低能离子束方法制备Fe组分渐变的Fe-Si薄膜

利用质量分离的低能离子束技术 ,获得了Fe组分渐变的Fe Si薄膜。利用俄歇电子能谱法 (AES)、X射线衍射法 (XRD)以及X射线光电子能谱法 (XPS)测试了薄膜的组分、结构特性。测试结果表明 ,在室温下制备的Fe Si薄膜呈非晶态。非晶薄膜在 40 0℃下退火 2 0min后晶化 ,没有Fe的硅化物相形成。退火后Fe Si薄膜的Fe组分从表面向内部逐渐降低。

低能离子束方法制备重掺杂Fe的Si∶Fe固溶体

利用质量分离的低能离子束方法 ,以离子能量为 1 0 0 0 e V,剂量为 3× 1 0 1 7cm- 2 ,室温下往 p型 Si(1 1 1 )单晶衬底注入 Fe离子 ,注入的样品在 4 0 0℃真空下进行热处理 .俄歇电子能谱法 (AES)对原位注入样品深度分析表明 Fe离子浅注入到 p型 Si单晶衬底 ,注入深度约为 4 2 nm.X射线衍射法 (XRD)对热处理样品结构分析发现只有 Si衬底的衍射峰 ,没有其他新相 .X射线光电子能谱法 (XPS)对热处理样品表面分析发现 Fe2 p束缚能对应于单质 Fe的峰 ,没有形成 Fe的硅化物 .这些结果表明重掺杂 Fe的 Si∶ Fe固溶体被制备 .电化学 C- V法测量了热处理后样品载流子浓度随深度的分布 ,发现 Fe重掺杂 Si致使 Si的导电类型从 p型转为 n型 ,Si∶ Fe固溶体和 Si衬底形成 pn结 ,具有整流特性

Undercooling and Rapid Solidification of Nb-Si Eutectic Alloys Studied by Long Drop Tube

Niobium-silicide alloys have great potential for high temperature turbine applications. The two-phase Nb/Nb5Si3 in situ composites exhibit a good balance in mechanical properties. Using the 52 in drop tube, the effect of undercooling and rapid solidification on the solidification process and micro-structural characterization of Nb-Si eutectic alloy was studied. The microstructures of the Nb-Si composites were investigated by optics microscope (OM), X-ray diffraction (XRD) and scanning electron microscope (SEM) equipped with X-ray energy dispersive spectrometry (EDS). Up to 480 K, deep undercooling of the Nb-Si eutectic samples was successfully obtained, which corresponds to 25% of the liquidus temperature. Contrasting to the conventional microstructure usually found in the Nb-Si eutectic alloy, the microstructure of the undercooled sample is divided into the fine and coarse regions. The most commonly observed microstructure is Nb+Nb5Si3, and the Nb3Si phase is not be found. The change of coarseness of microstructure is due to different cooling rates during and after recalescence. The large undercooling is sufficient to completely bypass the high temperature phase field.

Si underlayer induced nano-ablation in AgInSbTe thin films

AgInSbTelSi thin films on glass substrates are prepared by dc magnetron sputtering at room temperature. Using Si underlayer as the thermal diffusion layer, the super-resolution nano-ablation holes with a size of 70nm in the AgInSbTe phase change films are obtained by a far-field focused laser experimental setup, with laser wavelength 405nm and objective-lens numerical aperture 0.90. The nano-ablation formation mechanism is analysed and discussed via the thermal diffusion of sample structures.

Si（111）衬底上ZnO薄膜的磁控溅射法制备及表征

采用磁控溅射法在(111)单晶硅衬底上沉积了ZnO薄膜，并研究了退火温度对ZnO薄膜晶体质量、晶粒度大小、应力和光致发光谱的影响。X射线衍射(XRD)表明薄膜为高度c轴择优取向。不同退火温度下的ZnO薄膜应力有明显变化。应力分布最为均匀的退火温度为500℃。室温下对ZnO薄膜进行了光谱分析，可观测到明显的紫光发射(波长为380nm左右)。实验结果表明，用磁控溅射法在单晶硅衬底上能获得高质量的ZnO薄膜。

退火对Si（111）衬底上ZnO薄膜的结构和发光特性的影响

采用磁控溅射法在硅（111）衬底上制备了C轴高度取向的ZnO薄膜，并研究了退火温度和氧气气氛对ZnO薄膜晶体质量、晶粒度大小和光致发光谱的影响。X射线衍射表明，所有薄膜均为高度C轴择优取向，当退火温度低于900℃时，随着退火温度的升高，薄膜的取向性和结晶度都明显提高。室温下对ZnO薄膜进行了光谱分析，退火后的样品均可观测到明显的紫光发射。在一定的退火温度范围内，还可以观测到明显的紫外双峰。空气中退火的样品，当退火温度达到或高于600℃还可观测到绿光发射。实验结果表明，发光峰强度随退火温度和氧气气氛不同而不

Intense upconversion and infrared emissions in Er3+;Yb3+ codoped Lu2 Si O5 and (Lu0.5 Gd0.5)2 Si O5 crystals

High optical quality Lu2SiO5 (LSO) and (Lu0.5Gd0.5)(2)SiO5 (LGSO) laser crystals codoped with Er3+ and Yb3+ have been fabricated by the Czochralski method. Intense upconversion (UC) and infrared emission (1543 nm) are observed under excitation of 975 nm. The luminescence processes are explained and the emission efficiencies are quantitatively obtained by measuring the UC efficiency and calculating the emission cross section. The temperature-dependent optical properties of the crystals are also investigated. Our study indicates that Er3+-Yb3+ : LSO and Er3+-Yb3+: LGSO crystals are promising gain media for developing the solid-state 1.5 mu m optical amplifiers and tunable UC lasers. (c) 2008 American Institute of Physics.

Mo原子溅射能量对Mo／Si薄膜微结构的影响

用磁控溅射法制备了Mo／Si薄膜，用AFM和XRD分别研究了Mo原子的溅射能量不同时，Mo／Si薄膜表面形貌和晶相的变化。通过比较发现，随着Mo原子溅射能量的增大，Mo／Si薄膜表面粗糙度增加，Mo和Si的特征X射线衍射峰也越来越强，并且Mo膜层和Si膜层之间生成了Mo-Si2。Mo原子的溅射能量是诱导非晶Si结晶和MoSi2生成的主要原因。

不同膜层数的Mo/Si多层膜的表界面粗糙度和软X射线反射率

用磁控溅射法制备了顶层分别是Mo膜层和Si膜层的两个系列的Mo/Si多层膜，它们的周期厚度相同但是膜层数各不相同。Mo/Si多层膜的周期厚度和界面粗糙度由小角X射线衍射（SAXRD）曲线拟和得到。用原子力显微镜测量了Mo/Si多层膜的表面粗糙度。在国家同步辐射实验室测量了Mo/Si多层膜的软X射线反射率。通过理论和试验研究，发现Mo/Si多层膜的软X射线反射率主要由周期数和界面粗糙度决定，表面粗糙度对Mo/Si多层膜的软X射线反射率影响较小。

研究扩散屏障层对Mo/Si多层膜软X射线反射率影响的模拟

在特定波长下,用四层结构模型模拟了Mo/Si多层膜的软X射线反射率.研究了扩散屏障层dMo-on-Si和dSi-on-Mo对Mo/Si多层膜软X射线反射率的影响.研究发现,扩散屏障层并不总是损害Mo/Si多层膜的光学性能,通过合理设计dMo-on-Si和dSi-on-Mo厚度,增加dMo-on-Si与dSi-on-Mo的比值,也能提高多层膜的软X射线反射率.

用不同的Mo靶溅射功率制备Mo／Si多层膜

用磁控溅射法制备了周期厚度和周期数均相同的Mo／Si多层膜，用原子力显微镜和小角X射线衍射分别研究了Mo靶溅射功率不相同时，Mo／Si多层膜表面形貌和晶相的变化。随后在国家同步辐射实验室测量了Mo／Si多层膜的软X射线反射率。研究发现，随着Mo靶溅射功率的增大，Mo／Si多层膜的表面粗糙度增加，Mo的特征X射线衍射峰也增强，Mo／Si多层膜的软X射线峰值反射率先增大后减小。

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。