High Fill Factors of Si Solar Cells Achieved by Using an Inverse Connection Between MOS and PN Junctions
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Fill factors (FFs) of ~0.87 have been obtained for crystalline Si (c-Si) solar cells based on Ag front contacts after rapid thermal annealing. The usual single PN junction model fails to explain the high FF result. A metal/oxide/semiconductor (MOS) junction at the emitter is found to be inversely connected to the PN one, and when its barrier height/e is close to the open-circuit voltage of the solar cell, very high FF is obtainable. In this work, although the open-circuit voltage (<580 mV) is not high here, the efficiency of c-Si solar cell still reaches the state-of-the-art value (>20 %) due to the high FF achieved.
KeywordsSi solar cell Fill factor Ag contact MOS barrier
External quantum efficiency
Dark current density
Short-circuit current density
The ideal factor of the PN junction
Ideal factor of the MOS junction
Rapid thermal annealing
Shanghai Advanced Research Institute
Scanning electron microscope
Shanghai Institute of Technical Physics
The barrier height
Photoelectric conversion efficiency (η) of solar cell is determined by the product of open-circuit voltage (V OC), short-circuit current density (J SC), and fill factor (FF); therefore, achieving high V OC and J SC as well as FF is crucial for getting high η [1, 2]. Considering the large abundance of Si on the earth’s crust and the hyper amount of investment input in the Si solar cell industry, new approaches to enhance V OC, J SC, and/or FF for further increasing Si solar cell efficiency are always in demand. To our knowledge, FFs for the mostly efficient single crystalline- or c-Si solar cells reported so far are basically no larger than 0.835, for instance, for the PERL-type Si solar cell, FF = 0.828 (V OC = 706 mV, J SC = 42.7 mA/cm2, η = 25.0 %) , for the IBC-type Si solar cell, FF = 0.830 (V OC = 730 mV, J SC = 41.2 mA/cm2, η = 25.0 %) , for the HIT-type Si solar cell, FF = 0.835 (V OC = 738 mV, J SC = 40.8 mA/cm2, η = 25.1 %) , and for the HIT + IBC type Si solar cell, FF = 0.827 (V OC = 740 mV, J SC = 41.8 mA/cm2, η = 25.6 %) . This work reports our finding of high FF (~0.87) and analyses of its origin based on an inverse connection of metal/oxide /semiconductor (Ag/SiO2/Si) or MOS and PN junctions.
The substrate of the Si solar cell is P-type c-Si < 100 > wafer (two-sided polish, 10 × 10 × 0.2 mm3 in size, 1–5 Ω · cm). First, the Si wafer was degreased and ultrasonically cleaned and then dipped in diluted HF (1 %). Then, it was placed in the boiling NaOH solution with concentration of 1 g/L at 90 °C for 30 min and rinsed in deionized water and blown dry to texture the surface for antireflection. A phosphorous paste was deposited on the front surface of Si, followed by annealing the wafer at temperature of 900 °C for 20 min in a tube furnace in nitrogen with purity of 99.999 % to form PN junction. A 60-nm-thick SiO2 was evaporated by means of electron beam heating onto the top surface of now N+ Si emitter for surface passivation  in a home-made vacuum chamber with a base pressure less than 1 × 10−4 Pa. At the rear of the substrate, a 20-nm-thick Al2O3 was evaporated also by means of electron beam heating for rear passivation . A 1.0-μm-thick Ag grid was then deposited onto the SiO2 passivation layer as the front contact by resistance heating in another home-made vacuum chamber with a base pressure less than 5 × 10−3 Pa. A 1.0-μm-thick Al layer was deposited onto the Al2O3 passivation layer as the rear contact by resistance heating in the same system. Finally, the whole device was annealed in nitrogen atmosphere at 510 °C for 2 min followed by rapid thermal annealing (RTA) at 700 °C for 1 s. For RTA, we firstly pushed the sample from one end of the furnace tube to its middle within 3 s. The variation of temperature was from room temperature to 700 °C. Then, the sample was kept in the middle of the tube for 1 s, followed by being pulled out from the middle to the end of the tube within 3 s. All the processes of device fabrication were performed in a clean room. Its degree of cleanness was 100; that means, the number of dust particle with ϕ ≥ 0.5 μm was less than 3500/m3. The surface morphology was measured on a scanning electron microscope (SEM) (Philips, XL 30). The reflectance spectra were obtained with a spectrophotometer (Perkin-Elemer Lambda 900). The photovoltaic (PV) parameters of solar cells were measured on a solar simulator (Oriel/Newport, model 94023A) under 1-sun AM1.5G condition. In order to confirm the observed results of the high FF, the PV measurements were independently conducted on other two different solar simulators (Oriel/Newport, model 94043A, and Oriel/Newport, model 94023A). The external quantum efficiency (EQE) of the solar cell was acquired on a QE system of Oriel/Newport.
Results and Discussion
PV parameters of the c-Si solar cells
V OC (mV)
J SC (mA/cm2)
A (700 °C, 1 s)
A− (no annealing)
In order to examine whether a charging effect of capacitance exists during the measurement, the J-V curve has been measured by scanning the voltage either from the lower voltage side to the higher one, or from the higher voltage side to the lower one, or to and fro repeatedly. They all remained the same. Hence, no charging effect exists.
Figure 3b gives the J-V curves of another solar cell prepared in a similar way as cell A, which is termed cell B. Its PV parameters are also listed in Table 1, which are quite close to those of cell A. Hence, the c-Si solar cell as shown in Fig. 3a is reproducible. Figure 3b also presents the J-V curves of the same cell B as measured independently on other two different solar simulators in two different affiliations, which are termed cells B (SARI) and B (SITP), respectively. Here, SARI stands for Shanghai Advanced Research Institute of Chinese Academy of Sciences, and SITP is for Shanghai Institute of Technical Physics of Chinese Academy of Sciences. All these curves are nearly the same. Therefore, the high FF achieved cannot arise from instrumental errors. The PV parameters of the two newly measured J-V curves of cell B in Fig. 3b are given in Table 1, too.
The experimental J-V curve of cell A in Fig. 3a is then fitted with Eq. (1). It is found that only when n = 0.56 can the calculated curve fit the experimental one well. However, the n obtained here (0.56) is far less than 1.0, which is unphysical according to its definition. Recently, Richter et al.  have simulated the PV parameters of c-Si solar cell with the model of single PN junction. According to their simulations, it is unlikely to have the very high FF for the relatively low V OC as here (<600 mV). Therefore, the model of Eq. (1) is unable to explain the result of very high FF here.
To simulate the J-V curve of PN + MOS or PN-MOS, a numerical calculation procedure was used; that is, starting from J = J SC down to J = 0, for each point of J (the step of J was chosen 0.1 mA/cm2), both V PN and V MOS were calculated by Eqs. (1) and (2), respectively, combining all the other selected PV parameters. Then, Eqs. (3) and (4) were applied to get the total voltage across the solar cell for the models of forward and inverse connections, respectively. The resulting J-V curves of PN + MOS and PN-MOS are given in Fig. 4, too. It is clear that for the forward connection, FF even becomes lower; while, for the inverse connection, higher FF is available. It should be pointed out that it is only when ϕ B /e of the MOS junction is not far from V OC of the solar cell, which is the case during the simulation of Fig. 4, could a high FF be obtained. In fact, we have simulated the relation between FF and ϕ B . It is found that when ϕ B /e is very close to or even equals V OC, FF larger than 0.9 can be obtained.
We then use the model of PN-MOS to fit the J-V curve of cell A with Eqs. (1) and (2). The fitting curve has been plotted in Fig. 3a. At this moment, the derived PV parameters are n = 1.06, ns = 1.21, ϕ B = 0.505 eV, Rs = 0.11 Ω · cm2, and Rp = 8552 Ω · cm2. The values of n and ns are now rational, and ϕ B /e is close to V OC (although not very close to 0.572 V), which is consistent with the inference derived above.
It needs to be pointed out that all the PV parameters including FF are very sensitive to the annealing conditions, as have been illustrated in Fig. 3a. If there is no annealing or the annealing is insufficient, the barrier height and the serial resistance would become larger [18, 19, 20], which could severely degrade the performance of solar cell. On the other hand, if the annealing is overdone, Ag will easily penetrate through SiO2 and into the emitter zone or even into the PN junction, then the whole device would be ruined. The RTA is mainly used to modulate the barrier height of MOS junction, so a proper RTA is crucial to get a very high FF. On the other hand, the thickness of SiO2 also influences FF as well as V OC and J SC, via influencing Ag diffusion and barrier height of the MOS junction. An optimized combination of annealing and SiO2 thickness has been performed here to achieve a high efficiency.
In summary, we have obtained high FFs (~0.87) of c-Si solar cells by using Ag contact as front electrode after proper annealing and rapid thermal annealing treatments. Our model analysis indicates that the very high FF is caused by the inverse connection of MOS (Ag/SiO2/Si) and the PN junctions, with the MOS junction possessing a barrier height/e close to V OC. By using this approach, c-Si solar cells with efficiencies >20 % are achieved due to their high FFs, although their open-circuit voltages are not high (<580 mV) here. It is expected that further improvements on increasing open-circuit voltage and meanwhile remaining the very high FF could lead to further higher efficiency.
This work is supported by the National Basic Research Program of China (973 Program), Grant No. 2012CB934303, and the National Natural Science Foundation of China under Grant Nos. 61275178 and 51472051.
LXW prepared all the samples and measured the SEM and I-V data. ZQZ measured the QE data and I-V data. TNZ and XC measured the reflectance data and I-V data. ML designed the experiments and wrote the manuscript. All authors read and approved the final manuscript.
The authors declare that they have no competing interests.
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