This invention relates to an antireflective coating (ARC) on solar cells made of crystalline silicon as well as a method for producing such an antireflective coating. The aim of the invention is to describe an antireflective coating with optimized optical properties if the solar cell is encapsulated in a solar cell module (i.e. covered by glass or comparable polymer materials with refractive index of approx. 1.5). This ARC includes a hydrogenated silicon nitride (SiXNY:H) layer for passivation as well as a niobium oxide (Nb2O5) layer with high refractive index but low absorption in the visible spectral range.
State of the art front-side ARC for crystalline solar cells exhibit a SiXNY:H (short: SiN:H) layer with two functional properties: i) Reducing the amount of reflected light at the front-side of the solar cell device as well as ii) passivating the crystalline or multi-crystalline Si wafer material (field effect passivation & chemical passivation e.g. by hydrogen passivation of dangling bonds or impurities). These SiN:H films can be either deposited by PECVD or PVD techniques and usually have refractive indices at 633 nm of 1.9-2.1 which gives optimal efficiencies (electrical power output/power input of incident useful light) for solar cells.
Generally, the optimum refractive index (n) of a single ARC film has to fulfill the well-known requirement
n=sqrt(n—s*n—m) (Eq.1)
where n_s and n_m are the refractive indices of the substrate underneath and the medium above the ARC, respectively. Therefore optimal silicon solar cells (n_s=3.8 for Si; n_m=1.0 for air) require an ARC with n=1.95.
Solar cell modules on the other hand are covered by glass or plastic covers as well as polymer cements (e.g. EVA, Ethylene Vinyl Acetate) having a refractive index of around 1.5 at 633 nm which requires an ARC with refractive index of 2.39 according to Eq.1.
The above mentioned requirements for cells and modules have been calculated for a single wavelength (in this case 633 nm) for which the reflection of light is minimal. Nevertheless the above considerations are still valid if the solar cell efficiency is calculated by more elaborated methods including the optical properties of the ARC over the whole spectral range which is of importance for terrestrial solar applications. These more elaborated calculations can be performed either by dedicated software (e.g. PC-1D) or by calculating a weighted optical loss which reduces the efficiency of a hypothetical perfect ARC (transmission 100%). Every time simulated efficiencies are presented within the current work this second approach has been used, assuming an efficiency of 17.5% for a solar cell having perfect ARC.
a) and b) show the results of such a simulation on module level: For each refractive index the optimal film thickness has been calculated, and the resulting module efficiencies show a significant improvement for a refractive index of 2.4 and film thickness of 64 nm for the ARC. In order to calculate solar efficiency the reflection spectrum is convoluted by a spectral response function (also shown in the reflection graph) calculated from the AM1.5 photon flux multiplied by a typical IQE for mc-Si wafer material. Glass front-side reflection of 4% is also included in the reflection data.
(Note: If not stated otherwise all refractive indices stated from this point on refer to a wavelength of 633 nm which is also roughly the weighted center of the AM1.5 solar spectrum.)
Eq.1 as well as the simulation results in
The same trends have also been observed for PECVD SiN:H e.g. by Soppe et. al. [Prog. Photovolt: Res. Appl. 2005; 13:551-569] or Doshi et. al. [Applied Optics 36 (1997) 7826]: A compromise must be made in either the extinction coefficient or refractive index when trying to simultaneously obtain high values of n and low values of k in SiN:H films obtained from silane and ammonia.
Results for PVD SiN:H ARCs as well as PECVD results published e.g. in Doshi et. al. or Moschner et al. [Prog. Photovolt: Res. Appl. 2004; 12:21-31] revealed that SiN:H layers show improved passivation if Si-rich films with a higher refractive index of 2.3-2.4 are used during the initial phase of the film growth (close to the Si—SiN interface). This led to the development of double- or gradient layers by means of altering reactive gas compositions during the SiN:H deposition in order to have high refractive index material only close to the interface and low index material (with low absorbance) during the main part of the film deposition. One typical example of such a double layer SiN:H (labeled “SiN_DL” in
Several transparent materials (e.g. TiOX or Nb2O5) are known to have high refractive index n>2.2 and very low absorption from 300 nm to 1200 nm. But these materials will fall short in fulfilling the second requirement for solar cell ARCs: solar cell passivation by means of field effect passivation as well as chemical passivation e.g. by hydrogen passivation of dangling bonds or impurities.
U.S. Pat. No. 3,977,905 describes a single layer ARC made of Nb2O5 for use on solar cells protected by a glass cover, and specially emphasizes the low absorption in the short wavelength region from 300-500 nm. In a preferred embodiment the niobium is deposited by standard electron beam evaporation. Since no hydrogen containing process gases are used this single layer Nb2O5 ARC is not able to create sufficient surface and bulk passivation which is needed for state of the art multi-crystalline or mono-crystalline Si solar cells.
On the other hand Nb2O5 is well known as low absorbing transparent film for all kinds of optical applications. Nb2O5 being part of a multilayer ARC is described e.g. in U.S. Pat. No. 5,372,874 aiming at producing a broadband ARC for optical coatings with low absorption in the visible spectrum by means of reactive DC sputtering. The disclosure refers to a metal layer or specifically to a four layer ARC. Two layer ARCs for solar cell applications are also published in numerous ways: E.g. GB1526171 describes a combination of a high refractive index material (n=2.35-2.4, preferably an oxide of titanium) together with a low refractive index material (n=1.6-1.7, preferably an oxide of aluminum) where the high refractive index material is closer to the Si wafer and the low index material closer to the glass cover.
A double layer with a designated passivation layer close to the substrate is described in WO/2007/051457. Here the second layer is designed in such a way to hinder out-diffusion of hydrogen into the ambient during furnace firing. For improved optical performance the first layer made of either 1-10 nm of Si:H or 3-10 nm of SiN:H is combined with a second layer of TiO2, where the first layer is deposited by PECVD and the second TiO2 layer is deposited by means of sputtering (PVD).
A sketch of the most basic embodiment of the invention is shown in
The present invention proposes
a)-c) show Calculated absorption (a), reflection & absorption (b) as well as resulting solar module efficiency (c) for single layer high refractive index SiN:H films, double layer SiN:H films (labeled “SiN_DL”, having a high refractive index of approx. n=2.3 close to the interface, and approx. n=2.0 for the second layer), and two SiN:H/Nb2O5 double layer film stacks (with variable SiN film thickness but same overall thickness), respectively. Glass front-side reflection as well as low wavelength absorption of typical solar glass material is included in the calculation.
Number | Date | Country | |
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61582880 | Jan 2012 | US |