软X射线Mo/Si多层膜反射率拟合分析

由于多层膜的表界面粗糙度和材料之间的相互扩散等因素，导致多层膜的实际反射率小于理论计算的反射率，因此，多层膜结构参量的确定对镀膜工艺参量的标定具有重要意义。由于描述单个非理想粗糙界面散射的Stearns法适用于软X射线短波段区域，采用它的数学模型来描述软X射线多层膜的粗糙度，利用最小二乘法曲线拟合法对同步辐射测得的Mo／Si多层膜的反射率曲线进行拟合，得到了非常好的拟合结果，从而确定了多层膜结构参量，同时分析了多层膜周期厚度，厚度比率，界面宽度以及仪器光谱分辨率对多层膜反射特性的影响，这些工作都为镀膜工艺改进提供了一定的理论依据。     

Co/Cu多层膜反铁磁第一、第二峰耦合结构的磁电阻与结构研究

确定了Co/Cu多层膜的第一和第二反铁磁耦合对应的非磁层(Cu)的厚度,对相同厚度铁磁层(Co)制备了第一与第二反铁磁耦合的Co/Cu多层膜,利用同步辐射掠入射X射线散射(衍射)技术研究了耦合多层膜的界面结构,探索了耦合多层膜中磁电阻增强的可能原因.     

表面等离子体共振膜系结构优化设计

Kretschmann型激发表面等离子体共振(SPR)膜系结构是探针诱导表面等离子体共振耦合纳米光刻技术(PSPRN)的关键部分之一。采用多层介质的特性矩阵法计算膜系结构的透射系数和反射率,对PSPRN所需的单膜层、双膜层及三膜层膜系结构进行了优化设计。计算结果表明,光波波长为514.5 nm时,对于选定材料的最佳膜系结构是Ag膜厚度为46 nm的单膜层结构,Ag膜厚度为24 nm,AgOx厚度为95 nm的双膜层结构及Ag膜厚度为44 nm,SiO2厚度为180 nm,AgOx厚度为10 nm的三膜层结构,提出了记录层材料应选择折射系数小且吸收系数尽可能小的光刻材料的观点。     

超二代微光像增强器多碱光电阴极膜厚测量研究

介绍了多碱光电阴极的光学性能和光谱反射率特性,测量了多碱阴极的光谱反射率曲线.该曲线与普通光学膜层光谱反射率曲线相比,形状较不规则,原因是多碱阴极膜层存在光吸收.光谱反射率曲线上的干涉峰是入射光在玻璃与阴极膜层界面反射和在阴极膜层与真空的界面反射的两束光发生干涉的结果.根据干涉的原理,如果阴极膜层所反射的两束光的光程差为二分之一波长的偶倍数时,光谱反射将出现干涉加强峰;如果阴极膜层所反射的两束光的光程差为二分之一波长的奇倍数时,光谱反射将出现干涉减弱峰.根据超二代像增强器光谱反射干涉峰对应的波长,可以计算出其阴极膜层的厚度约为191 nm,比二代像增强器阴极膜层的厚度增加了38％.多碱阴极膜层厚度是影响多碱阴极灵敏度的一个关键参量,仅仅靠人眼观察阴极膜层颜色的方法不准确.实践证明,利用光谱反射的方法来计算阴极膜层厚度的方法简单有效.如果在多碱阴极的制作过程中进行光谱反射率的监控,那么将可以精确控制阴极膜层的厚度,对多碱阴极的研究将会更加深入,多碱阴极的灵敏度也将会得到进一步的提升.     

Mo/Si软X射线多层膜的界面粗糙度研究

用磁控溅射法分别制备了以Mo膜层和Si膜层为顶层的Mo/Si多层膜系列, 利用小角X射线衍射确定了各多层膜的周期厚度。以不同周期数的Mo/Si多层膜的新鲜表面近似等同于同一多层膜的内界面,通过原子力显微镜研究了多层膜界面粗糙度随膜层数的变化规律。并在国家同步辐射实验室测量了各多层膜的软X射线反射率。研究表明：随着膜层数的增加,Mo膜层和Si膜层的界面粗糙度先减小后增加然后再减小,多层膜的峰值反射率先增加后减小。     

4.48 nm正入射软X射线激光用Cr/C多层膜高反射镜的研制

针对4.48nm类镍钽软X射线激光及其应用实验,设计制备了工作于这一波长的近正入射多层膜高反射镜。选择Cr/C为制备4.48nm高反射多层膜的材料对,通过优化设计,确定了多层膜的周期、周期数以及两种材料的厚度比。模拟了多层膜非理想界面对高反射多层膜性能的影响。采用直流磁控溅射方法在超光滑硅基片上实现了200周期Cr/C多层膜高反射镜的制备。利用X射线衍射仪测量了多层膜结构,在德国BessyⅡ同步辐射上测量了在工作波长处多层膜反射率,测量的峰值反射率达7.5%。对衍射仪测量的掠入射反射曲线和同步辐射测量的反射率曲线分别进行拟合,得到的粗糙度和厚度比的结果相近。测试结果表明,所制备的Cr/C多层膜样品结构良好,在指定工作波长处有较高的反射峰,达到了设计要求。     

Mo/Si软X射线多层膜的界面粗糙度研究

 用磁控溅射法分别制备了以Mo膜层和Si膜层为顶层的Mo/Si多层膜系列, 利用小角X射线衍射确定了各多层膜的周期厚度。以不同周期数的Mo/Si多层膜的新鲜表面近似等同于同一多层膜的内界面,通过原子力显微镜研究了多层膜界面粗糙度随膜层数的变化规律。并在国家同步辐射实验室测量了各多层膜的软X射线反射率。研究表明：随着膜层数的增加,Mo膜层和Si膜层的界面粗糙度先减小后增加然后再减小,多层膜的峰值反射率先增加后减小。     

宽温范围LD端泵Nd∶YAG激光器泵浦源光谱理论化

针对先进光刻调焦调平传感器系统的增益系数工艺相关性开展理论仿真与实验研究。建立了增益系数工艺相关性理论模型,仿真分析了调焦调平传感器增益系数与测量误差随不同光刻工艺材料膜层厚度的变化规律。在自研实验系统上对表面涂覆不同厚度SiO₂薄膜的硅片样品进行了实验验证,发现实验与理论仿真得到的增益系数与测量误差随膜层厚度的变化规律一致。仿真与实验研究结果表明,调焦调平传感器的工艺相关性测量误差在SiO₂膜层厚度为250 nm和690 nm附近时分别出现约55.9 nm和36.6 nm的误差峰值。采用表面覆盖特定膜层的硅片来标定光刻机调焦调平传感器,可以有效减小增益系数工艺相关性的影响和测量误差。本研究结果对于光刻精密对焦控制、光刻工艺优化具有重要的参考意义。     

Mo/Si软X射线多层膜中厚度均匀性的精细控制

为了获得光学性质均匀的大面积软X射线多层膜,必须控制好周期结构中单层膜的厚度均匀性。为此建立了磁控溅射薄膜沉积技术中单层膜厚度均匀性的分析和控制模型,解释了基底变速转动法可用来获得膜厚均匀的多层膜,并根据理论分析获得了基底的变速路径。将其应用于基底公转速度变速法来制备均匀性可控的大面积Mo/Si软X射线多层膜。小角X射线衍射测试结果表明,采用优化后的变速路径制备的多层膜,样品不同位置的各级次衍射峰位都能很好吻合,说明多层膜的周期厚度基本一致。计算表明该方法在直径200mm范围内可将周期结构中Mo层的不均匀性从20.6%修正到1.1%,Si层的不均匀性从27.0%修正到1.6%。     

利用透射光谱与X射线反射谱精确测量溶胶-凝胶TiO2薄膜厚度和光学常数

在洁净K9玻璃基底上沉积TiO2薄膜,将透射光谱和X射线反射光谱相结合分析获得膜层的厚度和光学常数。X射线反射谱拟合能精确得到膜层的厚度、电子密度及表面和界面粗糙度,其中膜层厚度的数值为透射光谱的分析提供了重要参考。基于Forouhi-Bloomer色散模型拟合膜层透射光谱,得到薄膜折射率和消光系数,理论曲线和实验曲线吻合良好。对于同一样品,两种光谱拟合分析得到的厚度数值非常接近,差值最大为4.9nm,说明两种方法的结合能够提高光学分析结果的可靠性。     

Growth Rates of Edge-on Lamellar Crystals Confined in Polymer Thin Films

The growth rates of edge-on lamellar polymer crystals in variable thickness films were investigated in terms of dynamic Monte Carlo (MC) simulations. The growth rates linearly decreased with decreasing film thickness for the thinner films and were nearly constant for the thicker films. The mean stem lengths (crystal thickness) were also constant in different thickness films. The crystal widths parallel to the film thickness increased more slowly with increasing film thickness in the thinner films than that in the thicker films, indicating they were restrained by the film thickness. We propose that the growth rate of edge-on lamellar crystals in thin films is dominanted by the crystal width in the thinner films and by the crystal thickness in the thicker films; the variation of the film thickness can change the three-dimensional shape of the crystal growth front, also affecting the growth rate of the edge-on lamellar crystal.     

Raman micro‐spectroscopy for quantitative thickness measurement of nanometer thin polymer films

The sensitivity of far‐field Raman micro‐spectroscopy was investigated to determine quantitatively the actual thickness of organic thin films. It is shown that the thickness of organic films can be quantitatively determined down to 3 nm with an error margin of 20% and down to 1.5 nm with an error margin of 100%. Raman imaging of thin‐film surfaces with a far‐field optical microscope establishes the distribution of a polymer with a lateral resolution of ~400 nm and the homogeneity of the film. Raman images are presented for spin‐coated thin films of polysulfone (PSU) with average thicknesses between 3 and 50 nm. In films with an average thickness of 43 nm, the variation in thickness was around 5% for PSU. In films with an average thickness of 3 nm for PSU, the detected thickness variation was 100%. Raman imaging was performed in minutes for a surface area of 900 µm². The results illustrate the ability of far‐field Raman microscopy as a sensitive method to quantitatively determine the thickness of thin films down to the nanometer range. Copyright © 2015 John Wiley & Sons, Ltd.     

Crystallization Kinetics of Lamellar Crystals Confined in Polymer Thin Films

We used dynamic Monte Carlo simulations to investigate the crystallization kinetics of flat-on lamellar polymer crystals in variable thickness films. We found that the growth rates linearly reduced with decreasing film thickness for the films thinner than a transition thickness d_t , while they were constant for the films thicker than d_t . Moreover, the mean stem lengths (crystal thickness) we calculated decreased with film thickness in a similar way to the growth rates, and the intramolecular crystallinities we calculated confirmed the film thickness dependence of the crytsal thickness. Besides, the crystal melting rates in thin films were calculated and increased with decreasing film thickness. We proposed a new interpretation on the film thickness dependence of the crystal growth rate in thin films, suggesting that it is dominated by the crystal thickness in terms of the driving force term (l–l _min) expressed by Sadler, rather than the chain mobility based on experiments. The crystal thickness can determine whether a crystal grows or melts in a thin film at a fixed temperature, indicating the reversibility between the crystal growth and melting.     

Optical properties and structures of silver thin films deposited by magnetron sputtering with different thicknesses

A series of thin Ag films with different thicknesses grown under identical conditions are analyzed by means of spectrophotometer. From these measurements the values of refractive index and extinction coefficient are calculated. The films are deposited onto BK7 glass substrates by direct current (DC) magnetron sputtering. It is found that the optical properties of the Ag films can be affected by films thickness.Below critical thickness of 17 nm, which is the thickness at which Ag films form continuous films, the optical properties and constants vary significantly with thickness increasing and then tend to a stable value up to about 40 nm. At the same time, X-ray diffraction measurement is carried out to examine the microstructure evolution of Ag films as a function of films thickness. The relation between optical properties and microstructure is discussed.     

离子束溅射沉积不同厚度铜膜的光学常数研究

利用Lambda-900分光光度计对离子束溅射沉积不同厚度Cu膜测定的反射率和透射率,运用哈德雷方程,并考虑基片后表面的影响,对离子束溅射沉积的Cu膜光学常数进行了计算。结果表明,在同一波长情况下,膜厚小于100 nm的纳米Cu膜光学常数随膜厚变化明显;膜厚大于100 nm后,Cu膜的光学常数趋于一定值。Cu膜不连续时的光学常数与连续膜时的光学常数随波长变化规律不同;不同厚度的连续膜的光学常数随波长变化规律相同,但大小随膜厚变化而变化。     

Hydrophilicity of amorphous TiO2 ultra-thin films

The UV-light-induced hydrophilicity of amorphous titanium dioxide thin films obtained by radio frequency magnetron sputtering deposition was studied in relation with film thickness. The effect of UV light irradiation on the film hydrophilicity was fast, strong and did not depend on substrate or thickness for films thicker than a threshold value of about 12 nm, while for thinner films it was weak and dependent on substrate or thickness. The weak effect of UV light irradiation observed for the ultra-thin films (with thickness less than 12 nm) is explained based on results of measurements of surface topography, UV-light absorption and photocurrent decay in vacuum. Comparing to thicker films, the ultra-thin films have a smoother surface, which diminish their real surface area and density of defects, absorb partially the incident UV light radiation, and exhibit a longer decay time of the photocurrent in vacuum, which proves a spatial charge separation. All these effects may contribute to a low UV light irradiation effect on the ultra-thin film hydrophilicity.     

Thickness-dependent crystallization behavior of fast-growth phase-change amorphous films

The crystallization behavior of amorphous films embedded in substrates with thickness of several nanometers is investigated based on a thermodynamic model. It is found that there is an optimum layer thickness where the crystallization speed of the films is maximized with the lowest energy barrier for crystallization. This is induced by an energetic change from glass/substrate interface energy to crystal/substrate interface energy as the crystal size is larger than the film thickness during the crystallization. Thus, the crystallization speed in thin films is affected by its thickness.     

Formations and morphological stabilities of ultrathin CoSi₂ films

In this paper we investigate the formations and morphological stabilities of Co-silicide films using 1-8-nm thick Co layers sputter-deposited on silicon(100) substrates.These ultrathin Co-silicide films are formed via solid-state reaction of the deposited Co films with Si substrate at annealing temperatures from 450℃ to 850℃.For a Co layer with a thickness no larger than 1 nm,epitaxially aligned CoSi2 films readily grow on silicon(100) substrate and exhibit good morphological stabilities up to 600℃.For a Co layer thicker than 1 nm,polycrystalline CoSi and CoSi2 films are observed.The critical thickness below which epitaxially aligned CoSi2 film prevails is smaller than the reported critical thickness of the Ni layer for epitaxial alignment of NiSi2 on silicon(100) substrate.The larger lattice mismatch between the CoSi2 film and the silicon substrate is the root cause for the smaller critical thickness of the Co layer.     

Thickness dependence of the dynamics in thin films of isotactic poly (methylmethacrylate)

The film thickness dependence of both the glass transition temperature (T(g)) and the 1 kHz alpha relaxation were studied for thin films of isotactic Poly (methylmethacrylate) (i-PMMA) supported on aluminium substrates. Films in the thickness range 7-200 nm were studied. The ellipsometrically determined T(g) was found to show reductions for films thinner than 60 nm, with the largest observed reduction being 12 K for a 7 nm thick film. Measurements of the T(g) were also performed on i-PMMA films supported on silicon substrates. Dielectric studies of the temperature dependent 1 kHz alpha relaxation peak, showed that the position (T(alpha)) and shape of the peak have no film thickness dependence. This was shown to hold for films with one free surface and films with a 30 nm thermally evaporated capping layer. Capping the films was shown to have no effect on the thickness dependence of either T(g) or T(alpha). The implications of these results are discussed further and the different film thickness dependencies of T(g) and T(alpha) are discussed. This is done within the framework of the Vogel-Fulcher-Tamann (VFT) theory of glass forming materials and also in the context of the existence of a dynamic correlation length xi.     

Mg/B多层膜退火法中不同制备条件对MgB2超导薄膜性质的影响

用Mg/B多层膜退火的方法制备了一系列MgB₂超导薄膜,研究了退火温度、退火时间和薄膜厚度对于MgB₂薄膜性质的影响.厚度为250 nm的Mg/B多层膜经400 ℃低温退火后已经生成超导相,此厚度薄膜750 ℃下退火20—30 min实现最佳超导转变温度（T_c）.前驱膜分层厚度相同时,随着薄膜厚度减小MgB₂薄膜T_c明显降低,而且较薄的膜T_{c关键词： 2}超导薄膜')" href="#">MgB₂超导薄膜 电子束蒸发 超导成相