In this work we study the importance of optimizing the parameters of photoconductive layers to improve the efficiency of a photovoltaic cell. We compare the evolution of the performance of solar cells based on chalcopyrite materials by considering a non-decreasing band gap structure named model (a) based on the structure ZnO(n+)/CdS(n)/CuInSe2(p)/CuInS2(p+) and a decreasing band gap structure named model (b) based on the structure ZnO(n+)/CdS(n)/CuInS2(p)/CuInSe2(p+). The two structures are composed of 4 layers named respectively region 1, region 2, region 3 (base), region 4 (substrate); between regions 2 and 3 is located the space charge region (SCR) where exists a high electric field. The calculation of the external quantum efficiency of the cell and the short-circuit photocurrent density by numerical calculation are established by using the continuity equation of charge carriers and parameters such as the absorption coefficient, diffusion length which models the purity of the material, recombination velocities at the surface and at the interface which models their states, the thicknesses of the different layers, the solar irradiation. The results obtained applied to models (a) and (b), are presented in the form of tables and curves widely analyzed and commented. Considering first the same standard parameters, the model (a) whose absorption threshold is localized in the space charge region and the base, gives the best performance compared to model (b) whose absorption threshold is localized in the substrate. However, the optimization of the parameters, shows an improvement of the performances of the two models but above all a great evolution of the performances of the model (b) which external quantum efficiency becomes appreciably equal to that of the model (a). The short-circuit photocurrent density for solar spectra (AM0, AM1, AM1.5) evolves from (44.92 mA.cm-2; 33.031 mA.cm-2; 30.179 mA.cm-2) → (48.119 mA.cm-2; 35.155 mA.cm-2; 32.188 mA.cm-2) for the model (a), and evolves from (24.525 mA.cm-2; 19.309 mA.cm-2; 17.507 mA.cm-2) → (46.841 mA.cm-2; 34.303 mA.cm-2; 31.388 mA.cm-2) for the model (b).
Published in | American Journal of Energy Engineering (Volume 10, Issue 3) |
DOI | 10.11648/j.ajee.20221003.11 |
Page(s) | 53-67 |
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This is an Open Access article, distributed under the terms of the Creative Commons Attribution 4.0 International License (http://creativecommons.org/licenses/by/4.0/), which permits unrestricted use, distribution and reproduction in any medium or format, provided the original work is properly cited. |
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Copyright © The Author(s), 2022. Published by Science Publishing Group |
Solar Cell, Chalcopyrite Materials, Structure Parameter Optimization, Efficiency
[1] | M. Powalla, E. Lotter, R. Waechter, S. Spiering, M. Oertel, B. Dimmler, “Pilot line production of CIGS modules: first experience in processing and further developments”, Proc. 29th IEEE Photovoltaic Specialists Conf., New Orleans, 2002, p. 5 71. |
[2] | J. Kessler, M. Bodegard, J. Hedstrom and L. Stolt, “New world record Cu(In,Ga)Se, based mini-module: 16.6%”, Proc. 16 th European Photovoltaic Solar Energy Conf., Glasgow, 2000, p. 2057. |
[3] | M. Contreras, B. Egaas, K. Ramanathan, J. Hiltner, A. Swartzlander, F. Hasoon and R. Noufi, “Progress toward 20% efficiency in Cu(In,Ga)Se2 polycrystalline thin-film solar cells”, Prog. Photovolt. Res. Appl. Vol. 7, 1999, p. 311. |
[4] | J. F. Guillemoles, P. Cowache, A. Lusson, K. Fezzaa, F. Boisivon, J. Vedel and D. Lincot, “High quality CuInSe2 epitaxial films-molecular beam epitaxial growth and intrinsic properties”, J, Appl. Phys., Vol. 79, 1996, p. 7293. |
[5] | C. Eberspacher, K. L. Pauls and C. V. Fredric, “Improved processes for forming CuInSe2 films”, Proc. 2nd World Conf. on Photovoltaic Solar Energy Conversion, Vienna, 1998, p. 303. |
[6] | K. Ramanathan, R. N. Bhattacharya, J. Granata, J. Webb, D. Niles, M. A. Contreras, H. Wiesner, F. S. Haason and R. Noufi, “Advances in the CIS research at NREL”, Proc. 26th IEEE Photovoltaic Specialists Conf., Anaheim, 1998, p. 319. |
[7] | D. Lincot, J.-F. Guillemoles, P. Cowache, A. Marlot, C. Lepiller, B. Canava, F. B. Yousfi and J. Vedel, “Solution deposition technologies for thin film solar cells: status and perspectives”, Proc. 2nd World Conf. on Photovoltaic Solar Energy Conversion, Vienna, 1998, p. 440. |
[8] | F. Karg, D. Kohake, T. Nierhoff, B. Kuhne, S. Grosser and M. C. Lux-Steiner, “Performance of grid-coupled PV arrays based on CIS solar modules”, Proc. 17th European Photovoltaic Solar Energy Conf., Munich, 2002, p. 391. |
[9] | R. R. Gay, “Status and prospects for CIS-based photovoltaics”, Solar Energy Mater. Solar Cells, Vol. 47, 1997, p. 19. |
[10] | E. M. Keita, B. Ndiaye, M. Dia, Y. Tabar, C. Sene, B. Mbow,“Theoretical Study of Spectral Responses of Heterojunctions Based on CuInSe2 and CuInS2” OAJ Materials and Devices, Vol 5#1, 0508 (2020) – DOI: 10.23647/ca.md20200508. |
[11] | Subba Ramaiah Kodigala, “Cu(In1-xGax)se2 based thin solar cells”, 2010, Volume 35, Academic Press, ELSEVIER. Inc. |
[12] | T. Loher, W. Jaegermann, C. Pettenkofer, “Formation and electronic properties of the CdS/CuInSe2 (011) heterointerface studied by synchrotron-induced photoemission”, J. Appl. Phys. 77 (1995) 731. |
[13] | H. Hahn, G. Frank, W. Klinger, A. D. Meyer, G. Strorger, “Über einige ternäre Chalkogenide mit Chalcopyritestruktur”, Z. Anorg. Aug. Chem. 271 (1953) 153. |
[14] | Liann-Be Chang, Chzu-Chiang Tseng, Gwomei Wu, Wu-Shiung Feng, Ming-Jer Jeng, Lung-Chien Chen, Kuan-Lin Lee, Ewa Popko, Lucjan Jacak and Katarzyna Gwozdz, ‘’Low-Cost CuIn1−xGaxSe2 Ultra-Thin Hole-Transporting Material Layer for Perovskite/CIGSe Heterojunction Solar Cells’’, Appl. Sci. 2019, 9, 719; doi:10.3390/app9040719. |
[15] | Anjun Han, Yi Zhang, Wei Song, Boyan Li, Wei Liu and Yun Sun,’’ Structure, morphology and properties of thinned Cu(In, Ga)Se2 films and solar cells’’, Semicond. Sci. Technol. 2012, 27, 3. |
[16] | S. J. Fonash, Solar Cell device Physics, Academic Press, New York, 1981. |
[17] | H. L. Hwang, C. Y. Sun, C. Y. Leu, C. C. Cheng, C. C. Tu, “Growth of CuInS2 and its characterization”, Rev. Phys. Appl. 13 (1978) 745. |
[18] | E. M. Keita, B. Mbow, M. S. Mane, M. L. Sow, C. Sow, C. Sene “Theoretical Study of Spectral Responses of Homojonctions Based on CuInSe2” Journal of Materials Science & Surface Engineering, Vol. 4 (4), 2016, pp392-399. |
[19] | S. B. Zhang, Su-Huai Wei, and Alex Zunger, “Stabilization of Ternary Compounds via Ordered Arrays of Defect Pairs”, Phys. Rev. Lett, 1997, vol. 78, 4059. |
[20] | Abazović Nadica D., Jovanović Dragana J., Stoiljković Milovan M., Mitrić Miodrag N., Ahrenkil Phillip S., Nedeljković Jovan M., Čomor Mirjana I., “Colloidal-chemistry based synthesis of quantized CuInS2/Se2 nanoparticles”, Journal of the Serbian Chemical Society, 2012, Volume 77, Pages: 789-797. |
[21] | R. Noufi, R. Axton, C. Herrington and S. K. Deb, “Electronic properties versus composition of thin films of CuInSe2”, Appl. Phys. Lett., Vol. 45, 1984, p. 668. |
[22] | P. Migliorato, J. L. Shay, H. M. Kasper and S. Wagner, “Analysis of the electrical and luminescent properties of CuInSe2”, J. AppI. Phys. Vol. 46, 1975, p. 1777. |
[23] | E. M. Keita, Y. Tabar, B. Ndiaye, A. A. Correa, C. Sene, B. Mbow, “Modeling and Analysis of the Effects of Surface and Interface States on the Photocurrent and the Efficiency of a Solar Cell Based on n+npp+ Structure”, Int. J. Adv. Sci. Eng. Vol. 8 No. 3, 2022, p. 2328-2340. https://doi.org/10.29294/IJASE.8.3.2022.2328-2340 |
[24] | Hisashi Yoshikawa, Sadao Adachi. 1997. Optical Constants of ZnO, Jpn. J. Appl. Phys. 36, 6237-6243. |
[25] | B. MBOW, A. MEZERREG, N. REZZOUG, and C. LLINARES, “Calculated and Measured Spectral Responses in Near-Infrared of III-V Photodetectors Based on Ga, In, and Sb”, phys. Stat. Sol. (a) 141, 511 (1994). |
[26] | H. J. HOVEL and J. M. WOODALL, “Ga1-xAlxAs - GaAs P-P-N Heterojunction Solar Cells”, J. Electrochem. Soc. 120, 1246 (1973). |
[27] | H. J. HOVEL and J. M. WOODALL, 10th IEEE Photovoltaic Specialists Conf., Palo Alto (Calif.) 1973 (p. 25). |
[28] | El Hadji Mamadou KEITA, 2017. Doctoral Thesis, Etude théorique de réponses spectrales de cellules solaires à base de CuInSe2: Modèles à 2 couches (p/n et n/p), à 3 couches (p/n/n+, p+/p/n, n/p/p+ et n+/n/p) et à 4 couches (p+/p/n/n+ et n+/n/p/p+), Université Cheikh Anta DIOP de Dakar, Sénégal P. 24-47. |
[29] | E. M. Keita, B. Mbow, C. Sene, ‘' Perovskites and other framework structure crystalline materials”, chap No 22: Framework structure materials in photovoltaics based on perovskites 3D”, OAJ Materials and Devices, vol 5 (2), (Coll. Acad. 2021), p. 637-708. DOI: 10.23647/ca.md20201511. |
[30] | Alain Ricaud, “Photopiles Solaires”, de la physique de la conversion photovoltaïque aux filières, matériaux et procédés. 1997, 1e édition, Presses polytechniques et universitaires romandes, p. 40. |
APA Style
El Hadji Mamadou Keita, Fallou Mbaye, Bachirou Ndiaye, Chamsdine Sow, Cheikh Sene, et al. (2022). Optimizing Structures Based on Chalcopyrite Materials for Photovoltaic Applications. American Journal of Energy Engineering, 10(3), 53-67. https://doi.org/10.11648/j.ajee.20221003.11
ACS Style
El Hadji Mamadou Keita; Fallou Mbaye; Bachirou Ndiaye; Chamsdine Sow; Cheikh Sene, et al. Optimizing Structures Based on Chalcopyrite Materials for Photovoltaic Applications. Am. J. Energy Eng. 2022, 10(3), 53-67. doi: 10.11648/j.ajee.20221003.11
@article{10.11648/j.ajee.20221003.11, author = {El Hadji Mamadou Keita and Fallou Mbaye and Bachirou Ndiaye and Chamsdine Sow and Cheikh Sene and Babacar Mbow}, title = {Optimizing Structures Based on Chalcopyrite Materials for Photovoltaic Applications}, journal = {American Journal of Energy Engineering}, volume = {10}, number = {3}, pages = {53-67}, doi = {10.11648/j.ajee.20221003.11}, url = {https://doi.org/10.11648/j.ajee.20221003.11}, eprint = {https://article.sciencepublishinggroup.com/pdf/10.11648.j.ajee.20221003.11}, abstract = {In this work we study the importance of optimizing the parameters of photoconductive layers to improve the efficiency of a photovoltaic cell. We compare the evolution of the performance of solar cells based on chalcopyrite materials by considering a non-decreasing band gap structure named model (a) based on the structure ZnO(n+)/CdS(n)/CuInSe2(p)/CuInS2(p+) and a decreasing band gap structure named model (b) based on the structure ZnO(n+)/CdS(n)/CuInS2(p)/CuInSe2(p+). The two structures are composed of 4 layers named respectively region 1, region 2, region 3 (base), region 4 (substrate); between regions 2 and 3 is located the space charge region (SCR) where exists a high electric field. The calculation of the external quantum efficiency of the cell and the short-circuit photocurrent density by numerical calculation are established by using the continuity equation of charge carriers and parameters such as the absorption coefficient, diffusion length which models the purity of the material, recombination velocities at the surface and at the interface which models their states, the thicknesses of the different layers, the solar irradiation. The results obtained applied to models (a) and (b), are presented in the form of tables and curves widely analyzed and commented. Considering first the same standard parameters, the model (a) whose absorption threshold is localized in the space charge region and the base, gives the best performance compared to model (b) whose absorption threshold is localized in the substrate. However, the optimization of the parameters, shows an improvement of the performances of the two models but above all a great evolution of the performances of the model (b) which external quantum efficiency becomes appreciably equal to that of the model (a). The short-circuit photocurrent density for solar spectra (AM0, AM1, AM1.5) evolves from (44.92 mA.cm-2; 33.031 mA.cm-2; 30.179 mA.cm-2) → (48.119 mA.cm-2; 35.155 mA.cm-2; 32.188 mA.cm-2) for the model (a), and evolves from (24.525 mA.cm-2; 19.309 mA.cm-2; 17.507 mA.cm-2) → (46.841 mA.cm-2; 34.303 mA.cm-2; 31.388 mA.cm-2) for the model (b).}, year = {2022} }
TY - JOUR T1 - Optimizing Structures Based on Chalcopyrite Materials for Photovoltaic Applications AU - El Hadji Mamadou Keita AU - Fallou Mbaye AU - Bachirou Ndiaye AU - Chamsdine Sow AU - Cheikh Sene AU - Babacar Mbow Y1 - 2022/07/12 PY - 2022 N1 - https://doi.org/10.11648/j.ajee.20221003.11 DO - 10.11648/j.ajee.20221003.11 T2 - American Journal of Energy Engineering JF - American Journal of Energy Engineering JO - American Journal of Energy Engineering SP - 53 EP - 67 PB - Science Publishing Group SN - 2329-163X UR - https://doi.org/10.11648/j.ajee.20221003.11 AB - In this work we study the importance of optimizing the parameters of photoconductive layers to improve the efficiency of a photovoltaic cell. We compare the evolution of the performance of solar cells based on chalcopyrite materials by considering a non-decreasing band gap structure named model (a) based on the structure ZnO(n+)/CdS(n)/CuInSe2(p)/CuInS2(p+) and a decreasing band gap structure named model (b) based on the structure ZnO(n+)/CdS(n)/CuInS2(p)/CuInSe2(p+). The two structures are composed of 4 layers named respectively region 1, region 2, region 3 (base), region 4 (substrate); between regions 2 and 3 is located the space charge region (SCR) where exists a high electric field. The calculation of the external quantum efficiency of the cell and the short-circuit photocurrent density by numerical calculation are established by using the continuity equation of charge carriers and parameters such as the absorption coefficient, diffusion length which models the purity of the material, recombination velocities at the surface and at the interface which models their states, the thicknesses of the different layers, the solar irradiation. The results obtained applied to models (a) and (b), are presented in the form of tables and curves widely analyzed and commented. Considering first the same standard parameters, the model (a) whose absorption threshold is localized in the space charge region and the base, gives the best performance compared to model (b) whose absorption threshold is localized in the substrate. However, the optimization of the parameters, shows an improvement of the performances of the two models but above all a great evolution of the performances of the model (b) which external quantum efficiency becomes appreciably equal to that of the model (a). The short-circuit photocurrent density for solar spectra (AM0, AM1, AM1.5) evolves from (44.92 mA.cm-2; 33.031 mA.cm-2; 30.179 mA.cm-2) → (48.119 mA.cm-2; 35.155 mA.cm-2; 32.188 mA.cm-2) for the model (a), and evolves from (24.525 mA.cm-2; 19.309 mA.cm-2; 17.507 mA.cm-2) → (46.841 mA.cm-2; 34.303 mA.cm-2; 31.388 mA.cm-2) for the model (b). VL - 10 IS - 3 ER -