近红外波段锑基铋掺杂薄膜厚度对光学常数与光学带隙的影响

采用磁控溅射法制备了不同厚度的锑基铋掺杂薄膜,用X射线衍射(XRD)和透射电子显微镜(TEM)研究了薄膜结构随厚度的变化。利用椭圆偏振法测定了样品薄膜在近红外波段的光学常数与光学带隙,研究了膜厚对样品薄膜光学常数和光学带隙的影响。结果表明,膜厚从7 nm增加至100 nm时,其结构由非晶态转变为晶态。在950～2200 nm波段,不同厚度薄膜样品的折射率在4.6～8.9范围,消光系数在0.6～5.8范围,光学带隙在0.32～0.16 eV范围。随着膜厚的增加,薄膜的折射率和光学带隙减小,而消光系数升高;光学常数在膜厚50 nm时存在临界值,其原因是临界值前后薄膜微观结构变化不同。     

非晶氧化硅薄膜带尾发光特性

采用等离子体增强化学气相沉积技术,通过改变CO2流量制备了不同氧含量的非晶氧化硅薄膜。利用紫外可见吸收谱、傅里叶红外吸收谱和稳态/瞬态光致发光谱等技术研究了薄膜的微观结构和光学特性。实验结果表明,随着氧含量的增加,薄膜的带隙增大,光致发光强度增加、峰值朝高能方向移动、光谱半峰全宽展宽。时间分辨光谱显示薄膜发光峰值处的衰减时间随氧含量的增加从6.2ns单调增加到21ns,而同一样品的发光寿命随发射波长能量增加而减小。综合分析光学吸收、发射及发光衰减特性表明,薄膜的发光机制主要归结为非晶材料带尾态之间的辐射复合。     

生长温度对6H-SiC上SiCGe薄膜发光特性的影响

利用低压化学气相淀积工艺在6H-SiC衬底成功制备了SiCGe薄膜。通过光致发光(PL)谱研究了生长温度对SiCGe薄膜发光特性的影响。结果表明:生长温度为980,1030,1060℃的SiCGe薄膜的室温光致发光峰分别位于2.13,2.18,2.31eV处;通过组分分析和带隙计算,认定该发光峰来自于带间辐射复合,证实了改变生长温度对SiCGe薄膜带隙的调节作用。同时,对SiCGe薄膜进行了变温PL测试,发现当测试温度高于200K时,发光峰呈现出蓝移现象。认为这是不同机制参与发光所造成的。     

厚度对未掺杂ZnO薄膜光谱性能的影响

X射线衍射光谱、拉曼光谱和紫外可见透射光谱技术是薄膜材料检测的重要技术手段。通过对薄膜材料光谱性能的分析,可以获得薄膜材料的物相、晶体结构和透光性能等信息。为了解厚度对未掺杂ZnO薄膜的X射线衍射光谱、拉曼光谱和紫外可见透射光谱性能的影响,利用溶胶-凝胶法在石英衬底上旋涂制备了不同厚度的未掺杂ZnO薄膜样品,并对薄膜样品进行了X射线衍射光谱、拉曼光谱和紫外可见透射光谱的检测。首先,通过X射线衍射光谱检测发现,薄膜样品呈现出（002）晶面的衍射峰,ZnO薄膜为六角纤锌矿结构,均沿着C轴择优取向生长,且随着薄膜厚度的增加,衍射峰明显增强,ZnO薄膜的晶粒尺寸随着膜厚的增加而长大。利用扫描电子显微镜对薄膜样品的表面形貌分析显示,薄膜表面致密均匀,具有纳米晶体的结构,其晶粒具有明显的六角形状。通过拉曼光谱检测发现,薄膜样品均出现了437 cm-1的拉曼峰,这是ZnO纤锌矿结构的特征峰,且随着薄膜厚度的增加,其特征拉曼峰强度也增加,进一步说明了随着ZnO薄膜厚度的增加,ZnO薄膜晶化得到了加强。最后,通过紫外可见透射光谱测试发现,随着膜厚的增加,薄膜的吸收边发生一定红移,薄膜样品在可见光区域内的透过率随着膜厚度增加而略有降低,但平均透过率都超过90%。通过对薄膜样品的紫外-可见透射光谱进一步分析,估算了薄膜样品的折射率,定量计算了薄膜样品的光学禁带宽度,计算结果表明：厚度的改变对薄膜样品的折射率影响不大,但其禁带宽度随着薄膜厚度的增加而变窄,且均大于未掺杂ZnO禁带宽度的理论值3.37 eV。进一步分析表明,ZnO薄膜厚度的变化与ZnO晶粒尺寸的变化呈正相关,本质上,吸收边或光学禁带宽度的变化是由于ZnO晶粒尺寸变化引起的。     

膜层厚度对蓝宝石衬底上生长的ITO薄膜性质的影响

采用磁控溅射的方法在蓝宝石衬底上制备了氧化铟锡(ITO)透明氧化物薄膜;研究了不同厚度薄膜的结构、光学和电学特性。经X射线衍射(XRD)测量,发现在蓝宝石衬底上生长的ITO薄膜呈现了较高的(222)择优取向;随着膜层厚度的增加,该衍射峰对应的2θ衍射角逐渐向大角度方向移动,同时该衍射峰的半峰全宽逐渐减小,平均晶粒尺寸增大。 经光学透射光谱测量,发现随着膜层厚度的增加,光学透过率逐渐减小。膜层厚度为0.2 μm时,可见光透过率超过80%,当膜层厚度为0.8 μm时,可见光透过率下降到60%。电学测量结果表明,随着膜层厚度的增加,薄膜电阻率逐渐减小。膜层厚度为0.2 μm时,电阻率为9×10^-4 Ω·cm, 膜层厚度为0.8 μm时,电阻率为5.5×10^-4 Ω·cm。     

纳米ZnO镶嵌SiO2薄膜的磁控溅射制备和发光性质的研究

采用射频磁控反应溅射方法在SiO衬底上制备了纳米ZnO镶嵌SiO2薄膜.在室温下利用吸收光谱和光致发光光谱研究了样品的光学性质.发现吸收光谱随纳米ZnO尺寸的减小发生了明显的蓝移,表明随着ZnO尺寸的减小,量子尺寸效应增强,导致带隙展宽,吸收峰蓝移.光致发光光谱在387和441 nm附近出现了两个发光带,分析认为紫外发光来源于自由激子的辐射复合,而蓝色发光带来自于氧空位的电子到价带的跃迁,并用时间分辨光谱和发光衰减证实了上述观点.     

PbI2厚膜的结构、形貌与光谱性质研究

毫米级厚度碘化铅(PbI2)膜是制造下一代阵列高能辐射探测器的关键材料。采用近空间升华法制备了PbI2厚膜,研究升华源温度对制备样品晶体结构、表面形貌及光谱性质的影响。结果表明,随着源温度的升高,样品厚度由1 000μm下降到220μm。X射线衍射测试表明,厚膜为沿(002)晶面择优取向生长的六方相多晶结构,其晶粒尺寸、位错密度及生长应力与源温度密切相关。扫描电子显微镜测试显示,样品由六方片状颗粒堆积而成,其颗粒直径约为248μm,厚约32.7μm,有明显的层状结构。解谱拟合发现,样品的拉曼光谱有147,169,217和210cm-1等4个散射峰,前三个峰对应于4H晶型PbI2晶体的纵光学波振动模式,210cm-1来源于衬底SnO2的相关振动模式。随源温度的升高,147cm-1拉曼峰有明显变化,其峰强高于225℃时出现大幅度的下降,峰形展宽。在340nm光激发下,样品的室温光致发光谱在2.25,2.57和2.64eV附近出现弱的发光峰,来源于与缺陷和激子相关的复合。综合结构表征与光谱测试结果,200℃时沉积的PbI2厚膜具有最佳的结晶质量,其厚度约为659μm。     

不同厚度溅射Ag膜的微结构及光学常数研究

用直流溅射法在室温Si基片上制备了4．9nm-189.0nm范围内不同厚度的Ag薄膜，并用X射线衍射及反射式椭偏光谱技术对薄膜的微结构和光学常数进行了测试分析。结构分析表明：制备的Ag膜均呈多晶状态，晶体结构仍为面心立方；随膜厚增加薄膜的平均晶粒心潮6．3nm逐渐增大到14．5nm；薄膜晶格常数均比标准值（0．40862nm)稍小，随膜厚增加，薄膜晶格常数由0．40585nm增大到0.40779nm。250nm-830nm光频范围椭偏光谱测量结果表明：与Johnson的厚Ag膜数据相比，我们制备的Ag薄膜光学折射率n总体上均增大，消光系数k变化复杂；在厚度为4．9nm-83.7nm范围内，实验薄膜的光学常数与Johnson数据差别很大，厚度小于33．3nm的实验薄膜k谱线中出现吸收峰，峰位由460nm红移至690nm处，且其对应的峰宽逐渐宽化；当膜厚达到约189nm时，实验薄膜与Johnson光学常数数据已基本趋于一致。     

镶嵌有纳米硅的SiN_x薄膜光致发光的温度依赖特性研究

采用对靶磁控溅射法在单晶硅衬底上沉积镶嵌有纳米硅的氮化硅薄膜,然后在形成气体FG(10%H2,90%N2)气氛中进行450℃常规热退火50min。通过荧光光谱仪测得的稳态/瞬态光致发光(PL)谱研究了镶嵌有纳米硅的氮化硅(SiNx)薄膜样品光致发光特性。结果表明,样品的发光过程可以归因于纳米硅的量子限制效应发光和与缺陷相关的发光。随着激发光能量的增加,PL谱峰位发生蓝移,表明较小粒度的纳米硅发光比例增加;温度的降低会抑制非辐射复合过程,提高辐射复合几率,因此发光寿命延长,发光强度呈指数增加;随着探测波长的减小,样品的发光寿命则明显缩短,表明纳米硅的量子限制效应发光对温度有很强的依赖性。     

磁控溅射制备铬薄膜的结构和光电学性质(英文)

用直流磁控溅射技术在石英基片上制备不同厚度(5nm～114nm之间)的铬膜.使用X射线衍射仪和分光光度计分别检测薄膜的结构和光学性质,利用德鲁特模型和薄膜的透射、反射光谱计算铬膜的厚度和光学常量,并采用Van der Pauw方法测量薄膜电学性质.结果表明:制备的铬薄膜为体心立方的多晶态,随着膜厚的增加,薄膜的结晶性能提高,晶粒尺寸增大;在可见光区域,当膜厚小于32nm时,随着膜厚的增加,折射率快速减小,消光系数快速增大,当膜厚大于32nm时,折射率和消光系数均缓慢减小并逐渐趋于稳定;薄膜电阻率随膜厚的增加为一次指数衰减.     

钛酸锶钡薄膜的室温光学性能研究

采用溶胶-凝胶法制备了(Ba0.75Sr0.25)TiO3薄膜,研究了不同退火温度下样品的物相结构、薄膜的光致发光性能和光学透过率。结果表明:室温下非晶钛酸锶钡薄膜在蓝光激发下具有明显的发光现象,发光波长范围是500～650 nm,峰值在525 nm附近。延长非晶态薄膜的退火时间能够显著提高样品的发光强度,且发光强度随薄膜厚度增加而增大。晶态薄膜有微弱的发光现象。透射谱测试结果表明,钛酸锶钡薄膜在可见光范围内具有良好的光学透过率。     

Structural and optical properties of RF magnetron sputtered aluminum nitride films without external substrate heating

We report structural and optical properties of aluminum nitride (AlN) thin films prepared by RF magnetron sputtering. A ceramic AlN target was used to sputter deposit AlN films without external substrate heating in Ar-N₂ (1:1) ambient. The X-ray diffraction and high resolution transmission electron microscopy results revealed that the films were preferentially oriented along c-axis. Cross-sectional imaging revealed columnar growth perpendicular to the substrate. The secondary ion mass spectroscopy analysis confirmed that aluminum and nitrogen distribution was uniform within the thickness of the film. The optical band gap of 5.3 eV was evaluated by UV-vis spectroscopy. Photo-luminescence broad band was observed in the range of 420-600 nm with two maxima, centered at 433 nm and 466 nm wavelengths related to the energy states originated during the film growth. A structural property correlation has been carried out to explore the possible application of such important well oriented nano-structured two-dimensional semiconducting objects.     

Effect of vertical deposition angle on structural and optical properties of tantalum oxide nano layers deposited by electron gun evaporation

Tantalum oxide nano layers were deposition on glass substrate with different thicknesses (30, 60, 90 and 120 nm) in vertical deposition angle and high vacuum condition at room temperature by using electron gun evaporation method. There were no specific peaks in XRD patterns because of amorphous nature of these layers. AFM results show that surface roughness is reduced by increasing the thickness of the layers. FESEM images show nucleation, growth, accession and integration as interconnected islands in the lower thickness and re-nucleation at higher thicknesses (120 nm). We studied Raman spectra of the produced Ta₂O₅ amorphous layers. The calculated optical coefficients by using Kramers-Kronig relations show that with increasing film thickness, dielectric properties, absorption coefficient and band gap energy have increased.     

Analysis of amorphous-nano-crystalline multilayer structures by optical, photo-deflection and photo-current spectroscopy

Thin film structures consisting of nano-crystalline and amorphous silicon layers deposited on glass by plasma enhanced chemical vapour deposition have been studied by optical spectroscopy methods (transmittance, photo-thermal deflection spectroscopy and photo-current spectroscopy) while structure was examined by Raman spectroscopy. The nano-crystalline layers were grown on the same amorphous layers, using different radio-frequency (RF) discharge powers, leading to different structural and optical properties. The energy dependence of the absorption coefficient above the band gap agrees well to the bimodal size distribution of crystals and crystal fraction estimated by Raman spectroscopy. For energies below the band gap, the comparison of the absorption of the bi-layer systems with respect to single amorphous layer reveals that the samples produced at higher RF discharge present a higher disorder degree (Urbach edge increases) and higher number of structural defects (absorption related to the defects increases).     

Effect of sputtering pressure on structural and optical properties of silver oxide thin films; Kramers–Kronig method

Silver oxide nano layers were prepared by RF magnetron sputtering on amorphous SiO₂ substrates. O₂ pressure in chamber was varied from 1 to 4 and 7 mTorr during growth process. The effects of different O₂ pressure on structural, morphological and optical properties of the films were investigated by means of X-ray diffraction, scanning electron microscopy, atomic force microscopy and UV–Vis spectroscopy analyses. Optical reflectance measured in the wavelength of 350–950 nm by spectroscopy. Other optical properties and optical band gaps were calculated using Kramers–Kronig relations. The X-ray diffraction measurements showed change in crystalline structure with increasing O₂ pressure. Preferred orientation has been changed to another growth orientation at 4 mTorr O₂ pressure. The Atomic force microscope images showed increasing in roughness consistently by increasing oxygen pressure. The thickness of the thin films decreases (from 217 to 180 nm) with increasing O₂ pressure. Optical results revealed that the highest optical band gap of 3.1 eV and the highest transmittance of?~?80% were achieved at lower O₂ pressure (1 mTorr).     

酞菁铜旋涂薄膜的形貌与光谱学性质研究

采用旋涂法制备了2,9,16,23-四-异丙氧基酞菁铜(CuPc(OC3H7-i)4)薄膜,利用AFM、UV-Vis和FT-IR对薄膜的表面形貌和光谱学性质进行了表征。薄膜表面结构是由约为216nm×55nm×4nm的清晰纳米畴组成,旋涂膜中酞菁铜分子是处于一种无序的状态,其Soret带吸收与氯仿溶液相比位置不变,而Q带的聚集体和单体的吸收峰红移约20nm。     

脉冲激光沉积制备MgxNi1-xO合金薄膜的表征及光学性质研究

应用脉冲激光沉积(PLD)技术,固定脉冲激光能量密度为5 J/cm2,调节薄膜生长基底温度为300~700 ℃,制备了系列Mg_xNi_1-xO合金薄膜。通过透射电子显微镜(TEM)、X射线光电子能谱(XPS)、原子力显微术(AFM)等表征分析手段,详细分析了薄膜的成分及组织,研究了退火处理对样品的影响。通过UV-Vis分光光度计研究了透射光谱,结合理论计算了光学带隙宽度。结果表明:薄膜由非晶及多晶构成,紫外吸收边约为290 nm, 接近日盲波段的上限; 衬底温度为500 ℃、激光脉冲能量密度为5 J/cm2时生长的薄膜在短波部分吸收强烈,而长波部分几乎不吸收,有利于紫外探测; 退火处理改善了样品表面质量, 但不能有效拓宽光学带隙。     

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     

Structural characterization and optical properties of UO2 thin films by magnetron sputtering

Uranium dioxide films were deposited on Si (1 1 1) substrates by dc magnetron sputtering method at different sputtering parameters. The structure, morphology and chemical state of the films were studied by field emission scanning electron microscopy, X-ray diffraction, X-ray photoelectron spectroscopy and atomic force microscopy. Influences of film thickness on the microstructure and optical properties were investigated. Experimental results show that the film crystallites are preferentially oriented with the (1 1 1) planes. The average grain size increases with increasing film thickness. AFM images show that the root mean square roughness of the films is between 1.2 nm and 2.1 nm. Optical constants (refractive index, extinction coefficient) of the films in the wavelength range of 350-1000 nm are obtained by ellipsometric spectroscopy. The result shows that the refractive index decreases with the increasing film thickness, while extinction coefficient increases with the film thickness.