results of the current-voltage (𝐼-𝑉) measurement of bifacial solar cells A, B, and C. Figure 7 shows the 𝐼-𝑉 curve of these solar cells for (a) front and (b) rear side illuminations. For front side illumination, the 𝑉oc values are 0.492 V for solar cells A and B while for solar cell C it is 0.468 V. The short-circuit current densities (𝐽sc) for front side illumination are 26.75 mA/cm2, 28.25 mA/cm2, and 26.50 mA/cm2 for solar cells A, B, and C, respectively. For rear side illumination, the 𝑉oc for solar cell A remains at 0.492 V, but for solar cells B and C, the 𝑉oc are 0.468 V and 0.444 V, respectively. Device A with thermally grown SiO2 on both sides shows poor 𝐽sc of 13.25 mA/cm2 and is half the value of the front side. The SiN (solar cell B) and SiO2/SiN stacks (solar cell C) produce 𝐽sc of 20.25 mA/cm2, and 21.0 mA/cm2, respectively.

The values of 𝐽sc,𝑉oc, and FF for front and back illuminations of the bifacial solar cells are shown in Table 3. Also given are the values of the saturation current density 𝐽𝑜 calculated using the formula 𝐽lnsc𝐽𝑜=𝑞𝑉oc𝑘𝑇1,(1) where 𝑘 is the Boltzmann’s constant, 𝑞 is the electronic charge, and 𝑇 is the absolute temperature in Kelvin.

The substandard performance of the bifacial solar cell is attributed to many factors. One of the factors is the poor quality of ARC layers, thus giving rise to high reflectivity in particular for back illumination. This is clearly noticeable in the QE spectra. The effect related to the reflective indices of the ARC layer will have to be investigated further. The other factor is insufficient passivation. The saturation current density 𝐽𝑜 is of the order of 1010 A/cm2 which is higher compared to an optimum value of 1014 A/cm2. Besides that, the low fill factor due to ohmic losses as a result of a low conductivity of top semiconductor contributes the low efficiency of bifacial solar cell. Therefore, photogenerated carriers need to travel large lateral distances before being collected. The effect is manifested in high series resistance.

The 𝑉oc is also low as compared to the best 𝑉oc that can be obtained with good quality silicon solar cell, which is about 0.7 V. This is attributed to ineffective back surface field and also poor passivation. Meanwhile, the low value of 𝐽sc is attributed to poor passivation quality of the ARC layers. The high recombination velocity of minority carriers reduces 𝐽sc. The 𝐽sc values are about half that can be achieved from the best solar cell which is about 43 mA/cm2. From the results given in Table 3, thermally grown SiO2 and SiN produce about the same passivation quality compared to SiO2/SiN stack. It is expected that the performance of the bifacial solar cell can be improved by varying the processing conditions such as the method of removing the fired Al to form the BSF.

4. Conclusion

Bifacial solar cells performance with different surface passivations was investigated. The best passivation scheme for antireflection coating (ARC) was thermally grown SiO2 and SiN since they show similar results. The front side of the bifacial solar cells produced better performance compared to the back side. For future research, we will develop a dry process to deposit a p+ layer using boron solid source. We will also investigate the use of indium tin oxide (ITO) or silicon carbide (SiC) as ARC layers on both sides of the bifacial cells.

Acknowledgments

This work has been carried out with the support of the Malaysia Ministry of Science, Technology and Innovation (MOSTI) and Ministry of Higher Education (MoHE) under the TechnoFund and Fundamental Research Grant Scheme.