• 沒有找到結果。

Electrical and optical properties of ZnO:Al thin films grown by magnetron sputtering

N/A
N/A
Protected

Academic year: 2021

Share "Electrical and optical properties of ZnO:Al thin films grown by magnetron sputtering"

Copied!
4
0
0

加載中.... (立即查看全文)

全文

(1)

Electrical and optical properties of ZnO:Al thin films

grown by magnetron sputtering

Shr-Nan BaiÆ Tseung-Yuen Tseng

Received: 1 December 2007 / Accepted: 20 March 2008 / Published online: 17 April 2008

Ó Springer Science+Business Media, LLC 2008

Abstract The properties of transparent conductive ZnO:Al thin films grown by R.F. magnetron sputtering method are investigated. The working pressure (argon gas) is changed from 2.5 to 40.0 mTorr to study its influence on the characteristics of ZnO:Al thin films. The ZnO:Al thin films have better texture due to the increase in the surface mobility, which resulted from the increase in the mean free path of sputtering gas under lower working pressure. The microstructure of ZnO:Al films is found to be affected obviously by changing the working pressure. It is shown that the grain size of ZnO:Al thin films decreases with the increase of working pressure. The X-ray diffraction pat-terns indicate that the poor crystallized structure of ZnO:Al films is obtained at higher working pressure. Except 40 mTorr, the highly (002)-oriented ZnO:Al thin films can be found at the measured range of working pressure. Moreover, the growth rate of the films decreases from 1.5 to 0.5 nm/min as the working pressure increases from 2.5 to 40.0 mTorr. The results of optical transmittance mea-surement of ZnO:Al thin films reveal a high transmittance ([80%) in visible region and exhibit a sharp absorption edge at wavelength about 350 nm.

1 Introduction

The inexpensive and nontoxic zinc oxide (ZnO) based materials have attracted a lot of attentions as the trans-parent conductive material in recent years due to the extreme commercial interest in progressing flat panel dis-play, solar cell, and other different optoelectronic devices [1–5]. The ZnO-based materials are also promising for application as an ultraviolet and blue light emitter because of sufficiently large excitation binding energy of 60 meV, which is stable even at room temperature. There were many techniques employed to grow ZnO-based thin films, including magnetron sputtering [6,7], pulsed laser depo-sition [8], reactive electron-beam evaporation [9, 10], metalorganic chemical vapor deposition [11], metallic zinc oxidation [12], spray pyrolysis [13–15], and molecular beam epitaxy [16]. For all of these deposition techniques, sputtering technology is the most commonly used method because it can obtain good orientation and uniform thick-ness films at low substrate temperature or even on amorphous substrate. Krikorian et al. [17] have mentioned that three critical factors determining epitaxial growth in sputtering for a given material are background pressure, substrate temperature, and deposition rate. Under the var-ious growth conditions such as substrate temperature, annealing temperature, and various substrates, the growth of ZnO-based thin films has been widely investigated [18–

21]. However, the influence of working pressure on the electrical and optical characteristics of ZnO-based thin films is rarely found in the published literatures. In this investigation, a careful planning study of the effect of working pressure on the properties of R.F. magnetron sputtered ZnO:Al thin films is presented. The relationship between film characteristics and working pressure is also reported.

S.-N. Bai (&)

Department of Electronic Engineering, Institute of Electronic, Chienkuo Technology University, Changhua City 500, Taiwan, ROC

e-mail: snbai@ctu.edu.tw T.-Y. Tseng

Department of Electronics Engineering, Institute of Electronics, National Chiao-Tung University, Hsinchu City 300, Taiwan, ROC

e-mail: tseng@cc.nctu.edu.tw

123

J Mater Sci: Mater Electron (2009) 20:253–256

(2)

2 Experimental

The transparent conductive Al2O3-doped ZnO (ZnO:Al) films were grown on 1737F Corning glass substrate by R.F. magnetron sputtering system operating at room tempera-ture with a power of 50 W. The substrate was ultrasonically cleaned in acetone, alcohol, and D.I. water. A three-inch circular shape target of ZnO (purity, 99.99%) mixed with 2 wt.% Al2O3(purity, 99.99%) was employed. The sputtering chamber was evacuated to 8 9 10-6Torr through a mass flow controller. Then, the high purity Ar gas with pressure ranges varied from 2.5 to 40.0 mTorr was used to evaluate the influence of the working pressure on structural, electrical, and optical characteristics of the ZnO:Al thin films. Prior to the ZnO:Al films deposition, the pre-sputtering for 10 min was carried out in order to clean the target’s surface contamination.

The surface morphology and microstructure of the ZnO:Al films were studied using the high-resolution cold field emission scanning electron microscope (FE-SEM). The crystalline structure and orientation of the ZnO:Al thin films were analyzed by X-ray diffraction (XRD). The film thickness was determined from SEM images of the fracture cross-section area of the ZnO:Al films. The electrical resistivities were determined by the van der Pauw method. An electric current was applied through electrodes and each potential difference between the electrodes was measured. The electric resistivities were calculated from I–V curves by the least-squares method. The optical transmission spectra through the ZnO:Al thin films were recorded using an ultraviolet-visible spectrophotometer in the wavelength range of 200–800 nm.

3 Results and discussion

Figure1a and b shows the SEM micrographs of ZnO:Al thin films prepared at working pressure of 2.5 and 20.0 mTorr. It can be seen that the grain size of the films deposited at various working pressures is quite different. In Fig.1a and b, the grain size is decreased with an increase of working pressure. The higher working pressure may result in lower growth rate, smaller grain sizes and worse crystallinity. An increasing in working pressure can increase the sputtering rate and at the same time lower the energy of sputtered particles, and therefore as a result of the competing effects. The working pressure demonstrates a noticeable effect on the microstruc-ture of ZnO:Al thin films in this study. The sputtered materials possess a mean free path that is comparable to the distance in which from target to substrate at lower pressure. These arriving materials, at lower pressure, have much higher energy that results in higher surface mobility and thus a much larger possibility to form ZnO:Al thin films.

Figure2 demonstrates the growth rate of ZnO:Al films prepared with different working pressures. The average growth rate was calculated based on the mean value of thickness from the cross-section images of the thin films. It is found that the growth rate of the ZnO:Al films is quite sensitive to the working pressure of vacuum chamber. The growth rate is decreased with increasing of working pres-sure in the range from 2.5 to 40.0 mTorr. The decrease of growth rate with an increase of working pressure can be Fig. 1 SEM images of ZnO:Al thin films deposited at (a) 2.5 mTorr, (b) 20.0 mTorr 0.0 0.4 0.8 1.2 1.6 2.0 0

Working pressure (mTorr)

G row th r a te ( n m/ min) 45 40 35 30 25 20 15 10 5

Fig. 2 Growth rate of ZnO:Al thin films as a function of working pressure

254 J Mater Sci: Mater Electron (2009) 20:253–256

(3)

explained that the sputtered materials have no sufficiently energy due to the mean free path of the materials is smaller than the distance from target to substrate at higher pressure [22]. In addition, the collision probabilities of the depos-iting materials increase under higher working pressure; therefore, the sputtering rate decreases and results in the growth rate of ZnO:Al thin films decreases as the working pressure increases.

Figure3demonstrates the XRD patterns of ZnO:Al thin films deposited at working pressure of 2.5–40.0 mTorr. It is found that the intensity of the peaks is decreased with increasing of working pressure. All of the sputtered films exhibit preferential (002) orientation with c-axis perpen-dicular to the substrate surface, except the film prepared at 40 mTorr. Based on previous SEM and growth rate experimental results, the higher the working pressure, the thinner the ZnO films become. When the ZnO films are very thin, the lattice mismatches and crystal growth com-petition among the adjacent crystal islands will exist and these imperfections cause the intensity of (002) diffraction peak becomes weakened or even disappeared. The peak disappears at 40 mTorr of working pressure actually indi-cating that the microstructure of the film is amorphous. The ZnO:Al thin films deposited on glass substrate show only the (002) peak in the measured 2h region and no diffraction peaks from randomly oriented grains or other impurity phases are presented. Supposing a uniform strain across the deposited film, the size of the crystallites D in the grains can be estimated by the Scherrer’s formula [23]:

D¼ kk

B cos h

where k is the shape factor of the crystallite (expected shape factor is 0.9), k the X-ray wavelength, B the full width at half maximum (FWHM) of the (002) diffraction peak, and h the Bragg diffraction angle. The estimated values of the ZnO average grain size with working pres-sures of 2.5, 5, 10, and 20 mTorr are 19.8, 19.3, 15.4, and 12.2 nm, respectively.

Figure4shows the influence of working pressure on the electrical resistivity of the ZnO:Al thin films. It can be observed that the resistivity increases with an increase of working pressure. The resistivity is increased from 4.1 9 10-3to 5.2 9 10-1ohmcm as the working pressure is increased from 2.5 to 40.0 mTorr. The electrical resis-tivity is well known proportional to the reciprocal of the product of the carrier concentration and the mobility. Therefore, the variation in resistivity with working pressure maybe attributed to the change in carrier concentration and/ or mobility. ZnO is typically an n-type semiconductor in which has high conductivity mainly from stoichiometric deviation. The electrical conductivity of ZnO:Al films is higher than that of pure ZnO films because that the con-tribution from Al3+ions on substitutional sites of Zn2+ions acts as donor. Therefore, it can be reasonably suggested that the ZnO:Al films deposited under higher working pressure may have less carrier concentration causing the electrical conductivity of the ZnO:Al thin films lower. Besides, the ZnO:Al films are extremely chemically active. The chemisorption of oxygen atoms at the surface of ZnO:Al thin films may absorb electrons from the conduc-tion band and therefore reduces the carrier concentraconduc-tion and then broadens the depletion layers within the ZnO grain boundaries [24]. Additionally, it has been shown earlier that the growth rate is decreased with increasing of working pressure. The average grain size of the ZnO:Al films is smaller at a higher working pressure, which increases the grain-boundary scattering and thus decreases the mobility. Therefore, it can be summarized that the increase of electrical resistivity of ZnO:Al thin films with increasing working pressure is due to the decrease in the carrier concentration and mobility.

Figure5 demonstrates the optical transmission spectra of ZnO:Al films as a function of wavelength prepared at various working pressures. The average optical transmit-tance in the visible region is above 80% for all of the films and decreases with an increase in working pressure. According to the cross-section images of the ZnO:Al thin

0 500 1000 1500 2000 2500 30 35 40 45 50 55 60

Two theta (degree)

Intensity (a.u.) (a) (b) (c) (d) (e)

Fig. 3 X-ray diffraction spectra of ZnO:Al thin films deposited at various working pressures (a) 2.5 mTorr, (b) 5 mTorr, (c) 10 mTorr, (d) 20 mTorr, (e) 40 mTorr

1.E-03 1.E-02 1.E-01 1.E+00

Working pressure (mTorr)

R e sistivity ( o h m -c m) 0 5 10 15 20 25 30 35 40 45

Fig. 4 Electrical resistivity of ZnO:Al thin films as a function of working pressure

J Mater Sci: Mater Electron (2009) 20:253–256 255

(4)

films, the thickness of the films decreases as the working pressure is increased. The thickness of the ZnO:Al thin films with working pressure of 2.5, 5, 10, 20 and 40 mTorr is 164, 125, 95, 73, and 52 nm, respectively. At higher working pressures, the composition of the ZnO:Al becomes much nonstoichiometric and their grain sizes decrease. It results in the light scattering loss and the destruction of coherence between incident light and reflected light and therefore leads to the disappearance of interference fringes as well as the decrease in transmittance.

4 Conclusions

It is found that the structural, electrical, and optical properties of the sputtered ZnO:Al thin films depend on working pressure. The SEM observation shows that the grain size is decreased with an increase of working pressure. It implied that the growth rate decreases with increasing working pressure. This is attributed to the decrease in the surface mobility, which caused by the decrease in the mean free path of sputtering gas, under higher working pressure. The XRD results show that the ZnO:Al thin films deposited on glass substrate at different working pressures demonstrate only the (002) peak in the displayed 2h region. The study on the electrical resistivity of ZnO:Al films prepared at higher working pressures reveal that the films with smaller grain size have more grain-boundary scattering that lowers the electrical conductivity of the ZnO:Al films. Moreover, the chemisorption of oxygen atoms at the surface of ZnO:Al thin films is an another possible factor to affect the resistivity. The optical transmission studies demonstrate that the average optical transmittance in the visible region is above 80% for all of the films and decreases with an increase in working pressure.

Acknowledgements The authors appreciate the financial support from the National Science Council, Taiwan, Republic of China, under

Project Numbers NSC 95-2221-E-009-120 and NSC 95-2221-E-270-018. Mr. F. C. Chuang is thanked for his help in experimental works.

References

1. B.Y. Oh, M.C. Geong, T.H. Moon, W. Lee, J.M. Myoung, J.Y. Hwang, D.S. Seo, J. Appl. Phys. 99, 124505–124508 (2006) 2. Y.W. Zhu, H.Z. Zhang, X.C. Sun, S.Q. Feng, J. Xu, Q. Zhao, B.

Xiang, R.M. Wang, D.P. Yu, Appl. Phys. Lett. 83, 144–146 (2003). doi:10.1063/1.1589166

3. E. Hosono, S. Fujihara, I. Honma, H. Zhou, Adv. Mater. 17, 2091–2094 (2005). doi:10.1002/adma.200500275

4. B. Sang, A. Yamada, M. Konagai, Jpn. J. Appl. Phys. 37, L206– L208 (1998). doi:10.1143/JJAP.37.L206

5. D. Wang, C. Song, J. Phys. Chem. B 109, 12697–12700 (2005). doi:10.1021/jp0506134

6. A.N. Banerjee, C.K. Ghosh, K.K. Chattopadhyay, H. Minoura, A.K. Sarkar, A. Akiba, A. Kamiya, T. Endo, Thin Solid Films 496, 112–116 (2006). doi:10.1016/j.tsf.2005.08.258

7. X. Yu, J. Ma, F. Ji, Y. Wang, X. Zhang, C. Cheng, H. Ma, J. Cryst. Growth 274, 474–479 (2005). doi:10.1016/j.jcrysgro.2004. 10.037

8. J. PerrieI`re, E. Millon, W. Seiler, C. Boulmer-Leborgne, V. Craciun, O. Albert, J.C. Loulergue, J. Etchepare, J. Appl. Phys. 91, 690–696 (2002). doi:10.1063/1.1426250

9. R. Al Asmar, G. Ferblantier, F. Mailly, P. Gall-Borrut, A. Foucaran, Thin Solid Films 473, 49–53 (2005). doi:10.1016/ j.tsf.2004.06.156

10. H.Z. Wu, K.M. He, D.J. Qiu, D.M. Huang, J. Cryst. Growth 217, 131–137 (2000). doi:10.1016/S0022-0248(00)00397-3

11. B.P. Zhang, K. Wakatsuki, N.T. Binh, N. Usami, Y. Segawa, Thin Solid Films 449, 12–19 (2004). doi: 10.1016/S0040-6090(03)01466-4

12. A. Umar, S.H. Kim, Y.H. Im, Y.B. Hahn, Superlattices Micro-struc. 39, 238–246 (2006). doi:10.1016/j.spmi.2005.08.046 13. S.A. Studenikin, N. Golego, M. Cocivera, J. Appl. Phys. 83,

2104–2111 (1998). doi:10.1063/1.366944

14. A. Bougrine, A. El Hichou, M. Addou, J. Ebotheı`, A. Kachouane, M. Troyon, Mater. Chem. Phys. 80, 438–445 (2003). doi: 10.1016/S0254-0584(02)00505-9

15. M. Miki-Yoshida, F. Paraguay-Delgado, W. Estrada-Loı`pez, E. Andrade, Thin Solid Films 376, 99–109 (2000). doi: 10.1016/S0040-6090(00)01408-5

16. Z. Jin, T. Fukumura, M. Kawasaki, K. Ando, H. Saito, T. Sek-iguchi, Y.Z. Yoo, M. Murakami, Y. Matsumoto, T. Hasegawa, H. Koinuma, Appl. Phys. Lett. 78, 3824–3826 (2001). doi: 10.1063/1.1377856

17. E. Krikorian, R.J. Sneed, Astrophys. Space Sci. 65, 129–154 (1979). doi:10.1007/BF00643495

18. E.G. Fu, D.M. Zhuang, G. Zhang, W.F. Yang, M. Zhao, Appl. Surf. Sci. 217, 88–94 (2003). doi:10.1016/S0169-4332(03) 00523-3

19. V. Gupta, A. Mansingh, J. Appl. Phys. 80, 1063–1073 (1996). doi:10.1063/1.362842

20. C.H. Choi, S.H. Kim, J. Cryst. Growth 283, 170–179 (2005). doi: 10.1016/j.jcrysgro.2005.05.050

21. V. Srikant, D.R. Clarke, J. Appl. Phys. 81, 6357–6364 (1997). doi:10.1063/1.364393

22. N. Saito, Y. Igasaki, Appl. Surf. Sci. 169/170, 349–352 (2001). doi:10.1016/S0169-4332(00)00676-0

23. H.P. Klug, L.E. Alexander, X-Ray Diffraction Procedures for Polycrystalline and Amorphous Materials, 2nd edn. (Wiley-In-terscience, New York, 1974), pp. 687–690

24. S.N. Bai, T.Y. Tseng, J. Am. Ceram. Soc. 78, 2685–2689 (1995). doi:10.1111/j.1151-2916.1995.tb08041.x 0 20 40 60 80 100 200 Wavelength (nm) Tr an s m it ta n c e (%) (c) (b) (a) (e) (d) 900 800 700 600 500 400 300

Fig. 5 Optical transmittance spectra of ZnO:Al thin films deposited at various working pressures (a) 2.5 mTorr, (b) 5 mTorr, (c) 10 mTorr, (d) 20 mTorr, (e) 40 mTorr

256 J Mater Sci: Mater Electron (2009) 20:253–256

數據

Figure 1 a and b shows the SEM micrographs of ZnO:Al thin films prepared at working pressure of 2.5 and 20.0 mTorr
Figure 4 shows the influence of working pressure on the electrical resistivity of the ZnO:Al thin films
Fig. 5 Optical transmittance spectra of ZnO:Al thin films deposited at various working pressures (a) 2.5 mTorr, (b) 5 mTorr, (c) 10 mTorr, (d) 20 mTorr, (e) 40 mTorr

參考文獻

相關文件

Particularly, combining the numerical results of the two papers, we may obtain such a conclusion that the merit function method based on ϕ p has a better a global convergence and

 The nanostructure with anisotropic transmission characteristics on ITO films induced by fs laser can be used for the alignment layer , polarizer and conducting layer in LCD cell.

We investigate some properties related to the generalized Newton method for the Fischer-Burmeister (FB) function over second-order cones, which allows us to reformulate the

Microphone and 600 ohm line conduits shall be mechanically and electrically connected to receptacle boxes and electrically grounded to the audio system ground point.. Lines in

Montemor M F, Simoes A M, Carmezim M J, “ Characterization of Rare-earth Conversion Films Formed on the AZ31 Magnesium Alloy and Its Relation with Corrosion Protection” ,

Minami, ”Formation of Superhydrophobic Alumina Coating Films with High Transparency on Polymer Substrates by the Sol-Gel Method”, Journal of Sol-Gel Science and Technology, 26

Deformation twins did not exhibit in the samples tested at 250°C and the recrystallized grain with a grain size of about 2.3 µm was observed at the

In the respect of anti-reflection layer, we use optical simulation to calculate reflection of multilayer films with gradient-index, to find the best optical layer thickness with