Chandra Kamal
Borah
a,
Pawan K.
Tyagi
bc and
Sanjeev
Kumar
*a
aCentre of Advanced Research, Department of Physics, Rajiv Gandhi University, Arunachal Pradesh-791112, India. E-mail: sanjeev.kumar@rgu.ac.in
bDepartment of Physics, Central University of Haryana, Haryana-123029, India
cDepartment of Applied Physics, Delhi Technological University, Delhi-110042, India
First published on 23rd June 2020
The efficiency of a Si-HIT (heterojunction with intrinsic thin layer) solar cell based on a graphene/MoS2 heterostructure has been optimized by varying the various parameters of graphene (Gr) as a transparent conducting electrode (TCE) and n-type molybdenum disulfide (n-MoS2) as an emitter layer. The photovoltaic performance of a graphene/n-MoS2/a-Si:H/p-cSi/Au single facial HIT solar cell has been studied using AFORS-HET v2.5 simulation software. A maximum output efficiency of 25.61% has been achieved. The obtained results were compared with the results from a commercially available a-Si:H layer and p-cSi wafer after simulation. Moreover, the dependence of the cell performance on changes in the TCE and the back contact materials has also been studied. Finally, it has been demonstrated that the graphene layer and n-MoS2 layer could act as a TCE and an efficient emitter layer, respectively, in a n-MoS2/p-cSi based HIT solar cell.
In a solar cell, a transparent conductive electrode (TCE) is required to ensure the easy transportation of carriers from the emitter layer to the external circuit. The low sheet resistance (10 Ω sq−1) and high optical transparency (85%) mean that indium tin oxide (ITO) is a commonly used TCE in photovoltaic (PV) applications. However, the high cost, rarity and mechanical rigidity of ITO have limited its use for future flexible devices and these drawbacks initiated the search for new TCE materials.6 Recently, pristine graphene has been reported to have an optical transparency as high as 97.7% (single layer graphene) with a work function of 4.31–4.5 eV (ref. 7 and 8) and a sheet resistance of 120 Ω sq−1 in few-layer graphene.6 In addition, the intercalated graphene with ferric chloride is reported to have a high optical transparency of approximately 96% with a low sheet resistance of 8.8 Ω sq−1 and a high carrier density of 8.9 × 1014 cm−2 at room temperature and a high stability in air.6 At room temperature, the carrier mobility in the graphene layer exceeds 105 cm2 V−1 s−1.9 These extraordinary properties have led to the application of multilayer graphene as a TCE. Recently, Lazar et al.7 reported that doping with boron (B) and –NH2 can increase the work function of graphene (ΦGr) to 1.20 eV and 0.46 eV from 4.31 eV (pristine graphene). Kim et al.8 demonstrated that, after being irradiated by an α beam the work function of graphene increases to 4.9 eV. Conversely, the low photoresponsivity, poor external quantum efficiency, and low absorption of light reduces the application of graphene as an emitter layer instead of the TCE layer in HIT solar cell.10 Unlike graphene, another 2D material, molybdenum disulfide (MoS2) has emerged as a complement 2D material for graphene as an emitter layer in HIT solar cells. MoS2 has a mobility of 200 cm2 V−1 s−1 in the monolayer and approximately 517 cm2 V−1 s−1 in few layers, as well as a high on/off ratio in the order of 108 (ref. 11 and 12) and a fast photo-response time of 40 μs.13 MoS2 is reported to have an indirect bandgap of 1.2 eV in the bulk form and a direct bandgap of 1.9 eV in the single layer form.14 Moreover, double layer MoS2 has more than 85% optical transparency in the visible region.15 Recently, it has been reported that the work function of MoS2 changes with a change in the number of layers.16 It has also been demonstrated that MoS2 can be used to form significant n-type doping with a Benzyl Viologen (BV) dopant17 and polyethyleneimine (PEI)18. PEI reduces the sheet resistance of MoS2 2.6 times.18 These properties mean that MoS2 can be utilized as an emitter layer in MoS2/silicon HIT solar cells.
Experimentally and theoretically, it has been demonstrated that MoS2 can act as an emitter layer in heterojunction silicon solar cells. Tsai et al.19 fabricated a heterojunction solar cell of monolayer MoS2 and p-cSi and achieved a power conversion efficiency of 5.23%. Hao et al.20 also fabricated a bulk p–n junction after depositing a 40 nm thick layer of n-MoS2 onto p-cSi substrates and a 1.3% photoconversion efficiency was achieved.
The high transparency, as well as the high mobility of the graphene layer with a tunable bandgap and work function, along with practical and theoretical demonstrations of graphene/MoS2 and MoS2/Si heterojunctions, motivated us to propose a single facial HIT solar cell structure of graphene/n-MoS2/a-Si:H/p-cSi/Au. Here, we have used graphene as a TCE material. No reports have been published on the use of graphene as a TCE in HIT solar cells so far. In addition to graphene and MoS2, there are a few interesting candidates such as carbon nanotubes, black phosphorous and MXene, that show potential for use in silicon solar cells. So far, a power conversion as high as 17.2% has been observed in carbon nanotube based silicon solar cells.21–23 After proposing the structure of the cell, the influence of various parameters of the layers used on the cell performance were studied using AFORS-HET v2.5 simulation software. The main objective of the present simulation is to study the independent effects owing to the variation of the parameters of the layers on the cell performance and to demonstrate the prospective application of graphene as an effective TCE material in a n-MoS2/p-cSi HIT solar cell.
The charge stored in the defects is described by a distribution function, ft, specifying the probability that defects with a defect density Nt are at position E if the bandgap is occupied with electrons:
The electron/hole currents (jn/p) flow owing to the gradient of the corresponding quasi-Fermi energy (EFn/p). Within the semiconducting layer, this is equivalent to the sum of the diffusion and drift current with the corresponding mobility μn/p.
If the heterostructure is illuminated (specifying the spectral distribution ϕ(λ) of the incoming photon flux), the super-bandgap optical generation rate from the valence band into the conduction band of the semiconductor layers can be evaluated by considering the Lambert–Beer absorption model by specifying the spectral absorption coefficient α, as well as specifying the dielectric properties (n,k) of each layer. An optical sub-bandgap generation from a defect to the conduction/valence band can be defined by specifying the optical emission coefficients eon(E),eop(E) ≠ 0 for the defect state.
Recombination from the conduction band into the valence band may occur directly (band to band recombination, Auger recombination) and via trap states (Shockley–Read–Hall recombination, (SHR)).
Rn,p(x,t) = RBand–Bandn,p(x,t) + RAugern,p(x,t) + RSRHn,p(x,t) |
The transportation across the heterojunction interface is modeled by drift-diffusion. In order to do so, an interface layer is considered. The specified interface defects are distributed homogeneously within this layer. The cell currents have to be evaluated directly from the gradient of the corresponding quasi-Fermi energies. The electron affinity (χ), the bandgap (Eg) and the effective conduction/valence band density of states (NC, NV) will depend on the position x within the interface layer.
The electric potential is fixed to zero at one contact. At the second contact, a boundary condition has to be specified, which relates the external cell voltage/current to the internal quantities. Furthermore, the electron and hole currents moving into the metal contacts need to be modeled. The Schottky contact can either be voltage controlled, or current controlled.
Fig. 1 (a) The proposed HIT solar cell structure, and (b) band diagram as generated using AFORS-HET software for the proposed structure. |
Parameter | Front contact | Back contact | |||
---|---|---|---|---|---|
Initially | After optimization | Initially | After optimization | ||
Material | Graphene | ITO | Al | Au | Ag |
Thickness | 1L–5L (1L = 0.334 nm) | 80 nm | 80 nm | 10 μm | 10 μm |
Optical properties | n = 2.7 | ITO nk (default) | n = 1.19 | Au nk (default) | Ag nk (default) |
k = 1.45 | k = 7.05 | ||||
Work function (eV) | 4.31 | 4.4 | 4.06 | 5.4 | 4.64 |
4.50 | 4.45 | 4.20 | 4.74 | ||
4.54 | 4.5 | 4.26 | |||
4.77 | |||||
4.90 | |||||
Absorption loss | 0.023 (constant) | ITO abs (default) | 0.056 | 0 | 0 |
External reflection | 1L = 0 | ITO Ref (default) | 0.868 | 0 | 0 |
2L = 0.023 | |||||
3L = 0.046 | |||||
4L = 0.070 | |||||
5L = 0.092 | |||||
Surface condition | Plane | Plane | Plane | Plane | Plane |
Internal reflection | 0 | 0 | 0 | 0 | 0 |
Parameter | n-MoS2 | a-Si:H(i) | p-cSi |
---|---|---|---|
Thickness | 3L–6L (1L = 0.65 nm) | 3–10 nm | 50–500 μm |
Dielectric constant (εr) | 4–14 | 11.9 | 11.9 |
Electron affinity χ (eV) | 3.74–4.45 | 3.9 | 4.05 |
Band gap, Eg (eV) | 1.41–1.48 | 1.6–2.0 | 1.12 |
Effective conduction band density, NC (cm−3) | 3 × 1018 to 9 × 1020 | 2.5 × 1020 | 3 × 1019 to 1 × 1021 |
Effective valence band density, NV (cm−3) | 3 × 1018 to 9 × 1020 | 2.5 × 1020 | 3 × 1019 to 1 × 1021 |
Effective electron mobility, μn (cm2 V−1 s−1) | 517 | 20 | 1104 |
Effective hole mobility, μp (cm2 V−1 s−1) | 8.5 | 5 | 420 |
Acceptor concentration NA (cm−3) | 0 | 0 | 1015 to 1017 |
Donor concentration ND (cm−3) | 1012 to 1018 | 0 | 0 |
Electron thermal velocity, Ve (cm s−1) | 107 | 107 | 107 |
Hole thermal velocity, Vh (cm s−1) | 107 | 107 | 107 |
Layer density, (g cm−1) | 5.06 | 2.328 | 2.328 |
Auger electron recombination coefficient, (cm6 s−1) | ∼10−24 | 0 | 2.2 × 10−31 |
Auger hole recombination coefficient, (cm6 s−1) | ∼10−24 | 0 | 9.9 × 10−32 |
Band-to-band recombination coefficient, (cm3 s−1) | ∼10−7 | 0 | 9.5 × 10−15 |
Defect type | Single | Conduction tail | Single |
Defect charge | Acceptor | Acceptor | Acceptor |
Total defect density (cm−3) | 1018 | 6.4 × 1019 | 1010 |
Specific defect density (cm−3 eV−1) | 1018 | 1.83 × 1021 | 1010 |
Defect level energy (eV) | 0.6 | 0.035 (Urbach) | 0.56 |
Electron and hole capture cross section (cm−2) | 10−14 (default) | 7 × 10−16 | 10−14 |
Optical properties | n = 4.47; k = 1.01 | a-Si nk (default) | c-Si nk (default) |
Interface | Numerical model | Remarks |
---|---|---|
Graphene/n-MoS2 | MS-Schottky contact | Surface recombination velocity for electrons and holes = 107 cm s−1 (default) |
p-cSi/Au | ||
n-MoS2/a-Si:H | Drift diffusion model | Interface charge = 1011 cm−2 |
a-Si:H/p-cSi |
(1) |
eVbi = e(ΦMoS2 − ΦGr) | (2) |
Fig. 2 Optimization of the n-MoS2 layer: (a) and (b) donor concentration ND (cm−3), (c) and (d) effective conduction band and valance band density NC/NV (cm−3), (e) and (f) the bandgap energy Eg (eV), (g) and (h) the number of layers of MoS2, (i) and (j) the electron affinity χ (eV), and (k) and (l) the dielectric constant εr. The p-cSi parameters were maintained as: thickness = 100 μm, NA = 1 × 1016 cm−3, NC/NV = 3 × 1019 cm−3 and χ = 4.05 eV, and the graphene parameters were maintained as: number of layers = 5, reflectance = 0.092 and work function = 4.31 eV. The other parameters are given in Tables 1 and 2. |
The NC/NV is related to the effective mass of the electrons and holes as follows: . Furthermore, is related to the mobility (μe/h) as follows: . From these two relationships, it can be concluded that with the change in mobility (μe/h) the conduction and valence band density (NC/NV) also changes. It has been reported that the mobility of the charge carriers in MoS2 changes with the change in the number of layer. MoS2 has a mobility of 200 cm2 V−1 s−1 in the monolayer and approximately 517 cm2 V−1 s−1 in few layers.11 Therefore, after optimization of ND to 1018 cm−3, the NC/NV was optimized in the range 3 × 1018 to 9 × 1020 cm−3 as shown in Fig. 2c and d. It can be seen in Fig. 2d that the VOC increased from 646.1 to 668 mV with an increase of the NC/NV from 3 × 1018 cm−3 to 1020 cm−3. The increment in VOC can be understood by considering the equation: in which ni is the carrier concentration, n is the intrinsic electron concentration and p represents the intrinsic hole concentration. Here, n = no + Δn and p = po + Δp, in which no and po are the concentrations of the electrons and holes in the equilibrium condition and Δn, Δp are the excess photo-generated electron and hole concentrations, respectively. As, nopo = ni2, n = ND and Δn = Δp, VOC can therefore be rewritten as .57 We can assume that VOC increased with NC/NV owing to an increase of Δp and Δn. As shown in Fig. 2d, the VOC decreased a little bit to 666.4 mV as the NC/NV increased to 9 × 1020 cm−3, which is due to the decrement of eVbi according to eqn (1). The JSC was found to remain constant at 32.33 mA cm−2 with an increase of NC/NV from 3 × 1018 to 9 × 1020 cm−3. Although the generation rate (G) of the photo-generated carriers is reported to increase with higher values of NC/NV.58 The constant JSC indicates that the photo-generated carriers either recombine or are trapped close to the metal/semiconductor interface. As with the VOC, the FF is also found to increase and a maximum value of 82.33% was obtained at NC/NV = 3 × 1020 cm−3. Therefore, η was found to be enhanced from 15.82% to a maximum value of 17.73%.
After optimization of the ND and NC/NV to values of 1018 cm−3 and 3 × 1020 cm−3, respectively we varied the bandgap (Eg) in the range 1.41–1.47 eV (ref. 39) and results are shown in Fig. 2e and f. As we can see, all of the cell parameters are constant and a value of η = 17.74% was obtained in this range of Eg.
For the simulation with different numbers of layers of n-MoS2 as shown in Fig. 2g and h, the VOC was found to remain constant at a value of 664.8 mV, whereas the JSC reduced from 33.63 to 32.33 mA cm−2, when the number of layers was increased from 3 to 6. This happens because the increase in the number of layers reduces the transmittance of photons to reach the junction, which results in a reduction of the electron–hole pair generation rate. The reduction of the transmittance with the increase in the n-MoS2 layer number leads to a reduction of the FF. The η was found to decrease from 18.54% to 17.74% as the number of layers increased from 3 to 6. Hence, we used 3L as the optimized number of layers of MoS2 for further simulation.
Fig. 2i and j show the cell parameters for the optimization of χ in the ranges 3.7 to 4.1 eV. Here we have considered Eg = 1.47 eV for 3L MoS2.42 The VOC remained constant at a value of 664.8 mV when χ (eV) was increased from 3.7 to 4 eV. Upon a further increase in the χ to 4.1 eV, a small increase in the VOC to approximately 691.4 eV was obtained owing to an increase in the eVbi. A constant JSC of 33.63 mA cm−2 was found in the range 3.74–3.90 eV of χ and this was enhanced to 34.16 mA cm−2 for χ = 4.1 eV. A small increase in the ΔEC (see Fig. 1b) was observed with the increase in χ, which leads to a slightly higher VOC and JSC at χ = 4.1 eV. The FF was observed to increase from 82.93% (@ χ = 3.74 eV) to 83.41% (@ χ = 4.1 eV) as a result of the reduction in the sheet resistance. Therefore, η was found to increase from 18.54% to 19.19%.
It has been found from electric transportation measurements that the dielectric response of the MoS2 layers is sensitive to the substrate that is used and the dielectric effect relies on the thickness of the sample.43 The effect of the dielectric constant (εr) on the cell parameters is depicted in Fig. 2k and l. It can be observed in Fig. 2l, that the VOC does not depend on the variation of εr and it was found to be a constant at 691.4 eV. However, the JSC shows a light decrement from 34.83 to 34.39 mA cm−2 with an increase of εr up to 14. In a p–n junction, , which affect the relative permittivity of the MoS2 layer.54,57 The generation of the e–h pair increases in the MoS2 layer with an increase in the εr following Coulombs law as , in which F is the electrostatic force between the electron and holes, but at the same time the increase in εr reduces eVbi. As a consequence of both of these effects, we obtained a constant VOC. In contrast, under short circuit conditions, the photo-generated carriers experienced reduced eVbi, which boosts the recombination of the carriers. Thus, the JSC was found to decrease. The FF showed a minor increase from 82.43% to 83.41% when εr was increased from 4 to 6. After this the increase in FF slowed down and only reached 83.49% for εr = 14. In Fig. 2k, η was found to largely depend on the VOC and remained constant at 19.91% with εr. The cell parameters of the proposed cell were found to be independent of the electron mobility (μn) of the n-MoS2 layer, which has been varied in the range of 517–50 cm2 V−1 s−1.
Fig. 3 Optimization of the a-Si:H(i) layer: (a) and (b) thickness (nm) in which Eg was maintained at 1.6 eV. |
To understand the effect of NC and NV on the performance of the HIT solar cell, we varied these parameters within the range of 3 × 1019 to 1 × 1021 cm−3 for the p-cSi layer. It can be observed from Fig. 4c and d, with the increase in the NC/NV, the VOC decreased linearly from 699.2 to 560.2 mV. According to eqn (1), with the increase in the NV of p-cSi layer the eVbi decreases and therefore VOC also decreases. In contrast, the value of JSC shows a small increase from 37.81 to 37.91 mA cm−2 with NC/NV. It has also been reported that NC/NV influences the bandgap as well as the absorption of photons.58 It can be estimated that for NC/NV > 3 × 1019 cm−3, the high absorption of photons in the active silicon layer increased the G of electron–hole pairs. In Fig. 4d, the FF showed a deterioration from 82.76% to 81.02%, which resulted in the η dropping to 17.2% from 21.88%. The maximum value of η = 21.88% was obtained at NC/NV = 3 × 1019 cm−3.
In solar cell technology, the thickness of the p-cSi wafer plays an important role in the fabrication of HIT solar cells. Fig. 4e and f represents the variation of cell parameters as a function of the p-cSi wafer thickness from 50 to 500 μm. In Fig. 4f, the VOC remains constant at 699.2 mV. Upon a further increase in the thickness, the VOC reduced sharply to 697.7 mV and again remained constant up to a thickness of 350 μm. Above this thickness, the VOC was found to deteriorate to the value 696.1 mV and becomes independent of the change of thickness. This variation may be due to the variation in the recombination of the photo-generated carriers under open circuit conditions. The observed enhancement in the JSC from 36.22 to 40.09 mA cm−2 can be ascribed to the boost in the generation of the charge carriers with the increase in the p-cSi thickness under short circuit conditions. The FF was observed to increase slowly from 82.72% to 82.96% owing to the reduction in the series resistance. These processes help to increase the η from 20.95% to 23.15% at a thickness of 500 μm.
To study the role of the number of layers of n-MoS2 and the a-Si:H(i) layer thickness with the best optimized p-cSi parameters, the proposed cell was again simulated by varying the number of layers of MoS2 and the thickness of a-Si:H and the results are depicted in Fig. 4g, h and i, j respectively. From Fig. 4g and h, it can be clearly seen that the VOC increased from 696.1 to 699.2 mV when the number of layers of n-MoS2 was increased from 3 to 5. Furthermore, the increase in the number of layers to 6VOC remains constant at 699.2 mV. On the other hand, the JSC, FF, and η were observed to decrease with the increase in the number of layers. The JSC decreased from 40.09% to 39.42%, the FF from 82.96% to 82.25 and the η from 23.15% to 22.67%. In Fig. 4i and j, as the layer thickness of a-Si:H(i) was changed to 6 from 3 nm, the VOC gave a constant value of 696.1 mV and increased slightly to 697.7 mV when the thickness was increased to 6 nm. The VOC then became independent of the thickness even when it was increased to 10 nm. The JSC was found to decline from 40.09 to 39.05 mA cm−2 with the thickness of a-Si:H(i). The FF was found to decrease from 82.96% to 82.38% and a minimum η of 22.14% was achieved at 10 nm.
The presence of a strong covalent bond between the C and Mo atoms or the presence of a dangling bond of sulfur present in the interfaces affects the interfacial barrier height and a variation in the barrier height results in a variation in the contact resistance.60,61 Usually, the contact resistance is a vital factor that affects the solar cell performance.62 However, many experimental reports suggest that by controlling the Fermi level (i.e. the work function) of graphene, the contact resistance can be minimized in the graphene/MoS2 interfaces.63,64 Therefore, in this work, we have focused primarily on the work function of graphene. The depicted results shown in Fig. 5c and d, show the variation of the cell parameters with the variation of the graphene work function (ΦGr) from 4.31 to 4.9 eV. A large reduction in the VOC was observed in Fig. 5d, in which it decreased from 697.7 to 141.4 mV with an increase of ΦGr. From eqn (2), it can be observed that with the increase in ΦGr, the potential barrier energy eVbi of graphene/n-MoS2 decreases. It has also been reported that when the ΦTCO (contact) of Si HIT solar is low, the eVbi of the TCO (transparent conducting oxide)/n-type emitter has the same direction as that of the eVbi of the n-emitter/p-Si. On the other hand, when the ΦTCO (contact) is high, the eVbi of the TCO/n-type emitter contact will have an inverted direction to that of the eVbi of the n-emitter/p-Si junction. Moreover, with the increase in the Φ of the TCO contact in the silicon HIT solar cell, the depletion region in the emitter region increases and widens and results in the overlap of the contact/n-type emitter region and the n-type emitter/p-type silicon junction region if the emitter is not sufficiently thin enough.4 Thus, the higher ΦGr might increase the possibility of overlapping between the graphene/n-MoS2 depletion region and the n-MoS2/p-cSi depletion region, which has resulted in a reduction in the VOC. In contrast, owing to the overlap of the graphene/n-MoS2 depletion region and the n-MoS2/p-cSi depletion region, the eVbi of n-MoS2/p-cSi reduces. This results in a reduction of the built-in electric field which is unable to push the photo-generated carriers effectively to their respective sides under short circuit conditions and thus the JSC is observed to decline linearly from 44.25 to 40.09 mA cm−2 with an increase in the ΦGr. The overall reduction in the VOC and JSC reduced η from 25.61% to 23.15%. The maximum η = 25.61% was achieved at ΦGr = 4.31 eV of pristine graphene.
To validate our simulated results, a comparison has been performed by considering the best-optimized values of n-MoS2 and a-Si:H(i) with the practically available p-cSi parameters by varying the ΦGr and p-cSi thickness within the range of 4.31–4.9 eV and the 50–500 μm range respectively, as depicted in Fig. 5e–h and Table 4, using the practically available data for p-cSi.52,65 It can be seen from Fig. 5e and f, that the maximum η = 25% was obtained at ΦGr = 4.31 eV, which is close to our best-optimized results as shown in Fig. 5c and d. Similarly, in Fig. 5g and h, the same maximum η = 25% was achieved for a 500 μm thick p-cSi wafer.
Cell parameter | Most optimized cell (before optimization of the parameters of the graphene layers) | Graphene layer number optimized cell (after optimization of n-MoS2 and p-cSi) | n-cSi wafer optimized cell for practically available silicon parameters |
---|---|---|---|
V OC (mV) | 696.1 | 697.7 | 697.7 |
J SC (mA cm−2) | 40.09 | 44.25 | 43.27 |
FF (%) | 82.96 | 82.95 | 82.82 |
η (%) | 23.15 [@ 3L n-MoS2 at ND = 1018 cm−3, NC/NV = 3 × 1020 cm−3, Eg = 1.47 eV, χ = 4.47 eV, εr = 6, μn = 517 cm2 V−1 s−1, μp = 8.5 cm2 V−1 s−1, and @ 6 nm a-Si:H(i) at Eg = 1.6 eV and @ 500 μm p-cSi at NA = 1 × 1017 cm−3, NC/NV = 3 × 1019 cm−3, χ = 4.05 eV and @ 5L graphene at Φ = 4.31 eV] | 25.16 [@ 3L n-MoS2 at ND = 1018 cm−3, NC/NV = 3 × 1020 cm−3, Eg = 1.47 eV, χ = 4.47 eV, εr = 6, μn = 517 cm2 V−1 s−1, μp = 8.5 cm2 V−1 s−1, and @ 6 nm a-Si:H(i) at Eg = 1.6 eV and @ 500 μm p-cSi at NA = 1 × 1017 cm−3, NC/NV = 3 × 1019 cm−3, χ = 4.05 eV and @ 1L graphene at Φ = 4.31 eV] | 25 [@ 3L n-MoS2 at ND = 1018 cm−3, NC/NV = 3 × 1020 cm−3, Eg = 1.47 eV, χ = 4.47 eV, εr = 6, μn = 517 cm2 V−1 s−1, μp = 8.5 cm2 V−1 s−1, and @ 6 nm a-Si:H(i) at Eg = 1.6 eV and @ 500 μm p-cSi at NA = 5 × 1016 cm−3, NC/NV = 2.8 × 1019/1.04 × 1019 cm−3, χ = 4.05 eV and @ 1L graphene at Φ = 4.31 eV] |
Fig. 6 Changing the front and back contact: (a) and (b) variation in the Φ (eV) of ITO, (c) and (d) variation in the Φ (eV) of Al, and (e) and (f) variation in the Φ (eV) of Ag. |
Fig. 6e and f shows the variation in the cell parameters when the back contact was changed from Au to Ag and the Φ of Ag was maintained from 4.64 to 4.74 eV. It was observed that in this range of Φ for Ag, the VOC increased from 664.8 to 677.3 mV, whereas the JSC remained constant at 42.76 mA cm−2. The FF and η were observed to decrease from 82.72% to 83.5% and 23.51% to 24.19%, respectively. This η was close to our simulated ηmax value, that is, 25.61% when we used Au as a contact. Here, the back contacts have been considered as the uniform thin film deposited on the backside of p-cSi.
Finally, a comparison between the experimental and theoretical demonstration of graphene, MoS2, and Si-based solar cells was performed and the results are detailed in Table 5. However, except for our work none of the studies used graphene as a contact material or TCE.
Type of study | Solar cell structure | V OC (V) | J SC (mA cm−2) | FF (%) | η (%) | Ref. |
---|---|---|---|---|---|---|
Experimental | ITO/graphene/MoS2/n-cSi/(Ti/Ag) | 0.59 | 36.8 | 73 | 15.8 | 66 |
Experimental | Au/graphene/MoS2/n-Si/In | 0.56 | 33.4 | 60 | 11.1 | 67 |
Experimental | Au/graphene/MoS2/n-Si/Au | 0.50 | 28.1 | 47 | 6.56 | 68 |
Experimental | Pd/n-MoS2/i-SiO2/p-Si/In | 0.30 | 5.5 | 42 | 4.5 | 69 |
Experimental | Ni/graphene/MoS2/p-csi/Al | 0.51 | — | — | 2.58 | 70 |
Theoretical | TCO/MoS2/SiGe:H/p-Si/Al | 0.652 | 40.01 | 83.7 | 21.85 | 3 |
Theoretical | Graphene/n-MoS2/a-Si:H/p-cSi/Au | 0.697 | 44.25 | 82.95 | 25.61 | This work |
Footnote |
† Electronic supplementary information (ESI) available. See DOI: 10.1039/d0na00309c |
This journal is © The Royal Society of Chemistry 2020 |