版權所有 翻印必究 Effects of annealing on structure, resistivity and transmittance of Ga doped ZnO films 教授 : 林克默博士 學生 : 董祐成 日期 :2011/3/8 2015/12/161 STUT 太陽能材料與模組實驗室.

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版權所有 翻印必究 Effects of annealing on structure, resistivity and transmittance of Ga doped ZnO films 教授 : 林克默博士 學生 : 董祐成 日期 :2011/3/8 2015/12/161 STUT 太陽能材料與模組實驗室

版權所有 翻印必究 Outline Introduction Experimental Result and Discussion Conclusion 2015/12/16 STUT 太陽能材料與模組實驗室 2

版權所有 翻印必究 Introduction In this paper the authors has reported the effects of annealing temperature and atmosphere on the electrical resistance and optical transmittance of GZO thin films prepared by radio frequency (RF) magnetron sputtering. Annealing effects in the annealing temperature range up to 600uC were investigated to understand the effects of thermal energy and annealing atmosphere on the electrical and optical properties of GZO films better, 2015/12/16 STUT 太陽能材料與模組實驗室 3

版權所有 翻印必究 although annealing at such high temperatures are not allowed in most TCO applications. 2015/12/16 STUT 太陽能材料與模組實驗室 4

版權所有 翻印必究 Experimental GZO thin films were deposited on (002) sapphire and glass substrates using an RF magnetron sputtering technique. A target (97 wt-%ZnO–3 wt-%Ga 2 O 3 ) with a 2 inches diameter was used. The maximum horizontal component magnetic field strength at the target surface was 5 × T. 2015/12/16 STUT 太陽能材料與模組實驗室 5

版權所有 翻印必究 The substrate surfaces were cleaned in an ultrasonic cleaner for 10 min with acetone and methanol respectively and then blown dry with nitrogen before they were introduced into the sputtering system. The Ar and O 2 gas flow rates were fixed at 20 and 10 sccm respectively. The RF sputtering power and the substrate temperature were 80 W and 200 ℃ respectively. 2015/12/16 STUT 太陽能材料與模組實驗室 6

版權所有 翻印必究 The GZO thin film samples were annealed at 200, 400 and 600 ℃ for 1 h in an O 2, N 2 and N 2 +5%H 2 atmosphere. For the prepared samples X-ray diffraction (XRD) analysis was performed to investigate the crystallinity of the GZO films. The full width at half maximum (FWHM) of ZnO (002) XRD peaks was measured from the XRD diffraction spectra to assess the crystallinity. 2015/12/16 STUT 太陽能材料與模組實驗室 7

版權所有 翻印必究 An a-step (Dektak-3) was used to measure the film thickness. Scanning electron microscopy was performed to observe the microstructures of the GZO films. The carrier concentration, carrier mobility and electrical resistivity of the films were determined by Hall effect measurement (HEM-2000). The optical transmittance measurements were made using a UV/VIS spectrophotometer. 2015/12/16 STUT 太陽能材料與模組實驗室 8

版權所有 翻印必究 Result and Discussion 2015/12/16 STUT 太陽能材料與模組實驗室 9

版權所有 翻印必究 X-ray diffraction patterns shown in Fig. 1 indicate that the Ga doped ZnO thin films, as deposited and annealed at 400 ℃ in N 2, O 2 and N 2 +5%H 2 atmospheres exhibit a strong c axis orientation perpendicular to the substrate surface. The crystallinity evaluated from the intensity and FWHM of the (002) diffraction peak is enhanced by annealing regardless of the annealing atmosphere. The enhancement in crystallinity by annealing may be explained by many causes. One of them is an increase in grain size by annealing. 2015/12/16 STUT 太陽能材料與模組實驗室 10

版權所有 翻印必究 2015/12/16 STUT 太陽能材料與模組實驗室 11

版權所有 翻印必究 Figure 2 shows plan view SEM micrographs of GZO thin films for different annealing atmospheres and annealing temperatures. The grain size tends to increase and the grain shape tends to change from an equiaxed rough grain to a longish smooth grain as the annealing temperature increases from 400 to 600 ℃. 2015/12/16 STUT 太陽能材料與模組實驗室 12

版權所有 翻印必究 In addition to an increase in the grain size, the concentrations of point defects such as oxygen vacancy and zinc interstitial decrease as the annealing temperature increases. This also seems to contribute to the enhancement in crystallinity by annealing. 2015/12/16 STUT 太陽能材料與模組實驗室 13

版權所有 翻印必究 2015/12/16 STUT 太陽能材料與模組實驗室 14

版權所有 翻印必究 In the case of N 2 +5%H 2 annealing the resistivity decreases first and then increases as the annealing temperature increases. This may be attributed to the desorption of negatively charged oxygen species from the grain boundaries which act as trapping sites and form potential barriers during annealing Both the carrier concentration and mobility of the GZO film annealed in an O 2 atmosphere tend to decrease with increasing annealing temperature, as can be seen in Fig /12/16 STUT 太陽能材料與模組實驗室 15

版權所有 翻印必究 2015/12/16 STUT 太陽能材料與模組實驗室 16

版權所有 翻印必究 All the annealed GZO thin films have an average transmittance of ~80% and one as high as ~90% especially in the visible range. It seems that the transmittance is improved by annealing regardless of the annealing atmosphere. This improvement in transmittance may be attributed to enhancement in the crystallinity and a decrease in surface roughness. 2015/12/16 STUT 太陽能材料與模組實驗室 17

版權所有 翻印必究 The optical transmittance of a film is known to strongly depend on its surface morphology. The increase in transmittance by annealing may be attributed to an increase in the grain size as can be seen in the SEM images (Fig. 2). As the grain size increases, grain boundary scattering is reduced, so that the transmittance is improved. Absorption owing to an interband transition of ZnO occurs in the wavelength range from 340 to 380 nm. 2015/12/16 STUT 太陽能材料與模組實驗室 18

版權所有 翻印必究 2015/12/16 STUT 太陽能材料與模組實驗室 19

版權所有 翻印必究 In Fig. 5a and b respectively. The optical band gaps for the GZO films as deposited, annealed in an N2z5%H2 atmosphere, and annealed in an O2 atmosphere are 3.54, 3.32 and 3.40 eV respectively. Therefore, it may be said that annealing in a reducing atmosphere widens the optical band gap, while annealing in an oxidising atmosphere makes the optical band gap narrower. The phenomenon that the optical band gap increases with increasing carrier concentration is known as the ‘blueshift’. 2015/12/16 STUT 太陽能材料與模組實驗室 20

版權所有 翻印必究 Conclusion 當退火溫度為 400 度在 N 2 +5 %氫氣氛圍下可得 最低的電阻率 2.3×10 -4 Ωcm 。 在此證明無論是提高退火溫度或改變退火氛 圍 GZO 穿透率都不會受影響。 在 N 2 +5 %氫氣退火氛圍下可拓寬了能隙,而 在氧氣退火氛圍會使能隙變窄,這現象可解 釋為藍移。 2015/12/16 STUT 太陽能材料與模組實驗室 21

版權所有 翻印必究 2015/12/16 STUT 太陽能材料與模組實驗室 THANKS FOR YOUR ATTENTION 22