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| Autores principales: | , , , , , , , , , , |
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| Formato: | Preprint |
| Publicado: |
2021
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| Materias: | |
| Acceso en línea: | https://arxiv.org/abs/2110.06555 |
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| _version_ | 1866911290447888384 |
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| author | Sood, Mohit Bombsch, Jakob Lomuscio, Alberto Shukla, Sudhanshu Lomuscio, Alberto Hartmann, Claudia Frisch, Johannes Bremsteller, Wolfgang Ueda, Shigenori Wilks, Regan G. Bär, Marcus Siebentritt, Susanne |
| author_facet | Sood, Mohit Bombsch, Jakob Lomuscio, Alberto Shukla, Sudhanshu Lomuscio, Alberto Hartmann, Claudia Frisch, Johannes Bremsteller, Wolfgang Ueda, Shigenori Wilks, Regan G. Bär, Marcus Siebentritt, Susanne |
| contents | Copper indium disulfide (CuInS$_2$) grown under Cu-rich conditions exhibits high optical quality but suffers predominantly from charge carrier interface recombination resulting in poor solar cell performance. An unfavorable cliff like conduction band alignment at the buffer/CuInS$_2$ interface could be a possible cause of enhanced interface recombination in the device. In this work, we exploit direct and inverse photoelectron spectroscopy together with electrical characterization to investigate the cause of interface recombination in Zn(O,S)/CuInS$_2$ devices. Temperature-dependent current-voltage analysis indeed reveal an activation energy of the dominant charge carrier recombination path, considerably smaller than the absorber bandgap, confirming the dominant recombination channel to be present at the Zn(O,S)/CuInS2 interface. However, photoelectron spectroscopy measurements indicate a small spike like conduction band offset of 0.1 eV at the Zn(O,S) CuInS$_2$ interface, excluding an unfavorable energy level alignment to be the prominent cause for strong interface recombination. The observed band bending upon interface formation also rules out Fermi level pinning as the main reason, leaving near-interface defects (as recently observed in Cu-rich CuInSe2)1 as the likely reason for the performance limiting interface recombination. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2110_06555 |
| institution | arXiv |
| publishDate | 2021 |
| record_format | arxiv |
| spellingShingle | Origin of interface limitation in CuInS$_2$ based solar cells Sood, Mohit Bombsch, Jakob Lomuscio, Alberto Shukla, Sudhanshu Lomuscio, Alberto Hartmann, Claudia Frisch, Johannes Bremsteller, Wolfgang Ueda, Shigenori Wilks, Regan G. Bär, Marcus Siebentritt, Susanne Applied Physics Materials Science Copper indium disulfide (CuInS$_2$) grown under Cu-rich conditions exhibits high optical quality but suffers predominantly from charge carrier interface recombination resulting in poor solar cell performance. An unfavorable cliff like conduction band alignment at the buffer/CuInS$_2$ interface could be a possible cause of enhanced interface recombination in the device. In this work, we exploit direct and inverse photoelectron spectroscopy together with electrical characterization to investigate the cause of interface recombination in Zn(O,S)/CuInS$_2$ devices. Temperature-dependent current-voltage analysis indeed reveal an activation energy of the dominant charge carrier recombination path, considerably smaller than the absorber bandgap, confirming the dominant recombination channel to be present at the Zn(O,S)/CuInS2 interface. However, photoelectron spectroscopy measurements indicate a small spike like conduction band offset of 0.1 eV at the Zn(O,S) CuInS$_2$ interface, excluding an unfavorable energy level alignment to be the prominent cause for strong interface recombination. The observed band bending upon interface formation also rules out Fermi level pinning as the main reason, leaving near-interface defects (as recently observed in Cu-rich CuInSe2)1 as the likely reason for the performance limiting interface recombination. |
| title | Origin of interface limitation in CuInS$_2$ based solar cells |
| topic | Applied Physics Materials Science |
| url | https://arxiv.org/abs/2110.06555 |