We analytically investigate the light trapping performance in plasmonic solar cells with Si/metallic structures. We consider absorption enhancements for surface plasmon polaritons (SPPs) at planar Si/metal interfaces and localized surface plasmon resonances (LSPRs) for metallic spheres in a Si matrix. We discover that the enhancement factors at Si/metal interfaces are not bound to the conventional Lambertian limit, and strong absorption can be achieved around plasmonic resonant frequencies. In addition, those enhancements are greatly reduced as the fields decay away from the Si/metal interfaces. Therefore, localized plasmonic resonances can be used as efficient light trapping schemes for ultrathin Si solar cells (< 50 nm), while photonic guided mode enhancement is more appropriate for thicker films.
© 2012 OSA
CorrectionsXing Sheng, Juejun Hu, Jurgen Michel, and Lionel C. Kimerling, "Light trapping limits in plasmonic solar cells: an analytical investigation: errata," Opt. Express 20, 24699-24700 (2012)
In this paper, we analytically explore the fundamental light trapping limits for solar cells with various plasmonic structures. Research in thin-film silicon solar cells has been actively pursued in order to further reduce the module cost of the conventional Si wafer-based technology . Current thin-film Si technology, however, still show inferior performance compared to its wafer-based counterpart, mainly because of the low near-bandgap absorption for Si. Recently, solar cells based on plasmonic structures have been widely studied and considered to be a promising candidate for achieving high performance . In such dielectric/metallic structures, the induced plasmonic modes cause significant absorption enhancement and therefore can possibly improve the cell efficiency. However, metallic structures also suffer from parasitic loss and should be carefully designed enhance absorption in the active device layer while suppressing loss in metals.
The schematic solar cell structure we investigate is illustrated in Fig. 1 . When sunlight is incident upon a Si/metal solar cell structure, various processes can be induced to cause light trapping in the active Si layer, improving photon absorption: (1) Photonic guided modes propagate in the Si layer. These modes can be obtained by various scattering schemes like random textures , periodic gratings  and metal particles ; (2) Surface plasmon polaritons (SPPs) propagate at the planar Si/metal interface, which can be accomplished by coupling through corrugated films  or prisms ; (3) Localized surface plasmon resonances (LSPRs) are induced by metallic nanoparticles or gratings , which increase the effective photon absorption cross-section. Therefore, we can assume the incident light intensity is splitted into those three different ports that can be analyzed independently. The fundamental limits for photonic guided modes inside a weakly absorptive material have been extensively studied. The well-known results are classical 4n2 Lambertian limit , which concludes that the single pass absorption (αd) can be optimally enhanced by a factor Fph = 4n2 (Fph is about 50 for crystalline Si). Modified theories have also been proposed, which successfully establish photonic light trapping in the thin film regime [10–14]. For example, for ultrathin films (in the single mode regime) the upper limit of photonic enhancement factor is , where nwg and αwg are the group index and absorption coefficient of the waveguide mode, respectively . Combined photonic-plasmonic light trapping effects have also been discussed in recent literatures [12,14]. Plasmonic structures (SPPs and LSPRs) can provide unusually high local photonic density of states due to high field concentration at the dielectric/metal interfaces . These plasmonic modes significantly enhance the local photon absorption, and their optical enhancement cannot be evaluated by the conventional Lambertian models. Here we resort to rigorous electromagnetic analysis to understand the sole light trapping contribution to SPP and LSPR modes
2. Light trapping by surface plasmon polaritons (SPPs) at Si/metal interface
We consider a device geometry shown Fig. 2(a) , which is a planar interface between semi-infinite Si and metal. We assume the refractive index for Si is n2 = 3.6 (ε2 = 3.6*3.6), with an absorption coefficient α = 12.56 cm−1. Metals are chosen to be Ag, Au or Cu, of which the optical constants (ε1) are referred to . By rigorously solving the Maxwell Equations and the corresponding boundary conditions , we can derive the field components for the surface plasmon polariton (SPP) propagating mode:
The SPP propagation constant is
Here we consider a thin region with a thickness d in the Si side of the interface, where the field of SPP is mostly concentrated. Outside this region, the absorption enhancement is mainly induced by scattering and can be analyzed using Lambertian models. The ratio of absorption in this thin Si active layer to the total absorption in the SPP mode is
ASPP can be compared with the single pass absorption in the thin region, and the enhancement factor for SPP light trapping can be obtained:
Figure 2(b) plots FSPP as a function of wavelength for different metals when d approaches zero. All the curves peak at the corresponding plasma frequencies of the metals (when ε1 + ε2 = 0), of which the corresponding wavelengths are 0.582 μm, 0.679 μm and 0.652 μm for Ag, Au and Cu, respectively. As the electric fields evanescently decay away from the Si/metal interface, those peak values of FSPP are greatly decreased in thicker films. As illustrated in Fig. 2(c), FSPP becomes dominated by classical limits (4n2 ≈50) when the absorber thickness d exceeds a few nanometers.
3. Light trapping by localized surface plasmon resonances (LSPRs) in metal spheres
Another light trapping design is to use the localized surface plasmons excited by metal nano/micro particles embedded in semiconductors. In Fig. 3(a) , we consider a metal sphere (with a radius a) inside the dielectric Si medium. The absorption cross-section for this sphere can be described as the difference of the extinction cross-section and scattering cross-section :
In addition, the internal field E1, the scattered field Es, and the incident field Ei can be described by 
This can be compared with the single pass absorption (if we assume the absorbing Si shell is a planar film with the same volume), and the enhancement factor FLSPR can be obtained:
In this case, we assume d is small so that FLSPR is a function of material permittivity and sphere radius a. When the radius is small (a = 10 nm in Fig. 3(b)), only dipole resonances are excited. Therefore, the calculated enhancement factors FLSPR peak at the corresponding resonant frequencies (ε1 + 2ε2 = 0) . Around these resonance frequencies, significant absorption enhancement can be obtained, which are about 400, 250 and 120 for Ag, Au and Cu respectively. When the sphere radius becomes larger, higher order resonances can be observed, as shown in Fig. 3(c) for a = 200 nm. However, the enhancement is greatly reduced, because larger spheres generally provide greater scattering (instead of absorption) , which can in turn be analyzed by classical or modified Lambertian light trapping [9–11].
To summarize, we use theoretical approaches to analyze the fundamental light trapping limits for plasmonic solar cells, especially for SPPs at planar Si/metal interfaces and LSPRs in spherical metal particles. We show that the absorption enhancement due to highly concentrated field in plasmonic structures is not bound to conventional 4n2 light trapping limit. However, it should be noted that these calculations only provide upper limits for enhancements induced by SPPs and LSPRs in the ultrathin region closed to the Si/metal interfaces. Photonic modes in the dielectric body should still be explained by classical Lambertian models [9–11]. Combined photonic-plasmonic effects should be considered in a film with a considerable thickness (for example, larger than 50 nm) to make more practical predictions. Examples of such successful implementations have been reported in a few recent publications [12–14, 19]. These results can also be applied to other photovoltaic materials including III-V and organic semiconductors [13, 14]. To obtain resonance modes with different spectral range, metals and alloys with different plasmonic frequencies will need to be employed . For a real device, other issues like surface recombinations are also to be taken into account. For SPP modes, practical coupling methods should be introduced, which are not discussed in this paper. Angular sensitivity will be another issue for SPPs. LSPRs may have no coupling issues and less sensitive angular responses, but the metal particle size and shape should be carefully designed, depending on whether absorption or scattering is preferred. LSPRs induced by particle interactions can also enhance field concentration and should be explored in the future.
This work was supported by the Masdar Institute of Science and Technology. J. Hu also would like to acknowledge funding support provided by the DOE Sunshot Program under the award number DE-EE0005327.
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