Enhancement of output performance of Cu2ZnSnS4 thin film solar cells—A numerical simulation approach and comparison to experiments
The formation of stable, low resistance and nonrectifying contacts to Cu2ZnSnS4 (CZTS) thin film photovoltaic material are the major and critical challenges associated with its effect over the output performance of fabricated solar cells. The solution of continuity equation in one dimension for a so...
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Published in | Physica. B, Condensed matter Vol. 407; no. 21; pp. 4391 - 4397 |
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Main Authors | , |
Format | Journal Article |
Language | English |
Published |
Kidlington
Elsevier B.V
01.11.2012
Elsevier |
Subjects | |
Online Access | Get full text |
ISSN | 0921-4526 1873-2135 |
DOI | 10.1016/j.physb.2012.07.042 |
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Summary: | The formation of stable, low resistance and nonrectifying contacts to Cu2ZnSnS4 (CZTS) thin film photovoltaic material are the major and critical challenges associated with its effect over the output performance of fabricated solar cells. The solution of continuity equation in one dimension for a soda lime glass substrates (SLG) |Mo | CZTS | CdS | ZnO:Al cell structure is considered in the simulation of its current–voltage characteristics that is governed by the back contact material, acceptor concentration as well as thickness of the CZTS layer. Our primary simulation shows a 6.44% efficiency of the CZTS solar cell which is comparable to reported experimental data if these parameters are not optimized. However, by optimizing them a simulated conversion efficiency as high as 13.41% (Voc=1.002V, Jsc=19.31mA/cm2, fill factor (FF)=69.35%) could be achievable. The solar cell with a back contact metal work function of 5.5eV, an absorber layer's thickness of 2.68μm and an acceptor concentration of 5×1016cm−3 were optimum. The presented optimization is ideal and subject to experimental verification with a precise control of the process parameters along with reduced surface as well as bulk recombination, secondary phases and thermalization losses. |
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Bibliography: | ObjectType-Article-1 SourceType-Scholarly Journals-1 ObjectType-Feature-2 content type line 23 |
ISSN: | 0921-4526 1873-2135 |
DOI: | 10.1016/j.physb.2012.07.042 |