# Effect of Hydrogen Content in Intrinsic a-Si:H on Performances of Heterojunction Solar Cells

Authors: Yun-Shao Cho; Chia-Hsun Hsu; Shui-Yang Lien; Dong-Sing Wuu; In-Cha Hsieh
Journal: International Journal of Photoenergy
 (2013)

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## Abstract

Influences of hydrogen content in intrinsic hydrogenated amorphous silicon (i-a-Si:H) on performances of heterojunction (HJ) solar cells are investigated. The simulation result shows that in the range of 0–18% of the i-layer hydrogen content, solar cells with higher i-layer hydrogen content can have higher degree of dangling bond passivation on single crystalline silicon (c-Si) surface. In addition, the experimental result shows that HJ solar cells with a low hydrogen content have a poor a-Si:H/c-Si interface. The deteriorate interface is assumed to be attributed to (i) voids created by insufficiently passivated c-Si surface dangling bonds, (ii) voids formed by SiH2 clusters, and (iii) Si particles caused by gas phase particle formation in silane plasma. The proposed assumption is well supported and explained from the plasma point of view using optical emission spectroscopy.


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## Body

## 1. Introduction

The hydrogenated amorphous silicon/crystalline silicon (a-Si:H/c-Si) heterojunction (HJ) solar cell is one of the most interesting technological solutions for the photovoltaic market owing to its excellent performance and also its low processing costs. Some groups have already reported encouraging results for silicon HJ cells with a-Si:H emitters deposited by plasma-enhanced chemical vapor deposition (PECVD) [1]. Recently, efficiencies of up to 23% using PECVD have been demonstrated [2, 3]. In HJ solar cells, the control of the interface between different materials is an important factor for high-cell performances. Particularly, the reduction of carrier recombination at the p/n interface is critical. Extensive studies have also demonstrated that the use of a very thin intrinsic (i-) a-Si:H buffer layer inserted at the interface can minimize the interface recombination and thus increase the efficiency of HJ solar cells [4–6].In i-a-Si:H deposition, process parameters should be carefully controlled since they determine the film properties. It is found that lowering the deposition temperature tended to raise Si-H2 bond concentration and thus lowering the dangling bond passivation quality [7]. High temperature can somewhat lead to partial epitaxial Si growth which contains more defects than amorphous films [8, 9]. Moreover, hydrogen dilution is usually adopted for lowering electron temperature and suppressing poly silane radicals [10, 11]. A moderate dilution ratio is reported to result in a longer effective lifetime of Si wafer [12]. However, the effects of i-layer hydrogen content and plasma status on performances of HJ solar cells are rarely reported.In this study, the i-layer hydrogen content effect is investigated by computational simulation. Then, we practically fabricate 156 × 156 mm2 large-size HJ solar cells with high- and low-hydrogen content to validate the simulation result. Furthermore, the interface quality between i-layer and c-Si in high- and low-hydrogen content cases is discussed from the plasma emission spectra point of view.


## 2. Experimental

The two-dimensional, commercially available software Silvaco technology computer aided design (TCAD), from Silvaco Inc., was used to solve the Poisson equation coupled with the continuity equations of electrons and holes for virtual devices by dividing the whole structure into finite elements. The physical models that we used were Shockley-Read-Hall recombination model and concentration-dependent lifetimes. The photogeneration model including a ray tracing algorithm was used for calculating the transmission and absorption of incident light in the semiconductor layers. The solar cells considered here operate under the global standard solar spectrum (AM1.5G) illumination with 100 mW/cm2 total incident power density. The model structure was (n) a-Si:H/(i) a-Si:H/(p) c-Si/aluminum back surface field (Al-BSF). For the individual layer and the a-Si:H/c-Si interfaces, the distributions of defect states are specified. Note that for a-Si:H-related materials, the correct material parameters could be varied subject to their preparation conditions. Table 1 summarizes the main parameters used for calculation including measured and assumed values which can be found elsewhere [13–16]. The correlation between the i-layer hydrogen content and performance indicators of solar cells is calculated.Table 1
TCAD input parameters for n-Si/i-Si/c-Si HJ solar cells with various hydrogen content of i-layer.
Device parameters
Value
Device area (cm2)
1
Front surface
Texture
Solar cell structure
n-Si/i-Si/c-Si/BSF
Exterior rear reflectance (%)
90
Light source
One sun (AM 1.5, 100 mW/cm2)
Layer parameter
a-Si:H(n)
a-Si:H(i)
c-Si(p)
Al-BSF
Thickness (μm)
0.01
0.005
250
5
Band gap (eV)
1.92
1.7
1.12
1.12
Dielectric constant
11.7
11.7
11.7
11.7
Electron affinity (eV)
3.9
3.9
4.05
4.05
Electron mobility (cm2/V−1s−1)
20
20
1417
200
Hole mobility (cm2/V−1s−1)
10
10
470
80
Doping concentration (cm−3)
1
×
10
19
1
×
10
19
1
×
10
1
6
1
×
10
19
Hydrogen content (%)
—
0–18
—
—For HJ solar cell fabrication, the cell structure was Al/indium tin oxide (ITO)/(n) a-Si/(i) a-Si/(p) c-Si/Al-BSF. The boron-doped c-Si wafers with thickness of 250 nm, resistivity of 1–10 Ωcm, and surface texturization were used as a substrate. The sample size was 156 × 156 mm2. To form the Al-BSF, a 5 μm Al film was sputtered on the wafer backside followed by annealing at 800°C for 30 s. The deposition of the n-type a-Si:H was done in a PECVD system with the following process parameters: plasma frequency of 27.12 MHz, power density of 37.5 mW/cm2, substrate temperature of 200°C, deposition pressure of 90 Pa, SiH4 flow rate of 40 sccm, and total gases flow rate (PH3 + SiH4 + H2) of 125 sccm. The i-layers with low- and high-hydrogen content were prepared using hydrogen dilution ratios, H2/SiH4, of 0 and 8, respectively. Detailed parameters for the i-a-Si:H layers are summarised in Table 2. The thicknesses of n-layer and i-layer were 10 nm and 5 nm, respectively. The ITO with thickness of 90 nm was formed using sputtering to enhance the lateral conductivity and minimize reflection losses. For i-a-Si:H film properties, Fourier transform infrared (FTIR) spectroscopy was used to determine hydrogen content in the films. The hydrogen content (CH) was calculated from the integrated intensity of the Si-H rocking/wagging mode at 640 cm−1 in the FTIR spectra using the following formula [17]:
(1)CH=AωNSi∫‍ωr/wα(ω)ωdω,
where α(ω) is the absorption coefficient of the film at the wavenumber ω, ωr/w stands for the rocking/wagging bands around 640 cm−1. Aω=1.6×1019 cm−2 is the proportionality constant and NSi=5×1022 cm−3 is the atomic density of pure silicon. The film thickness was evaluated by an alpha-step profiler (Tencor, alpha-step 500). For HJ solar cells, J-V characteristics were measured under AM1.5G (1 sun, 100 mW/cm2) solar simulator irradiation. External quantum efficiencies (EQE) were measured using a lock-in amplifier with a current preamplifier under short-circuit conditions. The devices were illuminated by monochromatic light from a 150 W xenon lamp passing through a monochromator. A calibrated single crystalline silicon photodiode with known spectral response was used as a reference. The cross-sectional microstructure image was observed by high-resolution transmission electron microscopy (HRTEM). For plasma characterization, optical emission spectroscopy (OES) [18, 19] equipped with a spectra colorimeter was used to collect optical emission spectra of the plasma glowed. The measuring point was near the substrate surface.Table 2
Deposition conditions of low-H and high-H.
Parameter
Value
Low-H
High-H
Power  density (mW/cm2)
25
25
Pressure (Pa)
90
90
Electrode-to-substrate distance (mm)
30
30
Substrate temperature (°C)
180
180
SiH4 flow rate (sccm)
40
40
H2 flow rate (sccm)
0
320
Hydrogen content (%)
6
18


## 3. Results and Discussion

Figure1 schematically shows the mechanism of passivation of dangling bonds at c-Si surface. Without surface passivation, the dangling bonds act as recombination centers to trap electrons, resulting in a large recombination rate at the a-Si:H/c-Si interface of final HJ solar cells. These dangling bonds can be passivated by H atoms to obtain a relatively high-quality heterojunction. This in turn implies that H content in the i-a-Si:H layer plays a crucial role on the c-Si surface passivation for HJ solar cells. In this study the H content in the i-layer is controlled by adjusting the input hydrogen gas flow rate, and their relationship is shown in Figure 1(b). It can be seen that the hydrogen content increases with increasing the hydrogen gas flow rate due to more H atoms incorporated in the i-layer during the deposition process. However, the H content finally saturates to a value of about 18% at the hydrogen flow rate of 320 sccm. According to this result, in TCAD simulation the H content is set to be in the range of 0–18% to investigate its effect on the device performances.(a) Scheme of the mechanism of surface passivation on c-Si. (b) The relationship between hydrogen flow rate and i-layer hydrogen content.
(a)
(b)Figure2 shows the TCAD simulation result of the device external parameters such as open-circuit voltage (Voc), short-circuit current density (Jsc), fill factor (FF), and conversion efficiency (η) as a function of the H content in the i-layer. It can be seen that Voc show a strong dependence on the i-layer H content. The pure i-a-Si (H content = 0%) leads to Voc of 0.55 V, while the i-a-Si:H with H content of 6%–12% results in Voc around 0.6 V. Increasing the H content up to 18% further improves the Voc to 0.72 V. The better a-Si:H/c-Si interface passivation with an increase in i-layer H content could decrease the interface defect (dangling bond) density and recombination for carriers that overcome the a-Si:H/c-Si barrier, and thus could be the reason for the increase in Voc with an increase in i-layer H content [20]. Jsc and FF also show a similar tendency to that of Voc. Consequently, η can be significantly improved from about 11.7% to 19.7% when the H content increases from 0% to 18%. It is worth pointing out that high-H content i-layer leads to high-cell performances, which agrees well with the proposed mechanism of passivation mentioned above.Figure 2
Simulation results of the performances of HJ solar cells as a function of the i-layer hydrogen content.To validate the simulation result, experimental tests were carried out. The i-layers with low-H content of 6% and high-H content of 18% were selected for device fabrication. For each type of i-layer, 10 HJ solar cells were fabricated and their performances are quite close to each other with an error of less than 3%. Figure3(a) illustrates the J-V characteristics of the two types of HJ solar cells. It is observed that the tendency of the experimental result is in good agreement with the simulation data. The high-H cell has better conversion efficiency indicating an improved surface passivation. As compared to the low-H cell, Voc, Jsc, and FF are improved by 12.1%, 9.3%, and 9.4%, respectively. This consequently leads to an increase in η by about 34.2%. Note that FF values are slightly lower than the corresponding simulation values since the resistances of Al, ITO, and their interface are not taken into account in the simulation work.Experimental results of (a) J-V characteristics and (b) EQE spectra response for HJ solar cells with different i-layer hydrogen content.
(a)
(b)TheJsc of the fabricated low- and high-H solar cells can be investigated by EQE measurement as shown in Figure 3(b). Clearly, the EQE response can be divided into two wavelength regions. First, in the wavelength range of 300 to 700 nm, EQE values of the high-H cell are always higher than these of the low-H cell. Since blue light is absorbed close to the surface, the higher blue portion of EQE reflects a lower surface recombination and thus reflect better collection efficiency of minority carriers. Note that although the absorption of the two a-Si:H layers possibly may not be the same, the absorption loss due to very thin a-Si:H is trivial and is not one of the factors causing the observed EQE difference. Second, in the wavelength range of 700 to 1100 nm, the EQE values of the two cells become similar, since the light absorption depth in this wavelength range corresponds to deeper region in c-Si and thus irrelevant to the junction properties. The EQE at the wavelength of 1100 nm [21], close to the cut-off wavelength, is still over 20% owing to contributions of surface texturing and back surface field [22]. In summary the EQE result indicates that the higher Jsc of the high-H cells, as observed in Figure 3(a), is a consequence of the much higher spectral response in the short wavelengths due to better surface passivation.The cross-sectional HRTEM images of a-Si:H/c-Si interface in low- and high-H cells are shown in Figures4(a) and 4(b), respectively. The a-Si:H layer (including i- and n-layer) thickness of about 15 nm can also be evidenced by the TEM images. Interestingly, the low-H interface is deteriorated, whereas the interface region in the high-H case is quite smooth. The poor interface region can be assumed to mainly result from two factors. First, it is likely that the interface region contains voids or vacancies related to unpassivated dangling bonds on c-Si surface, illustrated in Figure 1(a), or from SiH2 bonds clustered in the i-layer [23]. Second, it seems that particles occur around the interface, and this phenomenon can be linked to plasma gas particle formation to c-Si substrate interaction. The assumptions are further discussed and explained below using the OES spectra from the plasma point of view.HRTEM images of the i-a-Si:H/p c-Si interface for (a) low-H and (b) high-H HJ solar cells.
(a)
(b)Figure5 compares the OES spectra between plasmas during i-layer deposition of low- and high-H solar cells. The peaks shown in the spectra result from several collision of energetic electrons with gas molecules involving the formation of neutral (SiH3, SiH2, SiH, Si), emissive (Si*, SiH*), and ionic (SiHx+) species, as given by [24, 25]
(2)SiH4+e⟶SiH3+H+e(4.0eV;τ>20ms)⟶SiH2+H2+e(2.2eV;τ<3ms)⟶SiH+H2+H+e(5.7eV;τ<3ms)⟶Si+2H2+e(4.2eV;τ<3ms)(3)SiH2⟶Si*+H2(4)Si*⟶Si+hν(4.9–5.1eV)(5)SiH3⟶SiH*+H2(6)SiH*⟶SiH+hν(3eV)
where e is the electron, hν is the released photon energy, and τ is the life time of the Si-based radicals. Among the various radicals, SiH2-related reactions described in (3), and (4) finally release a photon energy from Si* radiative decay corresponding to a wavelength of 252 nm. Interestingly, this released photon is detected by OES only in the plasma for the low-H cell, while this peak vanishes for the high-H cell. Thus, the plasma in low-H i-layer deposition contains a much larger amount of SiH2, finally leading to void-rich and low-quality i-layer [26, 27]. In addition, another effect accompanied with high SiH2 amount is the increased generation rate of poly silane (gas particle formation), Si2H6, according to [28]
(7)SiH2+SiH4⟶Si2H6
The resultant Si2H6 species will interfere with film deposition and thus lead to a poor interface. Therefore, the OES spectra confirm the assumptions as mentioned in Figure 4. On the contrary, the Si-related peak found in the spectra of the high-H cell is only SiH* at 414 nm (see (5) and (6)), and thus the increased proportion of SiH3 is beneficial to the film growth with high qualities [29] leading to a smooth interface shown in Figure 4(b).Figure 5
Optical emission spectra for the plasmas during low- and high-H i-layer deposition.


## 4. Conclusions

In this study, the effect of a-Si:H i-layer hydrogen content of 0–18% on performances of HJ solar cells is investigated. Both of the experimental and simulation results indicate that the i-layer with high-hydrogen content can lead to a higher degree of dangling bond passivation on c-Si surface. Compared to low-H i-layer, HJ solar cells with a high-H i-layer is found to have the i-layer/c-Si interface with reduced surface recombination and increased collection efficiency for blue light generated carriers. In addition to surface dangling bond passivation, the low-H solar cell exhibits a deteriorate i-layer/c-Si interface. The OES spectra clearly show the presence ofSi* peak only found in the plasma of low-H i-layer deposition suggesting that the large SiH2 portion may finally create voids and Si particles and thus decrease the i-layer/c-Si interface quality.



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*Source: 121875-2013-09-09.xml*