Superlattices and Microstructures 103 (2017) 335e342 Contents lists available at ScienceDirect Superlattices and Microstructures journal homepage: www.elsevier.com/locate/superlattices Effect of deposition temperature on the properties of Cu2ZnSnS4 (CZTS) thin films S.A. Khalate a, R.S. Kate a, J.H. Kim b, S.M. Pawar c, *, R.J. Deokate a, ** a Vidya Pratishthan’s, Arts Science and Commerce College, Baramati, 413 133, MS, India Chonnam National University, Gawanju, Seoul, South Korea c Dongguk University, Seoul, South Korea b a r t i c l e i n f o a b s t r a c t Article history: Received 31 January 2017 Accepted 3 February 2017 Available online 4 February 2017 Cu2ZnSnS4 (CZTS) thin films were deposited viva spray pyrolysis technique at different substrate temperature. The effect of substrate temperature on the structural, morphological, compositional and optical properties was reported. The X-ray diffraction and Raman analysis revealed that prepared CZTS thin film show kesterite phase without any secondary phases. Moreover, these analyses indicated the internal compressive stress relaxed with substrate temperature for all CZTS thin films. The homogeneous nature of CZTS thin films were observed from surface morphology and chemical composition study. The optical study provided good optical absorption (104 cm1) in the visible region and band gap energy was decreased and found quite close to the optimum value of about 1.57 eVe1.49 eV for solar cell application. © 2017 Elsevier Ltd. All rights reserved. Keywords: Cu2ZnSnS4 Thin film Spray Raman Optical properties 1. Introduction Kesterite Cu2ZnSnS4 (CZTS) semiconductor has attracted world-wide attention due to its excellent optical and electronic properties comparable to traditional Cu(In,Ga)Se2 (CIGS) and CdTe materials for thin film solar cells while consisting of earthabundant and low-toxic constituent elements. Literature survey shows that, due to most favorable band gap energy (1.5 eV), the large absorption coefficient over 104 cm1 in the visible solar spectrum and a p-type conductivity of copper-based quaternary semiconductors have attracted much attention in photovoltaic application [1e3]. These properties stimulate CZTS as a potential candidate for absorber in thin film solar cells. Thus, great efforts have been made for the fabrication of CZTS thin films in order to develop eco-friendly solar cells with high efficiency and low-cost technology [4e6]. CZTS thin films can be prepared by numerous techniques which include sputtering [7,8], thermal evaporation [9], electrospinning process [10], pulsed laser deposition [11], electron-beam-evaporated precursors [12,13], electrodeposition [14], co-evaporation [15] or by vacuum free chemical methods such as spray-pyrolysis [16,17], photochemical deposition [18,19] and solegel [20]. However, few studies have been devoted to CZTS deposition by spray pyrolysis [21,22] and it is observed that the properties of prepared films are intensely dependent on the deposition method and conditions of the films. * Corresponding author. ** Corresponding author. E-mail addresses: [email protected] (S.M. Pawar), [email protected], [email protected] (R.J. Deokate). http://dx.doi.org/10.1016/j.spmi.2017.02.003 0749-6036/© 2017 Elsevier Ltd. All rights reserved. 336 S.A. Khalate et al. / Superlattices and Microstructures 103 (2017) 335e342 In the present investigation, we have made an attempt to synthesize CZTS thin films by spray with various substrate temperatures. The structural, morphological and optical properties of CZTS thin films are studied and relative study supported to the substrate temperature. 2. Experimental 2.1. Preparation of CZTS thin films The spray pyrolysis method was used to deposit the CZTS thin films using the mixture of an aqueous solutions of cupric chloride (AR Grade 99.99%) 0.025 M, zinc chloride (AR Grade 99.99%) 0.025 M, stannic chloride (AR Grade 99.99%) 0.025 M and thiourea (AR Grade 99.99%) 0.2 M. The solutions were mixed in different composition ratios then sprayed on to glass substrate at various temperature (300e375 C) using SPD technique with flow rate 3 ml/min to achieve uniform and well adhesive CZTS thin films. Air was used as a carrier gas. Additional sintering of this thin film was not carried out [23]. It was observed that for higher temperature (>350 C) degradation of films occurred, which was probably due to with excess temperature. 2.2. Characterization techniques The structural characterization of these thin film samples was carried out using Bruker AXS D8 X-Ray Diffractometer (XRD), with CuKa radiation (l ¼ 1.54 Å) and Renishaw InVia Raman Microscope in the range of 10e80 and micro-Raman spectrometer JobineYvon LabRAM HR 800UV with the excitation by 514.5 nm photons of 20 mW Argon ion laser from spectra physics. The surface morphology and chemical composition were studied using field emission scanning electron microscope (FE-SEM) SU8000, Hitachi. Perkin Elmer Lambda 1050 UVeViseNIR spectrophotometer used to study optical properties. 3. Results and discussion 3.1. EDAX study Fig. 1 shows the composition variation of spray deposited CZTS thin films prepared at different substrate temperatures. The CZTS thin films deposited at substrate temperatures from 300 to 375 C were close to the stoichiometric ratio. The relative compositions of CZTS thin films were Cu-poor and Zn-rich (i.e. Cu/(Zn þ Sn) < 1 and Zn/Sn > 1) to all substrate temperature. To get stoichiometric results by spray method are very difficult to the quaternary compound films and similar results were found to the other studies [24e26]. Table 1 also shows the atomic percent of the CZTS thin deposited at different substrate temperature. With increasing substrate temperature the compositional ratios of sulfur content is slightly increased means sulfur vacancies are reduces and hence crystalline quality of CZTS thin films improved. However, at higher substrate temperature Sn and Zn elements are volatile; and the effect leads to the Cu-rich state. Due to volatile property more losses of Zn is found in all CZTS thin films. Thus, the atomic percentage of copper, zinc, tin and sulfur are well dependent on substrate temperature [27]. atomic percentage (%) 48 44 40 Cu Zn Sn S 36 32 28 24 20 16 12 8 290 300 310 320 330 340 350 360 370 380 o Substrate temperature ( C) Fig. 1. Variation of chemical composition of CZTS thin films for different substrate temperature. S.A. Khalate et al. / Superlattices and Microstructures 103 (2017) 335e342 337 3.2. Xeray diffraction studies The XRD patterns of spray deposited CZTS thin films deposited at different substrate temperatures (300, 325, 350 and 375 C) are shown in Fig. 2 and prepared CZTS samples are polycrystalline nature with kesterite phase with substrate temperature [28]. The diffraction peaks at angles 2q ¼ 28.49, 47.40 and 56.25 correspond to diffraction planes (112), (220) and (312), respectively [29] for all samples. Besides, as-prepared thin films might have a complete synthesization without post-annealing. The intensity and full width at half maximum (FWHM) of (112) peak showed strong and narrow behavior with good crystallinity. Fig. 3 gives the relative intensity and full width at half maximum (FWHM) of the (112) peak with respect to substrate temperature for CZTS films. The relative intensity of the (112) peak continuously increased and FWHM is decreased with substrate temperature. However, at high substrate temperature (>350 C), the (112) peak intensity dramatically decreased, shows the weak in crystallinity. Additionally, the lattice parameters of CZTS thin film prepared from 300 C to 375 C are similar as the other reports [17,21,22]. The lattice parameters have been found to be a ¼ 5.42 Å and c ¼ 10.84 Å, which give a value of c/2a ¼ 0.99. As the value of c/2a is close to 1 showed the unit cell is tetragonal and enlarged to different substrate temperature. With the increase of temperature from 300 C to 375 C, the crystallite size increased from 5 to 14 nm, and decreased the values 7 nm at 375 C substrate temperature. Table 2 shows the microstructural properties of the CZTS thin films deposited to various substrate temperature. The (hkl) and d-values of CZTS thin films are agree well with the values found in the JCPDS card [29]. The crystallite size of the films, calculated using Scherrer’s formula [30]. D¼ 0:9l bcosq (1) where D is the crystallite size, b is the broadening of the diffraction line measured at half of its maximum intensity (rad) (FWHM) and l the X-ray wavelength (1.5418 Å). The prepared CZTS films are polycrystalline in nature. The stresses are one of the most important critical factors affecting on the structural properties which changes geometric mismatch at boundaries between crystalline lattices of thin films and substrate [31]. The microstrains (3 ) are developed in the thin films, and calculated from the following relation [32]. 3 ¼ bcosq (2) 4 The variation of micro structural parameters like microstrain and stacking fault probability to all CZTS samples are shown in Fig. 4. The value of the interplanar spacing has been increased and internal microstrain relaxation in CZTS thin films is decreased. The microstrain relaxation is consistent with the expansion of the interplanar spacing of (112) plane and internal microstrain induces the formation of defect center [33,34]. However, this internal microstrain could be relaxed at the higher substrate temperature and deposited at low temperature CZTS thin films may be present smaller amounts of defects. The dislocation density (d) and stacking fault probability (a) of the CZTS thin films are estimated by the following equations [35,36]. d¼ a¼ 1 (3) D2 2p2 pffiffiffi Dð2qÞ 45 3tanq (4) Fig. 5 shows the variation of crystallite size (D) and dislocation density (d) of CZTS thin films. The dislocation density decreased from value 3.8 1016 lines/m2 to value 0.56 1016 lines/m2 and again reached to the value 1.7 1016 lines/m2. The minimum values are obtained to the CZTS thin film prepared at 350 C substrate temperature. The value of dislocation density gives the amount of defects in the CZTS thin film, the maximum value of (D) obtained for the CZTS thin film prepared at 350 C substrate temperature confirms the good crystallinity. Table 1 The atomic percent of CZTS thin films deposited for different substrate temperature. Substrate temperature ( C) Cu/(Zn þ Sn) Zn/Sn Metal/S 300 325 350 375 0.75 0.76 0.75 0.88 1.45 1.34 1 1.19 1.40 1.36 1.31 1.42 S.A. Khalate et al. / Superlattices and Microstructures 103 (2017) 335e342 o 375 C Intensity (A.U.) 312 220 112 338 o 350 C o 325 C o 300 C 20 30 40 50 60 70 80 2θ (Degree) 0.028 2800 0.026 2600 0.024 2400 0.022 2200 0.020 2000 0.018 1800 0.016 1600 0.014 0.012 1400 0.010 1200 0.008 1000 300 320 340 360 Intensity (arb. unit) FWHM (deg.) for (112) Fig. 2. X-ray diffraction patterns of CZTS films deposited for different substrate temperature. 380 o SubstrateTemperature ( C) Fig. 3. The FWHM values and relatively peak intensity of (112) diffraction peak of CZTS for different substrate temperature. 3.3. Raman spectroscopy of CZTS thin film Fig. 6 shows the recorded Raman spectra to all the prepared CZTS thin films. All spectra exhibited single Raman peak at 328 cm1 which is good indication of the kesterite phase of prepared CZTS thin films. Further, there is no any evidence of binary phases like SnS, SnS2, CuS, Cu2S and b-ZnS from Raman spectra [37]. 3.4. Surface morphology of CZTS thin film Fig. 7 shows the FE-SEM images of CZTS thin films to all substrate temperatures. The surface morphology is strongly dependent on the substrate temperature. The morphological studies shows that films deposited at 300 C have absence of S.A. Khalate et al. / Superlattices and Microstructures 103 (2017) 335e342 339 Table 2 The Micro structural properties of CZTS thin films deposited for different substrate temperature. Substrate temp. C hkl Diffraction angle 2q (deg.) Intensity d(obs.) (nm) FWHM (rad.) Crystallite size D (nm) Micro-strain (3 ) (103 lines2 m4) Dislocation density (d) (1016 lines/m2) Stacking fault 300 112 220 312 112 220 312 112 220 312 112 220 312 28.458 47.699 56.103 28.502 47.402 56.302 28.502 47.404 56.3 28.492 47.302 56.202 1086 448 330 1919 823 558 2797 1146 741 1777 560 414 3.1339 1.9051 1.638 3.1291 1.9163 1.6327 3.1292 1.9161 1.6327 3.1302 1.9201 1.6354 0.0223463 0.0271958 0.017951 0.0145137 0.01631 0.017061 0.00942 0.01043 0.010885 0.0131007 0.016572 0.014078 6.398664 4.661183 4.31457 9.255724 7.780842 7.162945 14.260595 14.510397 11.226644 2.60347 9.130281 11.161062 5.415112 6.218438 3.9605527 3.516838 3.73358 3.6707 2.282528 2.387554 2.399368 3.17453 3.795013 3.104616 2.44243 4.60265 5.37186 1.16729 1.65176 1.94902 4.91728 4.74943 7.93414 1.47535 1.19959 8.02766 0.0729069 0.2102407 0.035645 0.0289164 0.040383 0.0586877 0.0289164 0.0415349 0.0577436 0.0389018 0.0173482 0.0113828 325 350 375 6 5 3.1275 o d-spacing (A ) -3 Micro-Strain (×10 ) 3.1300 3.1250 4 3.1225 3 3.1200 3.1175 2 3.1150 300 320 340 360 380 o SubstrateTemperature ( C) Fig. 4. The variation of interplanar spacing and strain of CZTS thin film for different substrate temperature. well-defined grains. The CZTS thin film deposited at higher temperature (>300 C) has observed the dense structure with large grains. The average size determined from FE-SEM studies approximately found 50e100 nm to the CZTS thin film deposited at 350 C substrate temperature. The enhancement in crystalline quality in the CZTS thin film due to well decomposition and agglomeration of the neighboring crystallites at the higher substrate temperature [38]. The improvement of the grain size of CZTS thin films is consistent with the X-ray diffraction and Raman spectrum analyses. The large grains with less grain boundaries are beneficial for the devices performance due to less chance for the recombination of photogenerated carriers at the grain boundaries [39]. 3.5. Optical properties of CZTS thin film The optical transmittance spectra of the CZTS thin films were measured to resolve the values of band gap (Eg). The band gap values are determined by extrapolating the straight line to (ahn)2 versus photo energy (hn) curve with the intercept on horizontal photon energy axis, is shown in Fig. 8 [40,41]. The determined Eg values of CZTS thin films at 300, 325, 350, and 375 C are 1.57, 1.55, 1.49, and 1.52 eV, respectively. The obtained values are greater at lower substrate temperature due to the effect of internal compressive stress [34]. The internal compressive stress releases at higher temperature and the relaxations of internal compressive stress, crystal lattice expand subsequently diminish the band gaps of the thin films [42,43]. XRD and 340 S.A. Khalate et al. / Superlattices and Microstructures 103 (2017) 335e342 6 5 2 12 δ , X1016 (lines/cm ) Crystallite Size (nm) 14 4 10 3 8 2 6 1 4 0 300 320 340 360 380 o Substrate Temperature ( C) Fig. 5. Crystallite size and dislocation density of CZTS thin film for different substrate temperature. Raman spectra results confirm the internal compressive stress relaxation. The electronic transition from valence band to conduction band becomes easy due to the decrease in the possibility of the scattering of electron at grain boundaries, results the decrease of Eg. In addition, the CZTS thin film deposited at 350 C gives the relatively optimum band gap value (1.49 eV). 4. Conclusions In summary, polycrystalline Cu2ZnSnS4 (CZTS) absorber thin films have been deposited using spray pyrolysis technique with kesterite phase. The XRD and Raman results reveal that the formation of single phase CZTS with kesterite structure and the crystalline sizes depends upon substrate temperature. The interplanar spacing and internal microstrain relaxation denoted changes in CZTS thin film with temperature. The surface morphological study indicated that with increasing substrate temperature, the film crystallinity is improved. The optical absorption data reveal that the CZTS film has an optical bandgap of 1.59 eV. The thin film deposited at 350 C substrate temperature shows the suitable structural, morphological and optical properties for solar cell application. 300 0C 325 0C 350 0C 375 0C 500 nm Fig. 6. Surface FE-SEM images of CZTS thin film for different substrate temperature. 341 328 S.A. Khalate et al. / Superlattices and Microstructures 103 (2017) 335e342 Intensity (A.U.) 328 o 375 C 328 o 350 C 328 o 325 C o 300 C 100 200 300 400 500 600 700 800 -1 Raman Shift (cm ) Fig. 7. Raman spectra of CZTS thin films for different substrate temperature. 2 0 1.0 2 (α hν ) , (ev/cm) 2 1.5 300 C 0 325 C 0 350 C 0 375 C 0.5 0 1.35 1.40 1.45 1.50 1.55 1.60 1.65 1.70 1.75 hν ( eV) Fig. 8. Plot of (ahn)2 versus the photon energy (hn) of CZTS thin films for different. 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