Nb掺杂ZnO透明导电薄膜的结构以及光电性能研究

采用直流磁控溅射法在玻璃衬底上制备了高质量的Nb掺杂ZnO( NZO)透明导电薄膜.为了研究薄膜厚度对薄膜性质的影响,制备了五个厚度分别为239 nm,355 nm,489 nm,575 nm和679 nm的样品.XRD结果表明,ZnO∶ Nb薄膜是具有六角纤锌矿结构的多晶薄膜,并且具有垂直于衬底的c轴择优取向.随着膜厚的增加,薄膜的结晶质量明显提高.当厚度从239 nm增加到489 nm时,平均晶粒尺寸从19.7 nm增加到24.7 nm,薄膜的电阻率持续减小;当厚度进一步增加时,晶粒尺寸略有减小,电阻率有所增加.本实验获得的最低电阻率为4.896×10-4Ω·cm.随膜厚的增加,光学带隙先增大后减小.所有薄膜在可见光区域的平均透过率均超过88.3;.     

直流磁控溅射法制备铝铬共掺杂氧化锌薄膜及其结构和光电性能的研究

利用直流磁控溅射法在玻璃衬底上制备了铝铬共掺杂氧化锌(ZACO)透明导电薄膜.通过X射线衍射(XRD)和扫描电镜(SEM)等表征方法对薄膜特性进行测试分析,研究了溅射压强和溅射功率对薄膜生长速率以及光电特性的影响.结果表明,随着溅射气压(1.5～4.5 Pa)的增大,薄膜沿c轴方向的结晶质量提高,薄膜表面更加致密,晶粒大小更加均匀.薄膜生长率随压强的增大而减小,但电阻率先减小后增大.当溅射功率由80 W增大到100 W时,薄膜的生长速率增大,电阻率减小.溅射压强为3.5 Pa,溅射功率为100 W时,薄膜的电阻率达到最小值2.574×10-3 Ω·cm.紫外-可见透射光谱表明,所有薄膜在可见光区的透过率均超过89.9;.     

Study on the phase transition of the fractal scale-free networks

Based on the Ising spin, the phase transition on fractal scale-free networks with tree-like skeletons is studied, where the loops are generated by local links. The degree distribution of the tree-like skeleton satisfies the power-law form P(k)～ k~(-δ).It is found that when δ≥3, the renormalized scale-free network will have the same degree distribution as the original network. For a special case of δ = 4.5, a ferromagnetic to paramagnetic transition is found and the critical temperature is determined by the box-covering renormalization method. By keeping the structure of the fractal scale-free network constant, the numerical relationship between the critical temperature and the network size is found, which is the form of power law.     

溅射功率对铝铬共掺杂氧化锌透明导电薄膜特性的影响(英文)

室温下,利用直流磁控溅射法在玻璃衬底上制备了铝铬共掺杂氧化锌薄膜,研究了溅射功率(55-130 W)对薄膜结构、残余应力、表面形貌及其光电性能的影响。结果表明,ZnO(002)衍射峰的强度随着溅射功率的增大而增强,晶体结构得以改善。晶格常数、压应力和电阻率均随着溅射功率的增大而减小。当溅射功率为130 W时,制备的ZnO∶Al,Cr薄膜的最低电阻率可达1.09×10-3Ω.cm。功率由55 W增大到130 W时,光学带隙由3.39 eV增大到3.45 eV。紫外-可见透射光谱表明,所有薄膜在可见光范围内平均透过率均超过89%。     

Magnetic Instability in Accretion Disks with Anomalous Viscosity

Using the new model of anomalous viscosity, we investigate the magnetic instability in the accretion disks and give the dispersion formula. On the basis of the dispersion relation obtained, it is numerically shown that the instability condition of viscous accretion disk is well consistent with that of the ideal accretion disk, namely there would be magneto-rotational instability in the presence of a vertical weak magnetic field. For a given distance R from the centre of the disk, the growth rate in the anomalous case deviates from the ideal case more greatly when the vertical magnetic field is smaller. The large viscosity limits to the instability. In the two cases, the distributions of growth rate with wave number κ approach each other when the magnetic field increases. It greatly represses the effect of viscosity.     

BN织构陶瓷的制备与力学性能研究

以片状的BN为基体粉料,采用流延成型工艺结合热压烧结制备BN织构陶瓷,并对其结构、断面形貌以及力学性能进行了研究.实验结果表明,BN晶粒选择沿(002)晶面择优定向排列.织构陶瓷的力学性能呈现出明显的各向异性: 当加载方向垂直于片层时,弯曲强度和断裂韧性分别为53.75 MPa 和1.51 MPa·m1/2,均优于水平方向的力学性能.垂直方向上良好的性能归因于加载时片状颗粒引起的裂纹偏转.