Nian
Cheng
*a,
Weiwei
Li
a,
Zhenyu
Xiao
b,
Han
Pan
a,
Dingshan
Zheng
a and
Wen-Xing
Yang
*a
aSchool of Physics and Optoelectronic Engineering, Yangtze University, Jingzhou 434023, China. E-mail: chengnian@foxmail.com; wenxingyang2@126.com
bEnergy-Saving Building Materials Collaborative Innovation Center of Henan Province, Xinyang Normal University, 237 Nanhu Road, Xinyang 464000, China
First published on 20th November 2024
Cu2ZnSnS4 (CZTS) and Cu2ZnGeS4 (CZGS) nanoparticles are important inorganic hole transport layers (HTLs) for carbon electrode-based perovskite solar cells (C-PSCs). However, the performances of the corresponding C-PSCs are still not satisfactory, which mainly originates from the un-optimized photo-electronic properties of the pristine CZTS and CZGS nanoparticles. Herein, composition engineering via alloying CZTS and CZGS is used to optimize the photo-electronic properties of the resulting CZGxT1−xS HTLs (x = 0, 0.25, 0.50, 0.75, and 1.0), and when combined with a FA1−xMAxPbI3−yBry active layer, the performance of the C-PSCs was greatly increased. The optimum HTL of CZG0.5T0.5S exhibits a suitable conduction band energy barrier at the perovskite/CZG0.5T0.5S interface, and thus, charge carrier recombination at the perovskite/CZG0.5T0.5S interface is effectively suppressed. However, the CZG0.5T0.5S HTL exhibited much greater conductivity, which efficiently transported the holes from the perovskite to a carbon electrode. This resulted in C-PSCs with the CZG0.5T0.5S HTL demonstrating a champion power conversion efficiency of 19.8%.
C-PSCs can be fabricated with a hole transport layer (HTL)-free structure or a traditional sandwich structure with a suitable HTL.1,4 Compared with the HTL-free C-PSCs, C-PSCs with a HTL can provide greater flexibility to regulate the interfaces between perovskite films and carbon electrodes. Therefore, C-PSCs with HTLs usually exhibit more satisfactory PCEs in comparison to HTL-free C-PSCs. For instance, C-PSCs with Spiro-OMeTAD HTLs have demonstrated a state-of-the-art PCE of 22.07% as reported by Shi et al., which greatly narrows the PCE difference between C-PSCs and traditional metal electrode-based PSCs.5,6 However, Spiro-OMeTAD is quite expensive and exhibits relatively low thermal stability, which hinders the potential for industrialization of this type of C-PSC.
Inorganic Cu-based HTLs, which have been reviewed in detail in previous publications, can function as potential HTLs for C-PSCs.7–9 The merits of Cu-based HTLs, such as low cost and excellent chemical stability, can be incorporated into high-performance C-PSCs, which are prerequisites for the industrialization of PSCs. In our previous studies, we showed that C-PSCs with Cu2ZnSnS4 (CZTS) HTLs can provide the highest PCE of 17.76%.10 Composition engineering of CZTS was subsequently conducted by completely replacing the elemental Sn in the CZTS with elemental Ge, and the resulting Cu2ZnGeS4 (CZGS) acting as a HTL further promoted the PCE of C-PSCs to 18.02%.11 These two studies demonstrated that CZTS and CZGS are promising inorganic HTLs for C-PSCs. However, the reported PCEs for the corresponding C-PSCs with CZTS or CZGS HTLs are still not satisfactory, which might originate from the un-optimized photo-electronic properties of the hot-injection-synthesized CZTS or CZGS nanoparticles.
Sn and Ge are chemical elements from the fourth main group with similar ionic radii, and therefore, continuous Cu2ZnGexSn1−xS4 (CZGxT1−xS) alloy compounds can be formed with the Ge concentration varying from 0.0 to 1.0.12,13 With increasing Ge concentration, the band gap of the CZGxT1−xS alloy can be monotonously increased from 1.5 eV to 2.0 eV, with concomitant increase in the electrical conductivity of the CZGxT1−xS films.12,14 Therefore, the alloyed CZGxT1−xS compounds exhibit superior photo-electronic properties compared with the pure CZTS and CZGS, which can effectively promote the PCEs of CZGxT1−xS-based kesterite solar cells.13 We speculate that the alloyed CZGxT1−xS compound with superior photo-electronic properties could be a potential HTL for C-PSCs. However, thus far, there have been no experimental studies focusing on composition engineering of CZTS or CZGS HTLs for C-PSCs.
Herein, alloyed CZGxT1−xS nanoparticles are synthesized using a modified heating method adapted from previous studies. The composition of CZGxT1−xS is engineered by varying the Ge concentrations (x = 0, 0.25, 0.50, 0.75, and 1.0). C-PSCs using a FA1−xMAxPbI3−yBry active layer together with these CZGxT1−xS nanoparticle HTLs are fabricated, and their PCEs are closely related to the composition of the CZGxT1−xS HTLs. The highest PCE of 19.8% is demonstrated in C-PSCs with a CZG0.5T0.5S HTL, which confirms that CZGxT1−xS is a highly prospective HTL for C-PSCs, and a composition engineering strategy for the CZTS or CZGS HTL is a feasible method to further promote the performance of C-PSCs.
From the X-ray diffraction (XRD) patterns in Fig. 1a and ESI Fig. S1,† the CZGxT1−xS nanoparticles exhibit a kesterite structure with four typical XRD peaks at approximately 28.5°, 33.0°, 47.6°, and 56.5°.14,16,17 With increasing Ge concentrations, the XRD peaks slightly shift towards higher angles. The ionic radius of Ge4+ (0.53 Å) is smaller than that of Sn4+ (0.69 Å), and therefore, substitution of Sn4+ with Ge4+ would result in shrinkage of the crystal lattice.12 The specific positions of the three major diffraction peaks of the CZGxT1−xS samples are tabulated in ESI Table S1.† The corresponding lattice constants are also calculated and presented in Table S1.† The obtained lattice constants for CZTS (a = 5.48 Å, c = 10.79 Å) and CZGS (a = 5.35 Å, c = 10.70 Å) agree quite well with those from previous reports,18,19 while the lattice constants for CZG0.5T0.5S are between those of CZTS and CZGS.
Fig. 1 (a) XRD patterns and (b) Raman spectra for CZGxT1−xS samples. TEM morphologies of (c) CZTS, (d) CZG0.5T0.5S, and (e) CZGS samples. |
The CZTS and CZGS nanoparticles demonstrate typical Raman peaks in Fig. 1b at 334.8 cm−1 and 349.1 cm−1, respectively, which are consistent with previously reported Raman shifts for CZTS and CZGS samples.12,20 The CZG0.5T0.5S sample exhibits a Raman peak of 338.5 cm−1, which is located between the Raman peaks of CZTS and CZGS. This observation is consistent with previous reports, which have demonstrated that the main Raman peaks of the CZGxT1−xS samples are blueshifted with increasing Ge concentrations.12,14 No extra Raman peaks were detected in the three CZGxT1−xS samples, which confirms that our CZGxT1−xS nanoparticles are pure kesterite with tetragonal structures.
The morphologies and dispersibility of the CZGxT1−xS samples are presented in the TEM images in Fig. 1c–e. All the nanoparticles are roughly spherical, with particle sizes smaller than 20 nm. These nanoparticles show excellent dispersibility without any agglomeration, which is beneficial for forming well-dispersed nanoparticle ink and ensures the formation of uniform and compact CZGxT1−xS nanoparticle HTLs above the perovskite films. High-resolution TEM (HRTEM) characterizations of the CZGxT1−xS nanoparticles are presented in ESI Fig. S2.† The lattice distances of the CZGxT1−xS nanoparticles are estimated to be 3.33–3.13 Å from the lattice fringes, which correspond to the (112) crystal planes of the CZGxT1−xS nanoparticles and slightly decrease with increasing Ge concentrations.
The XPS survey spectra of the CZGxT1−xS nanoparticles are given in ESI Fig. S3.† The Cu, Zn, Ge, Sn, and S peaks are clearly detected, while Sn 3d and Ge 2p peaks are absent in the CZGS and CZTS nanoparticles, respectively. The exact compositions of the CZGxT1−xS nanoparticles are determined using Energy dispersive X-ray spectroscopy (EDS) and summarized in ESI Table S2.† The atomic ratios of Cu, Zn, Ge, Sn, and S are slightly different from their stoichiometric ratio, and this has been widely observed for CZTS and CZGS nanoparticles. However, the atomic ratios of Ge/(Ge + Sn) are 0.0, 0.22, 0.51, 0.74, and 1.0, which agree quite well with their nominal compositions.
The planar morphology of the FA1−xMAxPbI3−yBry perovskite film from a two-step deposition method is presented in Fig. S4†.21–23 Perovskite crystals with well-defined grain boundaries are clearly visible. The CZGxT1−xS nanoparticle HTLs are prepared via spin-coating the CZGxT1−xS nanoparticle ink and annealing at 100 °C in an ambient atmosphere.
The planar morphologies of the CZGxT1−xS nanoparticle HTLs are presented in Fig. 2a–c and ESI Fig. S5.† Clearly, the rough perovskite surface is planarized after the deposition of the CZGxT1−xS nanoparticle HTL, which is a prerequisite for the intimate contact with the subsequently blade-coated carbon electrode. Additionally, all three CZGxT1−xS nanoparticle HTLs are uniform without any obvious cracks or pinholes that could effectively separate the perovskite film from the carbon electrode. Thus, the carrier recombination at the C-PSCs can be suppressed, and superior PCEs can be demonstrated in our study. The compact and uniform characteristics of the CZGxT1−xS nanoparticle HTL are further demonstrated in the cross-sectional images in Fig. 2d–f. The CZGxT1−xS nanoparticles are completely and intimately capped on the perovskite films, and the HTLs exhibit film thicknesses of approximately 120 nm.
Fig. 2 Planar and cross-sectional SEM images of (a and d) CZTS, (b and e) CZG0.5T0.5S, and (c and f) CZGS HTLs. |
C-PSCs utilizing these CZGxT1−xS (x = 0, 0.25, 0.50, 0.75, and 1.0) nanoparticles as HTLs are fabricated according to our previous reports,10,11 and the photovoltaic performances are evaluated and summarized in Fig. 3a–d and Table S3.† Clearly, all the photovoltaic parameters, i.e., Voc, Jsc, FF, and PCE, are closely related to the composition of the CZGxT1−xS HTLs. The two reference CZTS and CZGS HTLs contributed to the C-PSCs with moderate average PCEs of 16.2% and 17.2%, respectively, which are consistent with the results from our previous reports.10,11 In contrast, the alloyed CZGxT1−xS HTLs (x = 0.25, 0.50, and 0.75) resulted in C-PSCs with greatly enhanced PCEs. The highest average PCE is 19.6%, which is demonstrated in C-PSCs with CZG0.5T0.5S as a HTL.
The champion C-PSCs with CZGxT1−xS HTLs are further studied. The corresponding J–V curves and the photovoltaic parameters of C-PSCs with the CZG0.5T0.5S HTL together with the reference CZTS and CZGS HTLs are presented in Fig. 4a and Table 1. The J–V curves of the C-PSCs with CZG0.25T0.75S and CZG0.75T0.25S HTLs are presented in ESI Fig. S6.† The highest PCEs for C-PSCs with CZTS and CZGS HTLs are 16.8% and 17.7%, respectively. When the alloyed CZG0.25T0.75S, CZG0.5T0.5S, and CZG0.75T0.25S nanoparticles are utilized as HTLs, the corresponding PCEs are greatly boosted to 18.6%, 19.8%, and 18.6% respectively. The enormously increased Voc (Voc = 1.138 V) compared with the two reference CZTS (Voc = 1.042 V) and CZGS (Voc = 1.084 V) HTLs is primarily responsible for the highest PCE for the corresponding C-PSC with CZG0.5T0.5S as the HTL, although the corresponding Jsc and FF are also slightly enhanced for the CZG0.5T0.5S HTL.
Fig. 4 (a) J–V curves, (b) stable output curves, (c) IPCE spectra, and (d) device stability for the champion C-PSCs with CZTS, CZG0.5T0.5S, and CZGS HTLs. |
V oc (V) | J sc (mA cm−2) | FF (%) | PCE (%) | |
---|---|---|---|---|
CZTS-reverse | 1.042 | 23.00 | 70.11 | 16.8 |
CZTS-forward | 1.038 | 22.92 | 69.69 | 16.6 |
CZG0.5T0.5S-reverse | 1.138 | 24.10 | 72.04 | 19.8 |
CZG0.5T0.5S-forward | 1.140 | 24.10 | 71.05 | 19.5 |
CZGS-reverse | 1.084 | 23.44 | 69.54 | 17.7 |
CZGS-forward | 1.073 | 23.44 | 67.75 | 17.0 |
The PCEs from the reverse and forward scan measurements are only slightly different, which indicates that the J–V hysteresis phenomenon is negligible in our C-PSCs with CZGxT1−xS HTLs. The steady-state PCEs were also evaluated under standard AM 1.5 G illumination in Fig. 4b. The average output current densities are 19.65 mA cm−2, 20.59 mA cm−2, and 21.10 mA cm−2 for C-PSCs with CZTS, CZGS, and CZG0.5T0.5S HTLs, respectively. Correspondingly, the steady-state PCEs are 16.3%, 17.6%, and 19.2%, respectively, which agree quite well with the PCE values from the reversed J–V measurements.
The current densities extracted from the IPCE spectra in Fig. 4c are 22.67 mA cm−2, 23.15 mA cm−2, and 23.89 mA cm−2 for C-PSCs with CZTS, CZGS, and CZG0.5T0.5S HTLs, respectively, which are also consistent with those from J–V measurements. The stability of the C-PSCs with the CZGxT1−xS (x = 0, 0.5, and 1.0) HTLs is further evaluated in an ambient atmosphere with humidity at approximately 30%. Without capsulation, C-PSCs with the CZTS, CZGS, and CZG0.5T0.5S HTLs demonstrated excellent storage stability with negligible PCE decay after 30 days, as shown in Fig. 4d. This phenomenon was also demonstrated in our previous studies, and is attributed to the waterproof capability and excellent chemical stability of the CZGxT1−xS HTLs and the carbon electrode.10,11,15,24,25
The device structure of our C-PSCs is schematically depicted in Fig. 5a, which consists of fluorine-doped tin oxide (FTO), SnO2 electron transport layer (ETL), perovskite layer, CZGxT1−xS HTL, and carbon electrode in sequence. The ultraviolet photoelectron spectroscopy (UPS) spectra of CZTS, CZG0.5T0.5S, and CZGS are provided in Fig. S7.† The Fermi levels are determined to be −4.68 eV, −4.64 eV, and −4.77 eV for CZTS, CZG0.5T0.5S, and CZGS HTLs, respectively, and the corresponding valence band positions are calculated to be −5.23 eV, −5.23 eV, and −5.22 eV, respectively. The optical band gaps of CZTS, CZG0.5T0.5S, and CZGS are estimated using Tauc plots from the UV-vis absorbance, as shown in Fig. S8,† and the corresponding band gaps are 1.55 eV, 1.72 eV, and 1.85 eV, respectively. Therefore, the conduction band positions of CZTS, CZG0.5T0.5S, and CZGS are −3.68 eV, −3.51 eV, and −3.37 eV, respectively.
Fig. 5 (a) Schematic device structure and (b) energy band alignment for our C-PSCs. (c) PL and (d) TRPL spectra for perovskite/CZGxT1−xS (x = 0, 0.5, and 1.0) films. |
According to first principles calculations, the valence band maximum of CZGxT1−xS mainly consists of Cu-d and S-p orbitals, whereas conduction band minimum consists of Ge or Sn-s orbitals and S-s orbitals. Thus, when more Ge is incorporated into CZGxT1−xS, the valence band maximum is nearly the same, while the conduction band minimum is significantly upshifted.26 The energy band alignment of our C-PSCs is depicted in Fig. 5b. The valence band of the CZGxT1−xS HTL is positioned between those of perovskite and the carbon electrode, and thus, a gradient energy band alignment is formed at the perovskite/CZGxT1−xS/carbon interface, which will facilitate hole transportation from the perovskite film to the carbon electrode. The conduction band energy barrier at the perovskite/CZGxT1−xS interface is enlarged from 0.42 eV for pure CZTS to 0.73 eV for pure CZGS.
The smallest conduction band energy barrier (0.42 eV) for the perovskite/CZTS interface might not be sufficiently large to effectively inhibit the backward electron transfer from the perovskite to CZTS HTL, and thus, moderate charge carrier recombination at the perovskite/CZTS interface continues to exist. When Ge is alloyed into CZTS, the obtained CZGxT1−xS (x = 0.5 and 1.0) HTL exhibits an enlarged optical band gap. Therefore, the conduction band energy barrier for perovskite/CZGxT1−xS could be increased, which could contribute to largely suppressed charge carrier recombination at the perovskite/CZGxT1−xS interface. Thus, a superior Voc and PCE for the C-PSCs with CZGxT1−xS (x = 0.5 and 1.0) HTLs are observed in our study.
The photoluminescence (PL) spectra of the perovskite/CZGxT1−xS films are presented in Fig. 5c. For the reference perovskite film without the CZGxT1−xS HTL, a characteristic PL peak at approximately 790 nm was observed. When CZGxT1−xS HTLs are capped onto the perovskite films, the PL intensities are enormously quenched, which originates from the fast hole transfer from perovskite to the CZGxT1−xS HTL due to the suitable energy band alignment at the perovskite/CZGxT1−xS interface.27,28
The magnified PL spectra of the perovskite/CZGxT1−xS films are further presented in the inset of Fig. 5c. Clearly, the perovskite/CZG0.5T0.5S film demonstrates the lowest PL intensity, indicating that the CZG0.5T0.5S HTL exhibits superior hole extraction capability compared with the reference CZTS and CZGS HTLs. This idea is further confirmed by the time-resolved photoluminescence (TRPL) spectra in Fig. 5d. The average decay time for perovskite film is 250.5 ns, which is enormously decreased to 40.1–56.0 ns after a CZGxT1−xS HTL is deposited onto the perovskite film (the details are summarized in Table S4†). Among the three CZGxT1−xS HTLs, CZG0.5T0.5S contributed the shortest average decay time compared with the other two reference CZTS and CZGS HTLs.27–29
Conductivity values of the CZGxT1−xS HTLs are estimated from their current density–voltage (J–V) curves using a FTO/CZGxT1−xS/carbon device and presented in Fig. 6a. The calculated conductivity values are 2.93 × 10−4 S m−1, 5.80 × 10−4 S m−1, and 4.17 × 10−4 S m−1 for the CZTS, CZG0.5T0.5S, and CZGS HTLs, respectively, after fitting the linear part of the J–V curves between 0.0 V and 0.5 V. The carrier mobilities of the CZGxT1−xS HTLs were estimated using Mott–Gurney equation J = 9ε0εμV2/(8L3), where μ denotes the hole mobility. After fitting the linear part of J1/2 V curves between 0.5 V and 1.0 V in ESI Fig. S9,† the hole mobilities are calculated to be 2.30 × 10−4 cm2 V−1 s−1, 4.27 × 10−4 cm2 V−1 s−1, and 3.14 × 10−4 cm2 V−1 s−1 for CZTS, CZG0.5T0.5S, and CZGS HTLs, respectively.
Previous studies have also demonstrated that Ge-doped CZTS exhibited superior hole mobilities,12,14 which are consistent with our observations and could partially contribute to the enhanced conductivity of the CZG0.5T0.5S HTL. It is also likely that the enlarged CZG0.5T0.5S crystal sizes in Fig. 1c–e could be a possible contributor to the enhanced conductivity and mobility of the corresponding CZG0.5T0.5S HTL. Therefore, the CZG0.5T0.5S HTL, which exhibited the highest conductivity, could transport the holes from the perovskite film to the carbon electrode in the most efficient manner compared with CZTS and CZGS HTLs, which might contribute to the highest Jsc values in the C-PSCs with CZG0.5T0.5S HTLs.
The built-in potential plays a vital role in the dissociation of photo-generated carriers and their transportation towards the ETL and HTL. The built-in potentials are evaluated to be 0.91 V, 0.93 V, and 1.01 V for the C-PSCs with the CZTS, CZGS, and CZG0.5T0.5S HTLs, respectively, as shown in Fig. 6b. The largest built-in potential in C-PSCs with the CZG0.5T0.5S HTL would contribute to the most efficient carrier dissociation and transportation towards the ETL and HTL, which also contributes to the highest Jsc and Voc in the corresponding C-PSCs.30–32 The dark current of the C-PSCs with CZGxT1−xS HTLs (x = 0, 0.5, and 1.0) is presented in Fig. 6c. The highest built-in potential in C-PSCs and hole mobility associated with the CZG0.5T0.5S HTL facilitated the most efficient hole transportation across the HTL, and thus, carrier accumulation at the perovskite/HTL interface is elevated. However, the CZG0.5T0.5S HTL ensures a sufficiently large energy barrier at the conduction band of the perovskite/CZG0.5T0.5S interface, which effectively suppressed the charge carrier recombination. Therefore, the C-PSC with the CZG0.5T0.5S HTL exhibited the smallest dark current due to its lowest charge carrier recombination rate in the C-PSC.33,34
After fitting the electrochemical impedance spectroscopy (EIS) spectra at 1.0 V in the dark with the corresponding equivalent circuit in Fig. 6d, the recombination resistances for C-PSCs are calculated to be 2687 Ω, 3914 Ω, and 5637 Ω for the CZTS, CZGS, and CZG0.5T0.5S HTLs, respectively. Clearly, the C-PSC with the CZG0.5T0.5S HTL exhibits the largest recombination resistance, which further confirmed that the charge carrier recombination rate in the corresponding C-PSC is the lowest among the three CZGxT1−xS (x = 0, 0.5, and 1.0) HTLs.32,35
Footnote |
† Electronic supplementary information (ESI) available: the Experimental section, XRD patterns, HRTEM images, XPS spectra, planar SEM image, champion J–V curves, UPS spectra, Tauc plots, and Tables S1–S4 are provided. See DOI: https://doi.org/10.1039/d4ta07106a |
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