Abstract:Alloying of Cu2ZnSnS4 (CZTS) with Ge can potentially promote grain growth and suppress the formation of Sn‐related defects. Herein, a two‐step fabrication route based on compound co‐sputtering and sulfurization at a high temperature is used to prepare Ge‐incorporated CZTS (Cu2ZnGexSn1 − xS4 [CZGTS]). For Cu2ZnGeS4 (CZGS), films deposited using elemental Ge and binary GeS targets are compared. The recrystallization is shown to be promoted for the absorbers deposited using Ge target, possibly due to lower sulfur… Show more
“…First, our results show that Ge-substitution does not affect polymorph preference (panel a) with kesterite being the groundstate polymorph (E Stannite À E Kesterite > 0 eV per formula unit) for all x Ge (see Table S5 in Section S4 of the ESI † for CZTS and CZGS wurtzite data). That Ge increases the relative stability of kesterite vs. stannite for all but dilute Ge-substitution is in general agreement with other theoretical work 59,121,122 and the experimental observation of enhanced grain growth in Ge-doped CZTSSe. [123][124][125] Recent scanning electron microscope images show that grain growth and crystallinity in CZTGS is not improved for x Ge > 0.2 121 but this could be due to suboptimal annealing conditions for each Ge composition during fabrication.…”
Section: Effect Of Ge-substitution In Cztssupporting
Kesterite solar cells, based on the prototypical absorber material Cu2ZnSnS4 (CZTS), are cheap, nontoxic, and chemically stable, thus rendering them promising, beyond-Si photovoltaic technologies. Their efficiencies, however, are limited by...
“…First, our results show that Ge-substitution does not affect polymorph preference (panel a) with kesterite being the groundstate polymorph (E Stannite À E Kesterite > 0 eV per formula unit) for all x Ge (see Table S5 in Section S4 of the ESI † for CZTS and CZGS wurtzite data). That Ge increases the relative stability of kesterite vs. stannite for all but dilute Ge-substitution is in general agreement with other theoretical work 59,121,122 and the experimental observation of enhanced grain growth in Ge-doped CZTSSe. [123][124][125] Recent scanning electron microscope images show that grain growth and crystallinity in CZTGS is not improved for x Ge > 0.2 121 but this could be due to suboptimal annealing conditions for each Ge composition during fabrication.…”
Section: Effect Of Ge-substitution In Cztssupporting
Kesterite solar cells, based on the prototypical absorber material Cu2ZnSnS4 (CZTS), are cheap, nontoxic, and chemically stable, thus rendering them promising, beyond-Si photovoltaic technologies. Their efficiencies, however, are limited by...
“…[ 29 ] Other example of such methodology applied to solar absorber alloys can be found in our earlier works. [ 30,31 ] The Brillouin‐zone integrations were performed using 3 × 2 × 2 Γ ‐centered Monkhorst–Pack grid [ 32 ] and a cutoff energy of 350 eV. The ionic force threshold for atomic relaxations was set to 0.01 eV Å −1 .…”
Figure 12. The corresponding a,c) EQE and b,d) J-V graphs of the CGSe sample with [Cu]/[III] ¼ 0.86 and 1.14, before and after sulfurization. The EQE of CGSe-Ref is not included in c), because it is zero for all wavelengths.
“…The Zn x Sn 1-x O y (ZTO) can be used as an alternative non-toxic substitute for the commonly used CdS buffer layer due to the possibility of band edge movement by either compositional change [21] or deposition temperature, [22] leading to reduced cliff-like alignment for CZGS absorbers (Figure 1). Moreover, the bandgap of CZGS [10,23] is comparable to CdS, [24] which results in significant parasitic absorption in the CdS. The wide bandgap ZTO [22] can reduce the parasitic short wavelength absorption loss compared with the CdS [24] buffer layer.…”
Section: Introductionmentioning
confidence: 99%
“…[7][8][9] We have previously reported the formation of a Ge-Sn gradient toward the rear interface of CZGTS absorbers made by sulfurizing a Cu 2 ZnGeS 4 (CZGS) layer buried underneath a CZTS layer. [10,11] Since the diffusion of Ge and Sn occurs faster through grain boundaries than grains, [10,12] the accumulation of Ge on absorber interfaces easily occurs during sulfurization, which modifies the bandgap energy at the interfaces. The importance of the conduction band offset (CBO) at the absorber and buffer interface is well established.…”
The Cu2ZnGe
X
Sn1‐X
S4 (CZGTS) thin‐film solar cells have a limited open‐circuit voltage (V
OC) due to bulk and interface recombination. Since the standard CdS buffer layer gives a significant cliff‐like conduction band offset to CZGTS, alternative buffer layers are needed to reduce the interface recombination. This work compares the performance of wide bandgap Cu2ZnGeS4 (CZGS) solar cells fabricated with nontoxic Zn
x
Sn1–x
O
y
(ZTO) buffer layers grown by atomic layer deposition under different conditions. The V
OC of the CZGS solar cell improved significantly to over 1 V by substituting CdS with ZTO. However, V
OC is relatively insensitive to ZTO bandgap variations. The short‐circuit current is generally low but is improved with KCN etching of the CZGS absorber before deposition of the ZTO buffer layer. A possible explanation for the device behavior is the presence of an oxide interlayer for nonetched devices.
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