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Photovoltaic Device with over 5% Efficiency Based on an n-Type Ag2ZnSnSe4 Absorber

Journal Article · · Advanced Energy Materials
 [1];  [2];  [3];  [3];  [3];  [3];  [3];  [2];  [3]
  1. IBM T J Watson Research Center, Yorktown Heights, NY (United States); DOE/OSTI
  2. University of California, San Diego, CA (United States)
  3. IBM T J Watson Research Center, Yorktown Heights, NY (United States)
The kesterite material Cu2ZnSn(S,Se)4 (CZTSSe) is an attractive earth–abundant semiconductor for photovoltaics. However, the power conversion efficiency is limited by a large density of I–II antisite defects, which cause severe band tailing and open–circuit voltage loss. Ag2ZnSnSe4 (AZTSe) is a promising alternative to CZTSSe with a substantially lower I–II antisite defect density and smaller band tailing. AZTSe is weakly n–type, and this study reports for the first time on how the carrier density is impacted by stoichiometry. Here, this study presents the first–ever photovoltaic device based on AZTSe, which exhibits an efficiency of 5.2%, which is the highest value reported for an n–type thin–film absorber. Due to the weakly n–type nature of the absorber, a new architecture is employed (SnO:F/AZTSe/MoO3/ITO) to replace conventional contacts and buffer materials. Using this platform, it is shown that the band tailing parameter in AZTSe more closely resembles that of CIGSe than CZTSSe, underscoring the strong promise of this absorber. In demonstrating the ability to collect photogenerated carriers from AZTSe, this study paves the way for novel thin–film heterojunction architectures where light absorption in the n–type device layer can supplement absorption in the p–type layer as opposed to producing a net optical loss.
Research Organization:
International Business Machines Corp., Armonk, NY (United States)
Sponsoring Organization:
USDOE; USDOE Office of Energy Efficiency and Renewable Energy (EERE)
Grant/Contract Number:
EE0006334
OSTI ID:
1533062
Alternate ID(s):
OSTI ID: 1401226
Journal Information:
Advanced Energy Materials, Journal Name: Advanced Energy Materials Journal Issue: 22 Vol. 6; ISSN 1614-6832
Publisher:
WileyCopyright Statement
Country of Publication:
United States
Language:
English

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Cited By (15)

New Earth-Abundant Thin Film Solar Cells Based on Chalcogenides journal April 2019
Progress and Perspectives of Thin Film Kesterite Photovoltaic Technology: A Critical Review journal February 2019
Cation Substitution in Earth-Abundant Kesterite Photovoltaic Materials journal January 2018
Synergistic Effects of Double Cation Substitution in Solution-Processed CZTS Solar Cells with over 10% Efficiency journal October 2018
Suppressed Deep Traps and Bandgap Fluctuations in Cu 2 CdSnS 4 Solar Cells with ≈8% Efficiency journal October 2019
Structural characterization of off-stoichiometric kesterite-type Cu 2 ZnGeSe 4 compound semiconductors: from cation distribution to intrinsic point defect density journal January 2018
Candidate photoferroic absorber materials for thin-film solar cells from naturally occurring minerals: enargite, stephanite, and bournonite journal January 2017
The role of Ag in aqueous solution processed (Ag,Cu) 2 ZnSn(S,Se) 4 kesterite solar cells: antisite defect elimination and importance of Na passivation journal January 2018
Metal@I 2 –II–IV–VI 4 core–shell nanocrystals: controlled synthesis by aqueous cation exchange for efficient photoelectrochemical hydrogen generation journal January 2018
Wide band gap kesterite absorbers for thin film solar cells: potential and challenges for their deployment in tandem devices journal January 2019
Heterovalent Ga 3+ doping in solution-processed Cu 2 ZnSn(S,Se) 4 solar cells for better optoelectronic performance journal January 2020
Analysis of loss mechanisms in Ag 2 ZnSnSe 4 Schottky barrier photovoltaics journal May 2017
Structural, electrical, and optical properties of Ag 2 ZnSnSe 4 for photodetection application journal January 2019
Emerging inorganic solar cell efficiency tables (Version 1) journal July 2019
Doping and alloying of kesterites journal August 2019

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