2020
DOI: 10.1002/adma.202000121
|View full text |Cite
|
Sign up to set email alerts
|

Device Postannealing Enabling over 12% Efficient Solution‐Processed Cu2ZnSnS4 Solar Cells with Cd2+ Substitution

Abstract: Kesterite Cu2ZnSnS4 is a promising photovoltaic material containing low‐cost, earth‐abundant, and stable semiconductor elements. However, the highest power conversion efficiency of thin‐film solar cells based on Cu2ZnSnS4 is only about 11% due to low open‐circuit voltage and fill factor mainly caused by antisite defects and unfavorable heterojunction interface. In this work, a postannealing procedure is proposed to complete a Cd‐alloyed Cu2ZnSnS4 device. The postannealing to complete the device significantly e… Show more

Help me understand this report

Search citation statements

Order By: Relevance

Paper Sections

Select...
2
1
1
1

Citation Types

0
115
0

Year Published

2021
2021
2022
2022

Publication Types

Select...
8

Relationship

2
6

Authors

Journals

citations
Cited by 240 publications
(126 citation statements)
references
References 69 publications
0
115
0
Order By: Relevance
“…In general, the C – V is sensitive to the interface traps. [ 6,44 ] With the incorporation of Ga, the N C – V became closer to the Hall results, implying the interface traps (i.e., Cu Zn antisite defect) were eliminated to some extent. The N C – V then achieved a minimum value of 3.91 × 10 16 cm −3 when the R Ga was 7.5%, while the W d increased from 0.213 µm ( R Ga = 0) to a maximum of 0.416 µm ( R Ga = 7.5%).…”
Section: Resultsmentioning
confidence: 76%
“…In general, the C – V is sensitive to the interface traps. [ 6,44 ] With the incorporation of Ga, the N C – V became closer to the Hall results, implying the interface traps (i.e., Cu Zn antisite defect) were eliminated to some extent. The N C – V then achieved a minimum value of 3.91 × 10 16 cm −3 when the R Ga was 7.5%, while the W d increased from 0.213 µm ( R Ga = 0) to a maximum of 0.416 µm ( R Ga = 7.5%).…”
Section: Resultsmentioning
confidence: 76%
“…Kesterite semiconductors, including Cu 2 ZnSnS 4 (CZTS), Cu 2 ZnSnSe 4 (CZTSe), and Cu 2 ZnSn(S,Se) 4 (CZTSSe), are ideal absorber materials for thin film solar cells due to their earth abundant elemental composition and high theoretical efficiency [ 1–5 ] compared to similarly structured chalcopyrite counterpart Cu(In,Ga)Se 2 (CIGS). However, the power conversion efficiency (PCE) of kesterite solar cells is only 12.6%, [ 6,7 ] far lower than that of CIGS, which has reached 23.35%.…”
Section: Introductionmentioning
confidence: 99%
“…However, the CZTSSe efficiency record is only 12.6% whereas the efficiency of CIGS solar cell has recently reached 23.35% [4][5][6]. Recently, people have indeed borrowed some strategies from CIGS to improve the performance of CZTSSe solar cells [2,[7][8][9][10][11][12][13][14][15]. For example, alkali metal doping of CIGS can improve the crystallinity of the absorber [16,17], reduce the density of point defects and increase the P-type carrier concentration [18,19].…”
Section: Introductionmentioning
confidence: 99%