2012
DOI: 10.1063/1.4726042
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Admittance spectroscopy of Cu2ZnSnS4 based thin film solar cells

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Cited by 82 publications
(70 citation statements)
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“…When heating with a fast heating rate (above 2.6 K s -1 ), which leads to formation of larger grains, the films show increased conductivity, with an average of 2.5 ×10 -2 Ω -1 cm -1 (average from 14 samples). This value is comparable with conductivities observed for CZTS films prepared by sulfurization of metallic precursors [39], which is an approved method for fabrication of CZTS solar cells [40][41][42]. Above a heating rate of 2.6 K s -1 no systematic dependency on the heating rate could be observed.…”
Section: Resultssupporting
confidence: 84%
“…When heating with a fast heating rate (above 2.6 K s -1 ), which leads to formation of larger grains, the films show increased conductivity, with an average of 2.5 ×10 -2 Ω -1 cm -1 (average from 14 samples). This value is comparable with conductivities observed for CZTS films prepared by sulfurization of metallic precursors [39], which is an approved method for fabrication of CZTS solar cells [40][41][42]. Above a heating rate of 2.6 K s -1 no systematic dependency on the heating rate could be observed.…”
Section: Resultssupporting
confidence: 84%
“…Figure 8 shows the Cole-Cole plot for cell S10 for voltage bias ranging -1 mV to -544 mV. Figure 9 presents the equiva- lent circuits that were used to adjust the experimental admit-tance data [31]. The simplest circuit, M1, corresponds to a device characterized by a series resistance, Rs, and a parallel capacitance and resistance, Cj and Rj, respectively.…”
Section: Impedance Spectroscopymentioning
confidence: 99%
“…The precursor deposition was carried out by dc magnetron sputtering and sulfurization by thermal annealing in a sulfur vapour atmosphere [6,7]. In order to make accurate transport measurements and to avoid any possible influence of the generally observed MoS x layer at the Mo/CZTS interface [5], the CZTS thin film studied here was deposited directly on the SLG substrate. However, the morphology, chemical composition, crystalline structure, as well as optical properties of this sample are similar to those prepared using the Mo layer.…”
Section: Sample Preparationmentioning
confidence: 99%
“…the CZTS absorber layer and the Mo back contact have been pointed out as factors that reduce the solar cell efficiency [4,5]. Strong research efforts have been made in the study of different CZTS synthesis routes [3][4][5][6][7][8][9][10], CZTS structural and optical properties [2,[6][7][8], as well as in the development of CZTS solar cells [3-5, 9, 10].…”
Section: Introductionmentioning
confidence: 99%