Abstract

A novel plasma-enhanced chemical vapour deposited (PECVD) stack layer system consisting of a-:H, a-:H, and a-:H is presented for silicon solar cell rear side passivation. Surface recombination velocities below 60 cm/s (after firing) and below 30 cm/s (after forming gas anneal) were achieved. Solar cell precursors without front and rear metallisation showed implied open-circuit voltages values extracted from quasi-steady-state photoconductance (QSSPC) measurements above 680 mV. Fully finished solar cells with up to 20.0% energy conversion efficiency are presented. A fit of the cell's internal quantum efficiency using software tool PC1D and a comparison to a full-area aluminium-back surface field (Al-BSF) and thermal is shown. PECVD-ONO was found to be clearly superior to Al-BSF. A separation of recombination at the metallised and the passivated area at the solar cell's rear is presented using the equations of Fischer and Kray. Nuclear reaction analysis (NRA) has been used to evaluate the hydrogen depth profile of the passivation layer system at different stages.

1. Introduction

Electrical rear surface passivation is becoming increasingly important in crystalline silicon solar cell technology. The main reason for that is the need for a cost decrease in the photovoltaic sector. This leads to wafers that are becoming thinner and thinner and a steadily increasing need for higher energy conversion efficiencies. The result of both trends is an increased importance of an effectively passivated rear surface. In Figures 1 to 3, simulations on rear surface passivation and cell thickness are presented using PC1D [1]. Open-circuit voltage and energy conversion efficiency η depend strongly on the rear surface recombination velocity (SRV) when high-quality silicon substrates are taken into account (s, excellent optics, front emitter, and passivation, Figure 1). For values in the range of 5∗101 cm/s to 5∗103 cm/s, the strongest interdependence was found. The thinner the solar cells the stronger this effect appears. Note that very thin solar cells (50 m) show a higher level at very low values while the 50 m cells suffer from a decreased light trapping in our simulation and convert the light a little less efficiently to electricity at the maximum power point. When looking at medium-efficient solar cells (s, excellent optics, front emitter, and passivation, Figure 2) the influence of the rear passivation increases when the cells are getting thinner. We found that the thinnest cells show even better efficiencies than thicker cells when an excellent rear passivation is applied. Low-efficiency cells (s, excellent optics, standard front emitter 50 Ω/sq, and low-level front passivation, Figure 3) show only a slight dependence on the rear passivation due to a low diffusion length (s approximately m). Hence, most minority carriers do not profit from a low rear recombination velocity but recombine in the bulk silicon. The thinner the low-efficient cells become, the more pronounced will be the influence of a good rear passivation.

Agostinelli etal. [2] have shown that silicon solar cells on very thin substrates (down to 105 m) can reach higher efficiencies compared to a standard Al-BSF rear structure when an adapted rear surface passivation is applied. Kray [3] has presented energy conversion efficiencies above 20% for substrates with less than 50 m thickness. Both publications make use of the passivated emitter and rear cell (PERC) concept [4].

Fraunhofer ISE has developed an economically feasible technology for mass production of the local rear contacts of PERCs [4] by implementing a laser technology. This patented laser-fired contacts (LFCs) approach [5] allows the local aluminium contact firing through a passivating—and in most cases isolating—layer system in approximately 1 to 3 seconds per cell. Within the same step, aluminium is alloyed into the silicon forming a regime underneath the local contact creating a very good ohmic contact at the cell’s rear [6, 7].

Rear side surface passivation schemes need to be adapted to the LFC process and to the industrial production environment. The most common layers are thermally grown silicon dioxide (Si), plasma-enhanced chemical vapour deposited (PECVD) hydrogenated amorphous silicon nitride (a-Si:H, in short: SiN), and PECVD hydrogenated amorphous silicon (a-Si:H, in short: a-Si). As thermally grown silicon dioxide (Si) layers are manufactured by a time- and energy-intensive high temperature process, they are not the first choice for mass production, although they possibly provide a very good and thermally stable passivation [8]. Unfortunately, the temperature level is not suitable for every material quality. Especially, low-cost wafers might degrade during an oxidation process.

SiN films are fabricated by a low temperature processing step (approximately 300–400°C). They also provide a very good passivation quality [915] but are not as thermally stable as Si layers [8]. The thermal stability of optimised SiN layers can be improved to a degree that is sufficient for the typical thermal budget of the solar cell production line excluding emitter diffusion. Additionally, the cells passivated with SiN films typically suffer from an inversion layer which is shunted by the local rear contacts [16, 17]. The inversion layer is due to a high density of fixed positive charges which typically can be found in SiN films.

Good a-Si films provide a very efficient surface passivation without forming such an inversion layer as a-Si films do not mainly passivate via a field effect but through the lowering of the density of states at the interface . Different groups have been using a-Si as passivation, either as single layer a-Si passivation [18], a-Si stacks [19, 20] or a-Si stacked with SiN [21, 22], or PECVD silicon oxide (Si) [23]. Not only intrinsic but also doped a-Si layers have been used. The major drawback when using a-Si passivation layers in crystalline silicon solar cell technology is the relatively low thermal stability of the passivation properties. After a typical screen printed contact firing step with temperatures of up to ∼850°C the passivation properties are strongly reduced [24].

Therefore, an alternative passivation layer system that(i)can be deposited quickly and easily at low temperatures, preferably using PECVD,(ii)provides good passivation without a significant shunting,(iii)is thermally stable in a contact firing process at ∼850°C,(iv)provides a compatible internal rear surface reflectance would be a very good way to incorporate an effective surface passivation layer system in today’s industrial solar cells.

2. Lifetime Investigation

2.1. Symmetric Sample Structure

As described above, thermally grown silicon dioxide layers provide all major requirements to be suitable for the rear passivation for silicon solar cells: good surface passivation, good rear reflectance, and thermal stability in solar cell production processes. Only the process throughput and cost and the possible degradation of the solar cell precursors seem to be the major and crucial problem.

PECVD silicon oxide layers (Si) look like a possible alternative to combine the good layer characteristics of an Si film with the benefits of PECVD. Regrettably, no PECVD Si layers could be found by the authors that show a good surface passivation and thermal stability, no matter if the layer has been annealed in different gas ambient (e.g., forming gas) or not. Hence, different stack layers have been under investigation with the PECVD Si layer being the first layer deposited (sitting directly on the wafer’s surface).

It should be noted that an investigation of deposited oxide layers stacked with PECVD Si has been presented by Agostinelli etal. [25].

Hoex etal. have presented well-passivating Si films deposited by the expanding thermal plasma (ETP) technique [26].

The lifetime investigation has been performed using silicon wafers as substrates with the following properties: float zone, p-type, boron doped, 1 Ω cm, 250 m thick, and shiny etched surfaces with a crystal orientation of (100) [27]. The wafers were cleaned with a wet chemical RCA clean bath sequence [28] including a final dip in hydrofluoric acid (HF) and subsequently, the deposition on both surfaces of the wafers has been performed. Two different PECVD stack layer systems have been investigated: (i) Si and Si and (ii) Si, Si, and Si. Si always has been the first layer deposited. The deposition took place in a parallel plate PECVD reactor using a plasma excitation frequency of 13.56 MHz and a gas mixture of monosilane (Si) and nitrous oxide (O) for the Si layer and monosilane, hydrogen () and nitrogen () for the Si layer. The deposition temperature for all layers was 350°C. The oxide layers can be deposited very quickly at a deposition rate of 120 nm/min. The nitride layer takes longer, at a rate of 8 nm/min. Thicknesses of 120 nm for the oxide and 70 nm for the nitride layers have been applied. See Figure 4 for the process sequence and Figure 5 for the sample structures.

Minority carrier lifetimes were measured using the quasi-steady-state photoconductance (QSSPC) method [29]. The surface recombination velocity has been calculated from the measured lifetimes assuming that only Auger recombination took place in the sample’s bulk (i.e., “perfect bulk”). The Auger model by Glunz etal. [30] has been applied for the calculation using the following equation [31]: with the silicon wafer’s bulk lifetime , the wafer thickness W, the effective surface recombination velocity (SRV) , and the diffusion constant for electrons .

The stack system of PECVD Si and Si led to as-deposited values below 700 cm/s. Subsequently, an annealing in forming gas at 425°C for 15 minutes has been performed. Minority carrier lifetime measurements at this stage showed values below 50 cm/s. Next, a thermal treatment comparable to firing of screen printed front contacts with a peak wafer temperature of approximately 850°C for about 3 seconds was done with increasing to <70 cm/s.

For the triple layer system (Si, Si, and Si, in short: PECVD-ONO), the same thermal processing as for the two layer sample structure has been applied. This led to the following surface recombination velocities: as-deposited: below 240 cm/s, after annealing in forming gas at 425°C for 15 minutes: below 30 cm/s, after thermal processing comparable to firing of screen printed front contacts with a peak wafer temperature of approximately 850°C for about 3 seconds: below 60 cm/s.

The results are summarised in Figure 6.

Both stack systems are suitable for the surface passivation of p-type Si wafers before and after a thermal treatment like the contact firing. After deposition and after annealing, a stronger passivation effect was found for the triple stack structure Si + Si + Si (PECVD-ONO, Patent pending). This effect will be investigated further in the future. However, one beneficial effect is the increased overall layer thickness providing a higher probability for hydrogen to diffuse to the silicon/silicon oxide interface and lowering the amount of recombinatively active interface traps.

2.2. Solar Cell Precursors

An investigation of the suitability of the newly developed PECVD-ONO stack system for passivation of solar cell rear sides is presented here. A short summary has been shown in [27].

Float zone wafers with the following characteristics were used: p-type, boron doped, 0.5 Ω cm, 250 m thick, and shiny etched surface with a crystal orientation of (100). The wafers were oxidised, front side windows were opened by photolithography. Then, an emitter was diffused into the front (120 Ω/sq.) followed by a wet chemical etch of the phosphorous silicate glass (PSG). In a second oxidation step, an antireflecting Si layer was grown on the front (and the oxide on the back was thickened). After removing the oxide on the rear and cleaning the surface in a wet chemical bath sequence of (i) HN and (ii) HF, the novel passivation stack PECVD-ONO has been deposited on the rear and the lifetime was measured. Subsequently, the samples were annealed at 425°C for 15 minutes in forming gas and/or a thermal treatment comparable to the firing of screen printed front contacts was performed. After each thermal process, the lifetime was measured using the QSSPC technique. The sample structure can be found in Figure 7 and the process sequence in Figure 8.

It can be summarised that the sample structure equals a finished solar cell except the metal contacts on front and rear.

Cuevas and Sinton have shown that implied values can be extracted from the measured effective minority carrier lifetimes [32, 33] using an approximation equation for : with Boltzmann’s constant k, temperature T, elementary charge q, free-electron density n, free-hole density p, and intrinsic free-electron density .

For p-type wafers and long diffusion lengths, (2) can be written as [32, 33] with being the density of acceptors.

can be calculated from with silicon’s density of states in the conduction band and in the valence band and the silicon band gap energy . Hence, one can calculate Implied values from QSSPC measurements. The implied was extracted at 1 sun. Initially, values of approximately 631 mV have been observed. After annealing or firing, the implied values increased strongly to values above 680 mV. Here, the results after firing were very similar regardless of whether an annealing was done prior to the firing step or not. The effect is suspected to be due to an enhancement of the front and rear surface passivation. See Figure 9.

3. Hydrogen Depth Profiling

For the passivation effect, the diffusion of hydrogen from the strongly hydrogenated silicon nitride layer to the Si/bulk Si interface might be responsible. Typically, a high density of recombinatively active states at this interface can be found. These states, mostly Si dangling bonds, can be saturated by hydrogen and implicitly made recombinatively inactive. Therefore, the hydrogen concentration and the change in hydrogen concentration in different layers within the passivation stack system is of great interest.

Nuclear reaction analysis (NRA) measurements have been performed at Forschungszentrum Dresden-Rossendorf, Germany [34]. NRA is based on a reaction between a nitrogen isotope which is accelerated to several MeV and a hydrogen atom in the sample. The reaction only takes place when the nitrogen atom has a specific kinetic resonance energy (6.385 MeV). At lower energy, no nuclear reaction will happen. At higher energy, the nitrogen atom looses speed (energy) while passing through the first atomic layers of the film. When the nitrogen is decelerated to the resonance energy, the reaction will happen if there is a hydrogen atom to react with (Figure 10). The reaction of hydrogen and nitrogen will finally lead to a atom and an alpha particle and a gamma quantum that are radiated. The reaction equations are as follows:Counting the measured gamma quanta for a certain nitrogen kinetic leads to the hydrogen concentration and the depth profile [34].

Silicon wafer samples comparable to the symmetrical lifetime samples were used for the NRA measurement [27]. The process state of the samples under investigation was as-deposited, after annealing (425°C, 15 min) and after firing (850°C, 3 s). The hydrogen depth profiling of the as-deposited sample showed a hydrogen concentration of approximately 8 at% in the PECVD Si films and approximately 16 at% in the Si film. Almost no hydrogen could be found within the crystalline silicon bulk. After annealing the hydrogen depth profile did not change much. Hence, no strong hydrogen diffusion could be observed. The sample that was subjected to the “contact firing” showed a significantly modified hydrogen profile. As expected at this temperature range, hydrogen was very mobile. The overall hydrogen concentration was lowered, within the Si layers approximately 5 at% hydrogen could be found and a peak concentration of approximately 8 at% was observed within the Si layer. This shows that a strong out-diffusion (i) from the hydrogenated layers to the ambient and (ii) from the nitride film to the surrounding oxide layers took place. No significant effect can be observed at the Si/c-Si interface (see Figure 11).

4. Solar Cell Fabrication

Finally, solar cells with the newly developed passivation stack system PECVD-ONO were fabricated to show the quality of the passivation on a final cell.

Starting the cell fabrication using float-zone Si substrates with the same characteristics as in the above experiments, the final cells exhibit evaporated TiPdAg front contacts, a thermally oxidised antireflection coating that also serves as front passivation layer, a 120 Ω/sq n-type emitter, fabricated by diffusion using a POC ambient, a 1 Ω cm p-type bulk, the newly developed PECVD-ONO stack passivation system, and an evaporated Al layer at the back and laser-fired contacts that led to a local Al-BSF underneath (above if looking at Figure 12) the point contacts. The rear surface was cleaned in a wet chemical bath sequence of (i) HN and (ii) HF.

The cell scheme can be found in Figure 12.

The final cell was annealed at 425°C in forming gas for 15 minutes. A thermal process comparable to the firing of screen printed front contacts (as used in the lifetime experiments described above) was not applied. This process would harm the solar cell structure used in this batch.

The best solar cell with the novel PECVD-ONO stack system as rear passivation led to a cell efficiency of 20.0% (see Table 1).

For comparison also thermally grown silicon dioxide was used for rear passivation within the same solar cell batch that is known for its excellent rear passivation quality. 20.8% peak efficiency could be obtained for these reference cells.

Internal quantum efficiency (IQE) measurements (Figure 13) allow for a comparison of the quality of the novel rear passivation PECVD-ONO stack with thermally grown Si as well as with full area high-quality Al-BSF (the Al-BSF cells originated from a different but similar solar cell batch). It could be proven that PECVD-ONO is superior to Al-BSF rear sides but shows lower quality than thermally grown Si.

To quantify the rear passivation quality in the finished solar cell, a numerical fit to the experimental external quantum efficiency (EQE), IQE, and reflection properties was prepared using PC1D [1]. The graphical results can be found in Figure 14. The total front and rear surface recombination velocities can be derived from the PC1D fit as 3200 cm/s ± 500 cm/s (front) and 550 cm/s ± 50 cm/s (rear), respectively. This includes the recombination at the passivated area as well as the contact area. Fischer presented an equation describing the SRV of locally contacted solar cell rear sides [36] with the minority carrier diffusion constant D, the wafer thickness W, the contact pitch , the metallisation fraction f, the SRV of the metallised surface , and the SRV of the passivated surface of the rear side. For the cells presented here, the following values are valid: = 27.1 cm2/s, W = 240 m, = 1 mm, and f = 1%. Kray and Glunz have experimentally investigated and modelled the recombination velocity at the laser-fired contacts leading to the expression [37] with  cm/s, α = 22.1 cm/s,  cm3, and  cm−3 and being the density of acceptors in the substrate (in our case  cm−3).

Hence, by using the above equations and the value extracted from PC1D, can be calculated to 500 cm/s ± 50 cm/s.

5. Conclusion

A novel surface passivation stack comprising of three PECVD layers was presented. The stack consists of a-Si:H, a-Si:H, and a-Si:H. Lifetime measurements with the novel stack system on both surfaces of p-type silicon wafers showed surface recombination velocities of <240 cm/s, after annealing at 425°C: <30 cm/s, after firing: <60 cm/s. Solar cell precursors without metallisation but with PECVD-ONO rear passivation exhibited implied values extracted from the QSSPC measurements of >680 mV. Hydrogen depth profiling using the NRA method was conducted resulting in hydrogen concentrations of approximately 8 at% in the PECVD Si films and approximately 16 at% in the Si film in the as-deposited and annealed state. After firing, the hydrogen concentrations were strongly lowered to 5 at% in the PECVD Si films and approximately 8 at% in the Si film.

Solar cells with the novel passivation stack were processed and showed efficiencies of up to 20.0%. IQE characterisation and modelling using PC1D led to a total SRV at the rear surface of 550 cm/s ± 50 cm/s. Additionally, the model for the recombination at locally contacted rear sides by Fischer and Kray led to an SRV of 500 cm/s ± 50 cm/s at the passivated area.

A patent on the novel PECVD-ONO passivation stack system is pending.

Acknowledgments

The authors would like to thank A. Leimenstoll, A. Herbolzheimer, and S. Seitz for clean room processing. The laser processing was supported by J.F. Nekarda, B. Fleischhauer, C. Harmel, and A. Grohe. Additionally, the authors thank K. Krüger for Ag plating, T. Roth for lifetime measurements, and E. Schäffer and K. Kordelos for I-V measurements. This work was partly supported by the EU funded project “Crystal Clear” under the project number SES6-CT2003-502583.