含氮氟化类金刚石(FN-DLC)薄膜的研究：(Ⅱ)射频功率对薄膜光学带隙的影响

以CF₄,CH₄和N₂为源气体，采用射频等离子体增强化学气相沉积法，在不同射频功率下制备了含氮氟化类金刚石薄膜样品.原子力显微形貌显示，低功率下沉积样品表面致密均匀.拉曼及傅里叶变换红外光谱分析显示，随着射频功率的改变，薄膜的结构和组分也随之变化.紫外-可见光透射光谱证明薄膜具有紫外强吸收特性，通过计算得到其光学带隙在1.89—2.29 eV之间.结果表明，射频功率增加，薄膜内sp²C含量增加，或者说C=C交联相对浓度增加、F的相对浓度降低，导致薄膜内π-π^*带边态密度增大，光学带隙减小. 关键词： 含氮氟化类金刚石薄膜 射频功率 光学带隙     

含氮氟化类金刚石(FN-DLC)薄膜的研究：(Ⅳ)氮掺杂对薄膜结构的影响

不同条件下，在单晶硅基片上沉积了含氮氟化类金刚石(FN-DLC)薄膜.原子力显微(AFM)形貌显示，掺N后，薄膜变得致密均匀.傅里叶变换吸收红外光谱(FTIR)表明，随着r(r=N₂/［N₂+CF₄+CH₄］)的增大薄膜中C—H键的逐渐减少，C〖FY=,1〗N和C≡N键含量逐渐增加.X射线光电子能谱(XPS)的C1s和N1s峰拟合结果发现，N掺入导致在薄膜中出现β-C₃N₄和a-CN_x(x=1,2,3)成分.Roman散射谱的G峰向高频方向位移和峰值展宽等证明：随着r的增大，薄膜内sp²键态含量增加. 关键词： 氟化类金刚石膜 键结构 氮掺杂     

反应磁控溅射法制备的氟化类金刚石薄膜的XPS结构研究

采用射频反应磁控溅射法用高纯石墨作靶、三氟甲烷(CHF₃)和氩气(Ar)作源气体制 备了氟化类金刚石（FDLC）薄膜，通过XPS光谱结合拉曼光谱、红外透射光谱和紫外 可见光光谱研究了源气体流量比等工艺条件对薄膜中键结构、sp2/sp3杂化比以及光学带隙等性能的影响.结果表明在低功率(60W)、高气压(2.0Pa)和适当的流量比(Ar/CHF₃=2∶ 1)下利用射频反应磁控溅射法可制备出氟含量高且具有较宽光学带隙和超低介电常数的FDLC薄膜. 关键词： 反应磁控溅射 氟化类金刚石薄膜 红外透射光谱 XPS光谱     

溅射制备非晶氮化镓薄膜的光学性能

采用直流磁控溅射方法在不同的氩气-氮气（Ar-N₂）气氛中制备了非晶氮化镓（a-GaN）薄膜. X射线衍射分析（XRD）和拉曼光谱（Raman）表明薄膜具有非晶结构. 通过椭偏光谱（SE）得到薄膜的折射率和厚度都随着氩气分量的增多而增大. 紫外—可见光谱（UV-Vis）的测量得到,当氩气分量R,即Ar/（Ar+N₂）,为0%时,薄膜的光学带隙为3.90eV,比晶体GaN （c-GaN） 的较大,这主要是由非晶结构中原子无序性造成的;而当R关键词： 非晶氮化镓 溅射 光学带隙 带尾态     

溅射制备Ge,Nb共掺杂窄光学带隙和低电阻率的TiO2薄膜

采用射频磁控溅射技术制备了Ge,Nb共掺杂的锐钛矿结构TiO₂薄膜,详细探讨了薄膜的结构、电阻率及光学带隙等性质随Ge,Nb掺杂量、溅射功率和热处理温度等参数的变化,发现Ge,Nb共掺杂可以同时调节TiO₂薄膜的光学带隙和电阻率.体积分数约为6%Nb和20%Ge的共掺杂TiO₂薄膜电阻率由10⁴Ω/cm减小至10^-1Ω/cm,光学带隙由3.2 eV减小至1.9 eV.退火后掺杂TiO₂薄膜不仅显示更低的电阻率,还表现出更强的可见-红外光吸收.结果表明,改变Ge,Nb的掺杂量和退火条件能够制备出电阻率和带隙都可调的TiO₂薄膜.     

氮化硅薄膜中纳米非晶硅颗粒的键合结构及光致发光

采用螺旋波等离子体化学气相沉积技术以N₂/SiH₄/H₂为反应气体制备了镶嵌有纳米非晶硅颗粒的氢化氮化硅薄膜,通过改变N₂流量实现了薄膜从红到蓝绿的可调谐光致发光.傅里叶红外透射和紫外-可见光吸收特性分析表明,所生长薄膜具有较高的氢含量,N₂流量增加使氢的键合结构发生变化,非晶硅颗粒尺寸减小,所对应的薄膜的光学带隙逐渐增加和微观结构有序度减小.可调光致发光(PL)主要来源于纳米硅颗粒的量子限制效应发光,随N₂流量增加,PL的谱线展宽并逐渐增强. 关键词： 傅里叶红外透射谱 光吸收谱 纳米硅粒子镶嵌薄膜 光致发光     

射频磁控溅射制备氮化锌薄膜的椭圆偏振光谱研究

在不同的衬底温度下,使用反应射频磁控溅射法,在玻璃衬底上制备了氮化锌薄膜样品.用X射线衍射仪、原子力显微镜和椭偏仪对薄膜的晶体结构、表面形貌、光学性质进行了表征分析.薄膜的晶粒尺寸会随着衬底温度的升高先增大后减小,在200?C时薄膜的结晶性最好.用椭偏仪测试样品,建立物理模型计算出氮化锌薄膜在430—850 nm范围内的折射率和消光系数等光学参数.利用Tauc公式计算出氮化锌薄膜的光学带隙在1.73—1.79 eV之间.     

含氮氟化类金刚石(FN-DLC)薄膜的研究：(Ⅲ)疏水性能分析

不同沉积条件下，在单晶硅基底上沉积了含氮氟化类金刚石(FN-DLC)薄膜，用静滴接触角/表面张力测量仪测量了水与FN-DLC膜表面的接触角.用X射线光电子能谱、Raman光谱和傅里叶变换吸收红外光谱(FTIR)分析了薄膜的组分和结构.用原子力显微镜观测了薄膜的表面形貌.结果表明，FN-DLC薄膜疏水性能主要取决于薄膜表面的化学结构、薄膜表面极化强度的强弱、以及薄膜的表面粗糙度的大小.sp³/sp²的比值减小，CF₂基团含量增加，薄膜粗糙度增加，接触角增大；反之，则接触角减小.在工艺上，沉积温度和功率的减小，气体流量比r(r=CF4/［CF₄+CH₄］)的增加，都会使水的浸润性变差，接触角增大. 关键词： 氟化类金刚石膜 疏水性 接触角     

蓝宝石基片的处理方法对ZnO薄膜生长行为的影响

采用反应射频磁控溅射方法,在经过不同方法处理的蓝宝石基片上,在同一条件下沉积了ZnO薄膜.利用原子力显微镜、X射线衍射、反射式高能电子衍射等分析技术,对基片和薄膜的结构、表面形貌进行了系统表征.研究结果显示,不同退火条件下的蓝宝石基片表面结构之间没有本质的差异,均为α-Al₂O₃ (001)晶面,但基片表面形貌的变化较大.在不同方法处理的蓝宝石基片上生长的ZnO薄膜均具有高c轴取向的织构特征,但薄膜的表面形貌差异较大.基片经真空退火处 关键词： ZnO薄膜 反应磁控溅射 基片处理 形貌分析     

Ge20Sb15Se65薄膜的热致光学特性变化研究

采用磁控溅射法制备了Ge₂₀Sb₁₅Se₆₅薄膜, 研究热处理温度(150—400 ℃)对薄膜光学特性的影响. 通过分光光度计、X射线衍射仪、显微拉曼光谱仪对热处理前后薄膜样品 的光学特性和微观结构进行了表征, 并根据Swanepoel方法以及Tauc公式分别计算了薄膜折射率色散曲线和光学带隙等参数. 结果表明当退火温度(T_a)小于薄膜的玻璃转化温度(T_g)时,薄膜的光学带隙(E_g^opt)随着退火温度的增加由1.845 eV上升至1.932 eV, 而折射率由2.61降至2.54; 当退火温度大于薄膜的玻璃转化温度时,薄膜的光学带隙随退火温度的增加由1.932 eV降至1.822 eV, 折射率则由2.54增至2.71. 最后利用Mott和Davis提出的非晶材料由非晶到晶态的结构转变模型对结果进行了解释, 并通过薄膜XRD和Raman光谱进一步验证了结构变化是薄膜热致变化的重要原因. 关键词： 20Sb₁₅Se₆₅薄膜')" href="#">Ge₂₀Sb₁₅Se₆₅薄膜 热处理 光学带隙 折射率     

氮流量对磁控溅射法制备氮化钛薄膜光学性能的影响

采用磁控溅射方法在载波片和Al基片上制备了氮化钛薄膜;通过改变N2流量来改变薄膜中N／Ti原子比例。采用分光光度计和扫描隧道显微镜测试手段对氮化钛薄膜光学性能随N2流量变化的规律进行了研究。薄膜反射率光谱和扫描隧道图谱分析表明,氮化钛薄膜主要遵循自由载流子光吸收机制,随着N含量的增加,溥膜中的自由电子数目不断减少,等离子体频率逐渐红移,反射率降低,薄膜颜色发生变化。从薄膜扫描隧道谱（STS）可知,TiN薄膜表现出类似金属的光学性能,并且其禁带宽度Eg=1．64eV。     

低温铝诱导晶化制备纳米晶硅薄膜的物相和光学性能研究

采用射频磁控溅射镀膜系统,在玻璃衬底上制备了非晶硅(α-Si)/铝(Al)复合薄膜,结合氮气(N₂)气氛中低温快速光热退火制备了纳米晶硅(nc-Si)薄膜;利用光学显微镜、共焦光学显微仪、X射线衍射(XRD)仪、拉曼散射光谱(Raman)仪和紫外-可见光-近红外分光光度计(UV-VIS-NIR)对纳米晶硅薄膜的表面形貌、物相及光学性能进行了表征,研究了退火工艺对薄膜性能的影响。结果表明： 300 ℃,25 min光热退火可使α-Si/Al膜晶化为纳米晶硅薄膜,晶化率为15.56%,晶粒尺寸为1.75 nm;退火温度从300 ℃逐渐升高到400 ℃,纳米晶硅薄膜晶粒尺寸、晶化率、带隙逐渐增加,表面均匀性、晶格畸变量逐渐减小;退火温度从400 ℃逐渐升高到500 ℃,纳米晶硅薄膜的晶粒尺寸、晶化率继续增加,带隙则逐渐降低;采用纳米晶硅薄膜的吸光模型验证了所制备的纳米晶硅薄膜的光学特性,其光学带隙的变化趋势与吸光模型得出的结果一致。     

Effect of thermal annealing on r.f. sputtering-deposited nanocrystalline GaN<Subscript><Emphasis Type="Italic">x</Emphasis></Subscript>As<Subscript>1−<Emphasis Type="Italic">x</Emphasis></Subscript> thin films

GaNAs thin films were deposited on Corning glass substrates by radio frequency (r.f.) sputtering in molecular nitrogen ambient. The stoichiometry in the GaNAs alloy was controlled by changing the nitrogen incorporation in the film during the growth process, through the variation of the r.f. power in the range 30–80 watts which produced films with N concentrations in the range: x = 0.85–0.90. The structural and optical properties of the GaNAs thin films were studied by X-ray diffraction (XRD), photoacoustic (PA) and photoluminescence (PL) spectroscopies. XRD measurements show a broad diffraction band with a peak close to the (002) diffraction line of the GaN hexagonal phase, and a slight shoulder at the position corresponding to the (111) GaAs cubic phase. The PA absorption spectra showed a remarkable shift to higher energies of the absorption edge as the r.f. power decreases corresponding to the films with higher N concentrations. Thermal annealing of the GaNAs films at temperatures of 450 °C produced a GaAs nanocrystalline phase with grain sizes in the range 10–13 nm, as confirmed by the XRD measurements that showed a well-defined peak in the (111) GaAs direction, and also by the PA spectra which showed an absorption band at energies around 1.45 eV due to the quantum confinement effects. PL spectra of thermal-annealed GaNAs films showed a very intense emission at 1.5 eV which we have associated to transitions between the first electron excited level and acceptor states in the GaAs nanocrystallites.     

Sputtered deposited nanocrystalline ZnO films: A correlation between electrical, optical and microstructural properties

Zinc oxide thin films were prepared by dc (direct current) and rf (radio frequency) magnetron sputtering on glass substrates. ZnO films produced by dc sputtering have a high resistance, while the films produced using rf sputtering are significantly more conductive. While the conductive films have a compact nodular surface morphology, the resistive films have a relatively porous surface with columnar structures in cross section. Compared to the dc sputtered films, rf sputtered films have a microstructure with smaller d spacing, lower internal stress, higher band gap energy and higher density. Dependence of conductivity on the deposition technique and the resulting d spacing , stress, density, band gap, film thickness and Al doping are discussed. Correlations between the electrical conductivity, microstructural parameters and optical properties of the films have been made. PACS 73.25.+i; 81.15.cd; 81.05.ys     

Tin-mono-sulfide (SnS) thin films prepared by chemical spray pyrolysis with different [S]/[Sn] ratios

SnS thin films were deposited by chemical spray pyrolysis using cost-effective and low-toxicity sources materials like tin (II) chloride dihydrate and thiourea as sources of tin and sulphur, respectively. We have studied the properties of sprayed SnS thin films with [S]/[Sn] ratios were varied from 1 to 4 in order to optimize these parameters. X-ray diffraction was used for analyzing the films structure, Raman Spectroscopy for assessing the films quality and structure, scanning electron microscope (SEM) for surface morphology and energy dispersive energy (EDS) for compositional element in samples, atomic force microscopy (AFM) for the topography of surfaces and optical spectroscopy for measuring transmittances and then deducing the band gap energies. All films obtained are polycrystalline with (111) as preferential direction for films with [S]/[Sn] ratio equals to one while for [S]/[Sn] ratios from 2 to 4 the main peak becomes (101) and the (111) peak decreases in intensity. Raman spectroscopy confirms the presence of only one SnS phase without any additional parasite secondary phases. SEM images revealed that films are well adhered onto glass surface with rounded grain. AFM confirms this result being films with [S]/[Sn] = 1 the roughest and also with the largest grain size. EDS results show an improvement of stoichiometry with the increase of the [S]/[Sn] ratio. From optical analysis, it is inferred that the band gap energy decreases from 1.83 to 1.77 eV when the [S]/[Sn] ratio changes from 2 to 4.     

High-energy heavy-ion induced physical and surface-chemical modifications in polycrystalline cadmium sulfide thin films

The effect of high electronic energy deposition on the structure, surface topography, optical properties, and electronic structure of cadmium sulfide (CdS) thin films have been investigated by irradiating the films with 100 MeV Ag⁺⁷ ions at different ion fluences in the range of 10¹²–10¹³ ions/cm². The CdS films were deposited on glass substrate by thermal evaporation, and the films studied in the present work are polycrystalline with crystallites preferentially oriented along (002)-H direction. It is shown that swift heavy ion (SHI) irradiation leads to grain agglomeration and hence an increase in the grain size at low ion fluences. The observed lattice compaction was related to irradiation induced polygonization. The optical band gap energy decreased after irradiation, possibly due to the combined effect of change in the grain size and in the creation of intermediate energy levels. Enhanced nonradiative recombination via additional deep levels, introduced by SHI irradiation was noticed from photoluminescence (PL) analysis. A shift in the core levels associated with the change in Fermi level position was realized from XPS analysis. The chemistry of CdS film surface was studied which showed profound chemisorption of oxygen on the surface of CdS.     

Microstructure and optical properties of nanocrystalline ZnO and ZnO:(Li or Al) thin films

Zinc oxide thin films (ZnO, ZnO:Li, ZnO:Al) were deposited on glass substrates by a sol-gel technique. Zinc acetate, lithium acetate, and aluminum chloride were used as metal ion sources in the precursor solutions. XRD analysis revealed that Li doped and undoped ZnO films formed single phase zincite structure in contrast to Al:ZnO films which did not fully crystallize at the annealing temperature of 550 °C. Crystallized films had a grain size under 50 nm and showed c-axis grain orientation. All films had a very smooth surface with RMS surface roughness values between 0.23 and 0.35 nm. Surface roughness and optical band tail values increased by Al doping. Compared to undoped ZnO films, Li doping slightly increased the optical band gap of the films.     

氧分压对磁控溅射制备ZnO薄膜的结构及光学特性的影响

采用射频反应磁控溅射法在玻璃衬底上成功制备出具有c轴高择优取向的ZnO薄膜,利用X射线衍射及紫外-可见吸收和透射光谱研究了氧分压变化对ZnO薄膜的微观结构及光吸收特性的影响。结果表明,当工作气压恒定时,用射频反应磁控溅射制备的ZnO薄膜的生长行为主要取决于成膜空间中氧的密度,合适的氧分压能够提高ZnO薄膜的结晶质量;薄膜在可见光区的平均透过率达到90%以上,且随着氧分压的增大,薄膜的光学带隙发生了一定程度的变化。采用量子限域模型对薄膜的光学带隙作了相应的理论计算,计算结果与对样品吸收谱所作的拟合结果符合较好,二者的变化趋势完全一致,表明ZnO纳米晶粒较小时,薄膜光学带隙的变化与量子限域效应有很大关系。     

氧掺入对纳米硅薄膜微结构及能带特性的影响

采用等离子体增强化学气相沉积法(PECVD)制备了富硅氧化硅薄膜,利用XRD衍射仪,傅里叶变换红外透射光谱仪以及紫外-可见光分光光度计分析了氧掺入对薄膜微观结构以及能带特性的影响。结果表明,随着氧掺入比(CO₂/SiH₄)的增加,薄膜晶粒尺寸减小,晶化度降低,纳米硅(nc-Si)表面的张应力先增加后减小。红外吸收谱分析表明,氧掺入比增加导致薄膜内氧含量增高,富氧Si—O键合密度增加,富硅Si—O键合密度降低。同时,薄膜结构因子减小,有序度增大,薄膜微观结构得到改善。当氧掺入比大于0.08时,薄膜结构因子增大,有序度降低。此外,氧掺入增加导致薄膜带隙不断增加,带尾宽度呈现先减小后增大的趋势。因此,通过氧掺入可以调节纳米硅薄膜微观结构及能带特性,氧掺入比为0.08时,薄膜具有高晶化度和较宽的带隙,微观结构得到有效改善,可用作薄膜太阳能电池的本征层。