Influence of annealing temperature on the phase composition and optical properties of CuInS2 films

https://doi.org/10.1016/j.mssp.2013.03.015Get rights and content

Abstract

We studied the growth of CuInS2 thin films by single-source evaporation of CuInS2 powder in a high-vacuum system with a base pressure of 10−3 Pa. After evaporation, the films were annealed in a sulfur atmosphere at temperatures from 200 to 500 °C for 1 h. XRD curves and Raman spectra of the films demonstrated that chalcopyrite CuInS2 was the major crystalline phase. The morphology of CuxS exhibited a star-like structure, which we report for the first time. The phase composition and optical properties of our polycrystalline thin films were effectively modified by annealing in S. For films annealed at 200 and 350 °C, a secondary CuIn11S17 phase appeared, which may be related to solid-state reaction in the S atmosphere. This secondary CuIn11S17 phase has not been widely reported in previous studies. After annealing at 500 °C, only a chalcopyrite phase was detected, with bandgap energy of 1.46 eV, which is nearly identical to the optimal bandgap energy (1.5 eV) of single-crystal CuInS2. This indicates that the composition of the CuInS2 film annealed at 500 °C was nearly stoichiometric. The bandgap of the samples first increased and then decreased with increasing annealing temperature, which may be attributed to an increase in grain size, the secondary CuIn11S17 phase, and deviation from stoichiometry.

Introduction

Chalcopyrite thin-film solar cells are already being used in the rapidly growing photovoltaics market. In particular, the ternary compound CuInS2 has potential for high conversion efficiency owing to its high absorption coefficient of approximately 105 cm−1 and its direct bandgap of 1.5 eV [1], which matches well to the solar spectrum. Furthermore, no high toxic component was included in this compound semiconductor. However, the efficiency of CuInS2 solar cells has only reached 12.2% [2], which is much lower than that of other analogous chalcopyrite thin-film solar cells (CuInSe2). To improve the efficiency of CuInS2 solar cells, a variety of methods have been used to deposit CuInS2 thin films, including wet chemical routes [3], rapid thermal processes [4], co-evaporation of elemental sources [5], sulfurization of metallic precursor films [6], chemical vapor deposition [7], sputtering [8], electro-deposition [9], and spray pyrolysis [10], [11]. Some groups have used thermal evaporation of a single source (CuInS2 powder) to prepare thin films. Akaki et al. prepared Sb-doped CuInS2 thin films by single-source thermal evaporation and studied their structural and electrical–optical properties [12]. They obtained polycrystalline CuInS2 thin films after annealing at >200 °C. The Sb-doped CuInS2 thin films were close to stoichiometry compared to nondoped CuInS2 thin films. Abaab et al. deposited CuInS2 thin films by single-source vacuum thermal evaporation of a substrate submitted to a longitudinal thermal gradient [13]. Some of the films were annealed in a sulfur atmosphere and converted to homogeneous CuInS2 layers. The optical bandgap of the films after sulfurization was 1.5 eV, which is close to the optimal value for photovoltaic energy conversion. Rabeh et al. prepared CuInS2 films by single-source thermal evaporation and post-growth treatment at 100–350 °C in air [14]. For annealing temperatures >200 °C, the n-type conductivity was stable and the resistance correlated well with the annealing temperature. Zribi et al. studied the optical properties of sodium-doped CuInS2 thin films grown by single-source evaporation [15]. They observed that the optical bandgap decreased with increasing sodium concentration. The refractive index and extinction coefficient also depended on the sodium concentration. The same group grew Na-doped and Sn-doped CuInS2 thin films by double source thermal evaporation using CuInS2 powder and the doping element [16], [17], [18]. The doped films were annealed at 250–500 °C under vacuum. The structure, morphological, and optical properties of the films were studied by XRD and UV-Vis-NIR spectroscopy. The change in bandgap for doped samples annealed at 250–500 °C was discussed in detail.

For device applications it is important to know the structure and optical properties of CuInS2. As our source material we used a bulk CuInS2 polycrystalline ingot grown by the vertical Bridgman method. CuInS2 thin films were prepared by the single-source thermal evaporation method. The films were then annealed at 200–500 °C for 60 min in a sulfur atmosphere. The effects of annealing temperature on the phase composition and optical properties of the films are discussed.

Section snippets

Experiments

A bulk CuInS2 polycrystalline ingot was grown by the vertical Bridgman method. Stoichiometric amounts of Cu, In and S with a nominal purity of at least 99.999% were mixed together and sealed in a quartz tube under vacuum. To avoid explosion induced by excessive sulfur vapor pressure, the quartz tube was heated slowly at 20 °C/h. Complete homogenization was obtained by keeping the melt at 1100 °C for approximately 24 h. Then the tube was cooled at a rate of 7 °C/h. The resulting ingot was crushed

Results and discussion

Fig. 1 shows the XRD pattern and Raman spectrum for the polycrystalline CuInS2 ingot. The XRD pattern reveals that only the chalcopyrite CuInS2 phase was present in the ingot (comparison with standard PDF card #27–0159). The inset in Fig. 1a is a magnification of the XRD pattern from 53° to 57°. It is well known that the chalcopyrite and spharelite (disordered zinc-blende structure) phases exhibit differences in XRD pattern. One difference is the splitting of some peaks associated with

Conclusion

CuInS2 is a good absorber material for photovoltaic applications and much effort has been devoted to studies of the fundamental properties of CuInS2 for successful device fabrication. In the present study, CuInS2 thin films were deposited by single-source evaporation of CuInS2 powder from a crushed ingot. The films were annealed in a sulfur atmosphere at temperatures from 200 to 500 °C for 1 h. XRD and Raman results demonstrated that chalcopyrite CuInS2 was the major crystalline phase. The phase

Acknowledgements

This work was supported by the Program for Changjiang Scholars, Innovative Research Team in University (No. IRT0739), Shanghai Leading Academic Disciplines (S30107), the National Natural Science Foundation of China (Nos. 60906043 and 51102162) and the Shanghai Natural Science Foundation (09ZR1409200). We would like to thank the Analysis and Testing Center in Shanghai University for SEM and EDS measurements.

References (26)

  • R. Klenk et al.

    Thin Solid Films

    (2005)
  • K. Siemer et al.

    Sol. Energy Mater. Sol. Cells

    (2001)
  • P. Guha et al.

    Sol. Energy Mater. Sol. Cells

    (2003)
  • H. Rodriguez-Alvarez et al.

    J. Cryst. Growth

    (2008)
  • J. Álvarez-García et al.

    Thin Solid Films

    (2000)
  • K. Muller et al.

    Thin Solid Films

    (2004)
  • M.H.C. Jin et al.

    Mater. Sci. Eng. B

    (2005)
  • R. Cayzac et al.

    Mater. Sci. Eng. B

    (2009)
  • R. Garuthara et al.

    Sol. Energy Mater. Sol. Cells

    (2003)
  • I. Oja et al.

    Thin Solid Films

    (2005)
  • Y. Akaki et al.

    J. Phys. Chem. Solids

    (2003)
  • M. Abaab et al.

    Sol. Energy Mater. Sol. Cells

    (1999)
  • M.B. Rabeh et al.

    Thin Solid Films

    (2007)
  • Cited by (8)

    • Morphology and phase-controlled growth of CuInS<inf>2</inf> nanoparticles through polyol based heating up synthesis approach

      2021, Materials Science in Semiconductor Processing
      Citation Excerpt :

      Regarding the above mentioned, In(acac)3 is suitable for making nanoparticle ink. It should be mentioned that annealing is an essential process in the production of thin films with high quality, even when the vacuum-based deposition technique is applied [17,62]. Excessively large particles prevent the formation of smooth and uniform layers.

    • Characterization of calcined CuInS<inf>2</inf>nanocrystals prepared by microwave-assisted synthesis

      2017, Journal of Alloys and Compounds
      Citation Excerpt :

      Up to now, CuInS2 materials have been produced by several different methods, such as sputtering [2], spray pyrolysis [3,4], molecular beam epitaxy [5,6], sulfurization, successive ionic layer adsorption and reaction [7,8], evaporation [9,10]. Some important developing results of solar cells based on CuInS2 have been made in the past several years to carry out that there are three possible structures, including the chalcopyrite (CH) phase, CuAu (CA) phase, and CuPt (CP) phase, but CH and CA phases are usually observed at room temperature to be stable phases and coexisted in the produced CuInS2 material due to the low formation energies [11–15]. As we have known that the CA phase is involved with the decreasing of grain size but the increasing of defects in grains, and further with degradation of the solar cell efficiency [16,17].

    • Morphology-controlled growth of special nanostructure CuInS<inf>2</inf> thin films on an FTO substrate and their application in thin film solar cells

      2015, International Journal of Hydrogen Energy
      Citation Excerpt :

      However, the highest laboratorial efficiency is only 13% [4], and it is limited by its light-collection and recombination losses in space-charge regions. To improve the efficiency of the CIS solar cells, a variety of methods have been used to deposit CIS thin films, including cryogenic mechanical milling [5], chemical bath deposition [6], electrodeposition [7], evaporation [8], paste coating technologies [9], magnetron sputtering [10], microwave irradiation [11,12] and solvothermal method [13–19]. Up to date, controllable synthesis for CIS thin films with various nanostructures has drawn significant attention.

    View all citing articles on Scopus
    View full text