A photonic-plasmonic structure for enhancing light absorption in thin film solar cells Joydeep Bhattacharya, Nayan Chakravarty, Sambit Pattnaik, W. Dennis Slafer, Rana Biswas, and Vikram L. Dalal Citation: Appl. Phys. Lett. 99, 131114 (2011); doi: 10.1063/1.3641469 View online: https://doi.org/10.1063/1.3641469 View Table of Contents: http://aip.scitation.org/toc/apl/99/13 Published by the American Institute of Physics Articles you may be interested in Photonic crystal enhanced light-trapping in thin film solar cells Journal of Applied Physics 103, 093102 (2008); 10.1063/1.2908212 Plasmonic nanoparticle enhanced light absorption in GaAs solar cells Applied Physics Letters 93, 121904 (2008); 10.1063/1.2988288 Surface plasmon enhanced silicon solar cells Journal of Applied Physics 101, 093105 (2007); 10.1063/1.2734885 Plasmonic reflection grating back contacts for microcrystalline silicon solar cells Applied Physics Letters 99, 181105 (2011); 10.1063/1.3657513 Tunable light trapping for solar cells using localized surface plasmons Journal of Applied Physics 105, 114310 (2009); 10.1063/1.3140609 Improved red-response in thin film a-Si:H solar cells with soft-imprinted plasmonic back reflectors Applied Physics Letters 95, 183503 (2009); 10.1063/1.3256187 APPLIED PHYSICS LETTERS 99, 131114 (2011) A photonic-plasmonic structure for enhancing light absorption in thin film solar cells Joydeep Bhattacharya,1 Nayan Chakravarty,1 Sambit Pattnaik,1 W. Dennis Slafer,2 Rana Biswas,1,3,a) and Vikram L. Dalal1,a) 1 Microelectronics Research Center and Department of Electrical and Computer Engineering, Iowa State University, Ames, Iowa 50011, USA 2 Lightwave Power, Cambridge, Massachusetts 02138, USA 3 Department of Physics and Astronomy and Ames Laboratory, Iowa State University, Ames, Iowa 50011, USA (Received 11 May 2011; accepted 21 August 2011; published online 30 September 2011) We describe a photonic-plasmonic nanostructure, for significantly enhancing the absorption of long-wavelength photons in thin-film silicon solar cells, with the promise of exceeding the classical 4n2 limit for enhancement. We compare identical solar cells deposited on the photonic-plasmonic structure, randomly textured back reflectors and silver-coated flat reflectors. The state-of-the-art back reflectors, using annealed Ag or etched ZnO, had high diffuse and total reflectance. For nano-crystalline Si absorbers with comparable thickness, the highest absorption and photo-current of 21.5 mA/cm2 was obtained for photonic-plasmonic back-reflectors. The periodic photonic plasmonic structures scatter and reradiate light more effectively than a randomly roughened C 2011 American Institute of Physics. [doi:10.1063/1.3641469] surface. V Long-wavelength red and near-infrared (IR) photons are poorly absorbed in thin film silicon solar cells, due to their long absorption lengths.1,2 Light trapping is necessary to harvest photons with k > 600 nm. A randomly textured back reflector is commonly used that reflects light randomly thereby increasing the photon path length in the absorber layer.3–14 Recently, much work has been done on periodically textured back reflectors (BRs) that enhance longwavelength photon absorption through diffraction and light concentration.15–29 Here we systematically compare randomly textured BRs with a periodic, designed, photonic plasmonic reflector, and show that the photonic plasmonic structure is more effective in enhancing light absorption in thin film Si solar cells. We choose nano-crystalline silicon (nc-Si) as the absorber material, since micro-morph tandem solar cells are a widely accepted high efficiency thin-film cell architecture,1,2,6,9,14,29 with a top amorphous hydrogenated silicon (a-Si:H), and a bottom nc-Si cell. The a-Si:H cell collects short-wavelength photons, whereas the nc-Si cell collects red and near-IR photons up to the band edge (1100 nm). It is necessary to achieve light trapping in the bottom nc-Si cell rather than in a-Si:H. We identify photon management strategies that maximize the photo-current by systematically comparing nc-Si solar cells grown on randomly roughened and periodically textured BRs. For meaningful comparisons, the nc-Si absorber layer thicknesses were kept the same and the device architecture was identical in the solar cells. Randomly roughened BRs, with features much less than the wavelength, randomly scatter incoming light. Yablonovitch30 demonstrated that Lambertian scattering increases the path length by 4n2, for loss-less conditions, where n(k) is the refractive index. This enhancement can approach 50 in silicon.30 There are significant losses, and experimental enhancements are suggested31 to be considerably less than 4n2. Alternatively, periodic BRs have a pitch considerably smaller than the wavelength in the absorber k/n(k). Incoming light is diffracted by the periodic texture, with closely spaced diffraction resonances, where absorption is maximized.15,20,27,28 Also plasmonic concentration of light near the periodic BR increases the enhancement.20,25 We show that this combination of photonic and plasmonic effects works the best at enhancing light absorption in thin film cells. The concept is widely applicable to any material system, particularly to organic cells. We used six distinct BRs including 1) A planar stainless steel (SS) substrate; 2) A SS substrate with a Cr (5 nm)/Ag (200 nm) layer followed by 80 nm of ZnO; 3) Annealed Ag/ ZnO on SS with annealing of Cr/Ag at 400 C followed by 80 nm of ZnO; 4) Etched ZnO using 1 lm of Al doped ZnO deposited by sputtering, and then etched with a hydrochloric (HCl) acid (0.185%). A 5 nm Cr layer followed by a 100 nm Ag layer were thermally evaporated on the roughened etched ZnO. Feature sizes between 400 and 1500 nm were observed in roughened substrates. We utilized SS substrates with periodic nano-structures prepared using nano-imprint lithography9 at Lightwave a) FIG. 1. (a) SEM image of nano-hole back reflector. (b) SEM image of nano-pillar back reflector. The pitch is 750 nm. Authors to whom correspondence should be addressed. Electronic addresses: biswasr@iastate.edu and vdalal@iastate.edu. 0003-6951/2011/99(13)/131114/3/$30.00 99, 131114-1 C 2011 American Institute of Physics V 131114-2 Bhattacharya et al. Appl. Phys. Lett. 99, 131114 (2011) FIG. 2. (Color online) AFM images of photonic plasmonic BR (a), nano-hole (b), and (c) annealed Ag BRs. SEM images from the top of ITO showing the conformal growth of the solar cell on the photonic plasmonic BR (d), nano-hole (e), and etched ZnO/Ag (g). Schematic cross section of p-i-n solar cell. Power (Cambridge, MA). Nano-imprinting used a reverse master to imprint a large area pattern onto a polymer layer on a substrate. The pitch of the periodic pattern was 750 nm, optimized with rigorous scattering matrix simulations.15,18,32 The nano-pillars were tapered (Fig. 1), a feature found in simulations32 to enhance light absorption with a height of 160 nm, near the optimum. The hole arrays had depths of 200 nm as optimized previously.17 After Ag/ZnO deposition, the deposition of n-i-p layers at temperatures below 250 C, was performed. The cells grow conformally (Fig. 2), with the substrate pattern observed at the top of the cell. The Raman spectra gave a crystalline volume fraction as described elsewhere.33 The i-layer crystallinity was kept constant at 55% for all devices. Before device fabrication, we characterized the randomly roughened BRs by measuring total and diffuse reflectance. We selected annealed Ag and etched ZnO reflectors as benchmark “best” reflectors, because they had (Fig. 2) very high diffuse reflectance, exceeding 70% over the entire spectral range (400–1100 nm), comparable to the state-of-theart.6,7,10,29 Nc-Si solar cells were deposited using plasma enhanced chemical vapor deposition employing H-profiling. A 250 nm a-Si:H nþ layer was grown on the substrates, followed by a very thin intrinsic a-Si:H seed layer (Fig. 3), and a thick ncSi layer. Optical specular reflection measurements found the i-layer absorber thickness to be 0.95 lm. Optical and electrical characterization on nc-Si:H solar cells were made. We measured I-V curves (Fig. 3) and the external quantum efficiency (EQE) to obtain the wavelength dependent photo-current between 400 and 1100 nm (Fig. 3) for all devices to confirm the I-V curves. A standard c-Si photo-diode was used for calibration of EQE and I-V. The EQE has a maximum of 90% near 530 nm. We used a 1.0 V bias measurement in QE to ensure complete collection of photo-generated carriers. There was only 2%-3% difference between EQE at 0 V and at 1 V. The discrepancy between currents observed in I-V and from QE was within 2%-3%. The progression of the currents estimated from EQE is described in Table I and in Fig. 3. The lowest current is obtained (Table I) for cells on SS. Ag on SS improves the current by 13%. Etched ZnO þ silver gives a higher current. Annealed Ag or nano-holes imprinted substrates shows a 27% improvement over flat silver, and finally, the photonic plasmonic structure gives the best results, an increase of 34% over flat silver. The EQE shows that cells on the Ag coated nano-hole, photonic plasmonic substrate, and randomly roughened substrates are considerably enhanced over the flat Ag/ZnO and SS substrates at long wavelengths (k > 580 nm) up to the band edge (1100 nm). The EQE oscillations for the periodic substrates are due to the diffraction. The EQE for the photonic plasmonic BR exceeds that of the etched ZnO and annealed Ag BRs over a wide range (k ¼ 580–800 nm). FIG. 3. (Color online) (a) Measured EQE (at 1.0 V) and (b) current-voltage characteristics for nc-Si solar cells on stainless steel (SS), flat Ag, random textured annealed Ag/ZnO, random textured etched ZnO/Ag, periodic nanohole, and photonic plasmonic substrates. The device deposited on the photonic plasmonic substrate produces the highest EQE at long wavelengths, in agreement with Table I. 131114-3 Bhattacharya et al. Appl. Phys. Lett. 99, 131114 (2011) TABLE I. Photo-currents (J) obtained from the EQE under AM1.5 illumination for a sequence of nc-Si solar cells, grown under identical device architectures on the different types of periodic, random, and flat reference BRs. The photo-current enhancement over the reference flat Ag/ZnO and bare SS substrates is shown. The obtained J agrees well with the I-V curves of Fig. 3. Type of back reflector Bare stainless steel substrate SS þ Ag Annealed Ag/ZnO Etched ZnO Nano hole/Ag/ZnO Photonic plasmonic BR/Ag/ZnO J (at 1.0 V) (mA/cm2) % Enhancement over flat Ag/over bare SS 14.2 16.1 20.4 19.9 20.4 21.5 — —/13 27/43 18/39 27/43 34/51 Significantly the photo-current Jsc for the photonic plasmonic substrate is the highest (21.5 mA/cm2), exceeding that of the randomly roughened annealed Ag BR, the etched ZnO/Ag, by comfortable margins much greater than the experimental uncertainties. For maximum plasmonic enhancement the back nþ layer should be very thin so that the reradiated photons from the plasmonic effect are not absorbed directly into it. Our devices had relatively thick back nþ layers, 0.25 lm to avoid shorts. Calculations show the best effects when the nþ layer thickness is <100 nm. We chose absorber layer thickness of 1 lm, typical for micro-morph cells. These conclusions should be observed for other thicknesses. Although surface plasmons can cause losses in random BRs, a substantial fraction of light coupled into localized plasmonic modes at the Ag/ZnO interface may be re-radiated in optimized textured back reflectors,14 and dynamical effects need further understanding. In conclusion, we have fabricated a controlled series of nc-Si solar cells on both photonic-plasmonic back reflectors and randomly textured back reflectors. The randomly textured BRs were chosen to have very high diffuse reflectance. The periodic BR of photonic plasmonic nano-structures outperforms the best annealed silver randomly textured back reflector, illustrating the viability of the photonic plasmonic structure for advanced photon harvesting. A very interesting direction is to combine our plasmonic structure with random texture. We thank Max Noack, Supriyo Das, and the entire Microelectronics Research Center team at Iowa State University. 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