升华能随温度和压力的变化及其对汽化反冲冲量的影响

 从普适的热力学原理出发,研究了升华能随温度和压力的变化。结果表明,升华能随温度或压力的增加而线性减小。采用光滑粒子流体动力学方法对金属铝在脉冲X射线辐照下的汽化反冲冲量进行了数值模拟,考察了升华能的变化对冲量的影响。结果表明,考虑升华能随温度和压力的变化后,冲量明显增加。     

非简谐振动对纳米金刚石表面性质的影响

借助米-里纳德-金斯势研究了纳米金刚石的Debye温度、表面能、表面压强、晶格参量随原子数和形状的变化规律, 探讨了非简谐振动和形状对其表面性质的影响.结果表明: 1)纳米金刚石的Debye温度和表面能随原子数的增多而增大, 其中杆状的Debye温度和表面能要小于立方形的值; 2)纳米金刚石的表面压强和低温时的晶格参量相对变化量随原子数N 的增多而减小,其中杆状的值要比立方形的值要大; 3)原子数较少时,非简谐振动效应和形状对纳米晶的Debye温度、表面能、 表面压强、晶格参量的影响显著.     

高压下Ni_3Al热力学性质的第一性原理研究北大核心CSCD

运用第一性原理方法结合准谐Debye-Grüneisen模型研究了高压下Ni3Al的热力学性质,拟合了Ni3Al的状态方程,计算了不同压强下Ni3Al的弹性模量及吉布斯自由能等热力学性质随温度的变化关系.计算结果表明:采用七阶Birch-Murnaghan方程拟合的晶格常数与实验测量结果吻合较好;零压下弹性模量、吉布斯自由能、焓、熵、热容和体膨胀系数随温度的变化与实验值符合较好;在特定压强下,Ni3Al的弹性模量和吉布斯自由能随温度升高而减小,焓、熵随温度升高而增加;预测的德拜温度约为500K,与实验值符合较好.     

高压下Ni3Al热力学性质的第一性原理研究

运用第一性原理方法结合准谐Debye-Grüneisen模型研究了高压下Ni3Al的热力学性质,拟合了Ni3Al的状态方程,计算了不同压强下Ni3Al的弹性模量及吉布斯自由能等热力学性质随温度的变化关系. 计算结果表明：采用七阶Birch-Murnaghan方程拟合的晶格常数与实验测量结果吻合较好;零压下弹性模量、吉布斯自由能、焓、熵、热容和体膨胀系数随温度的变化与实验值符合较好;在特定压强下,Ni3Al的弹性模量和吉布斯自由能随温度升高而减小,焓、熵随温度升高而增加;预测的德拜温度约为500K,与实验值符合较好.     

高温高压下合金碳化物Fe3Mo3C热力学性质的第一性原理计算

基于平面波赝势密度泛函理论的第一性原理与准谐德拜模型结合的方法研究了高温高压下合金碳化物Fe₃Mo₃C的热力学性质.在压强范围为0～40 GPa和温度范围为0～1200 K的条件下,Fe₃Mo₃C的体积比V/V₀、体弹性模量B和德拜温度θ受压强的影响比温度更大.温度一定时,体弹性模量和德拜温度随压强的增大而迅速增大. Fe₃Mo₃C的热容C_v、熵S以及热膨胀系数α受温度的影响较压强更大.压强一定时,材料的热容、熵以及热膨胀系数均随温度升高单调增大,其中,热容和热膨胀系数随温度先快速上升后趋于平缓,最后热容接近于Dulong-Petit极限.     

SrS相变和弹性性质的第一原理计算

利用平面波赝势密度泛函方法和准谐德拜模型研究了SrS从NaCl结构到CsCl结构的相变以及弹性性质.在零温下,我们计算的相变压强为17.9 GPa,这与实验值和其他作者的计算值符合很好.研究还表明:相变压强随温度增加而非线性地增加,然而力学不稳性的压强随温度增加而线性地增加.     

反钙钛矿结构RE_3AlC热物理性质理论研究

结合第一性原理和准谐德拜模型计算了RE_3AlC(RE=Sc、Y及镧系稀土)系列具有反钙钛矿结构碳化物的德拜温度、格律乃森常数、体积模量、自由能、比热容等热物理性质随着温度和压强变化的趋势。结果表明RE_3AlC碳化物的比热容、体积模量以及吉布斯自由能等随温度和压强变化的总趋势相似,其中RE_3AlC碳化物的体积弹性模量随着温度的升高而逐渐减小,同时随着压强的增加而增大;吉布斯自由能都随着温度的升高而降低,其中Sc_3AlC化合物的自由能最低,而Yb_3AlC化合物的自由能最高,表明Sc_3AlC化合物最稳定,而Yb_3AlC化合物稳定性最低;等容比热容随着温度和压强的变化在0-300 K温度段内变化较大,随后趋于平缓逐渐趋于杜隆.帕蒂极限值。     

温度和压强对金属化合物Co_2Zr和Co_2Ti的结构和热力学性质影响的研究

基于平面波赝势密度泛函理论(DFT)和广义梯度近似(GGA)的第一性原理计算了高温高压下金属化合物Co_2Zr和Co_2Ti的结构和热力学性质.Co_2Zr和Co_2Ti均为立方晶体,且结构类型为Cu2Mg结构.通过计算得出的晶格参数跟实验值符合较好.用准谐德拜模型计算了Co_2Zr和Co_2Ti的热力学性质.在0~100 GPa的压强和0~1500 K的温度作用下,两种物质的德拜温度Θ,热容CV,热膨胀系数α随压强和温度的变化而变化.随着压强的增大,德拜温度单调的增加;相同压强下,Co_2Ti的德拜温度始终大于Co_2Zr.热容CV和热膨胀系数α均随温度的增加而增加,增大压强时反而减小,说明减小温度和增大压强对CV以及α有相同的影响.     

气体压强对纳秒激光诱导空气等离子体特性的影响

环境气体的压强对激光诱导等离子体特性有重要影响.基于发射光谱法开展了气体压强对纳秒激光诱导空气等离子体特性影响的研究,探讨了气体压强对空气等离子体发射光谱强度、电子温度和电子密度的影响.实验结果表明,在10-100 kPa空气压强条件下,空气等离子体发射光谱中的线状光谱和连续光谱依赖于气体压强变化,且原子谱线和离子谱线强度随气体压强的变化有明显差别.随着空气压强增大,激光击穿作用区域的空气密度增加,造成激光诱导击穿空气几率升高,从而等离子体辐射光谱强度增大.空气等离子体膨胀区域空气的约束作用,增加了等离子体内粒子间的碰撞几率以及能量交换几率,并且使离子-电子-原子的三体复合几率增加,因此造成原子谱线OⅠ777.2 nm与NⅠ821.6 nm谱线强度随着气体压强增大而增大,在80 kPa时谱线强度最高,随后谱线强度缓慢降低.而离子谱线N Ⅱ 500.5 nm谱线强度在40 kPa时达到最大值,气体压强大于40 kPa后,谱线强度随压强增加而逐渐降低.空气等离子体电子密度均随压强升高而增大,在80 kPa后增长速度变缓.等离子体电子温度在30 kPa时达到最大值,气体压强大于30 kPa后,等离子体电子温度逐渐降低.研究结果可为不同海拔高度的激光诱导空气等离子体特性的研究提供重要实验基础,为今后激光大气传输、大气组成分析提供重要的技术支持.     

高压下TiC的弹性、电子结构及热力学性质的第一性原理计算

利用基于密度泛函理论的第一性原理平面波赝势方法 并结合准谐徳拜模型研究了NaCl结构的TiC在高压下的弹性性质、电子结构和热力学性质. 计算所得零温零压下的晶格常数、体弹模量及弹性常数与实验值符合得很好. 零温下弹性常数和弹性模量随压强增大而增大. 通过态密度和电荷密度的分析, Ti-C键随压强增大而增强. 运用准谐德拜模型, 成功计算了TiC在高温高压下的体弹模量、熵、热膨胀系数、徳拜温度、 Grüneisen参数和比热容. 结果表明压强对体弹模量、热膨胀系数和徳拜温度的影响大于温度对其的影响. 热容随着压强升高而减小, 在高温高压下, 热容接近Dulong-Petit极限.     

Sublimation du krypton à basse température

The sublimation of krypton at low temperature (25 ? T ? 50 K) is studied by means of high sentivity vibrating quartz microbalances. One of them supports, on its upper electrode, a condensed krypton crystal and allows the number of sublimated atoms per second to be measured, the temperature varying by steps. The evolution of the sublimation lobes versus temperature is determined by three others, situated in the same plane and respectively at 4°, 30° and 60° to the normal to the krypton crystal surface. The experimental results show the effects of radiation energy, partial pressure and thickness of krypton solid, on the krypton sublimation parameters. From the experimental results of the sublimation rate, the vapor pressure versus temperature and energy of activation of krypton sublimation are calculated and compared to results obtained by other authors. On the other hand for T < 42 K, the deviation of the sublimation lobe from Lambert's law increases as the temperature is lowered, i.e. for a lobe represented by cosⁿθ, n increases as T decreases.     

Considerations on the determining factors of the angular distribution of emitted particles in laser ablation

Simulations of particles which are emitted in laser ablation have been performed by the method of Direct Simulation Monte Carlo to investigate the deposition profiles of the emitted particles. The influences of the temperature, pressure and stream velocity of the initial evaporated layer formed during laser ablation process on the profile of the deposited film have been examined. It is found that the temperature gives a minor influence on the deposition profile, whereas the stream velocity and the pressure of the initial evaporated layer have a greater impact on the deposition profile. The energy in the direction of surface normal (E_⊥) and that in the parallel direction of the surface (E_||) are shown to increase and decrease, respectively after the laser irradiation due to collisions between the emitted particles, and this trend is magnified as the pressure increases. As a consequence, the stream velocity in the direction of surface normal increases with the increase in the pressure. A mechanism of the phenomenon that a metal with a lower sublimation energy shows a broader angular distribution of emitted particles is presented. It is suggested that low density of evaporated layer of a metal with a low sublimation energy at its melting point decreases the number of collisions in the layer, leading to the low stream velocity in the direction of surface normal, which results in the broader deposition profile of the emitted particles.     

Some theoretical considerations in modeling laser-induced incandescence at low-pressures

Laser-induced incandescence (LII) of nanoparticles at low pressures has received some attention in recent years as a particle sizing technique or a technique for inferring the mean value of the absorption function of the particle material. In this paper, we are concerned with some fundamental issues in the theory of LII with particular attention paid to those encountered at very low pressures. The commonly adopted Rayleigh approximation for particle laser energy absorption and subsequent thermal emission is critically evaluated against the Mie solution in the range of size parameter relevant to LII. The Rayleigh approximation can cause significant error in particle laser energy absorption rate, especially when shorter wavelengths are used, and potentially in the particle temperature inferred from the two-color LII. We also demonstrate that claims that low-pressure LII can be used for particle sizing are flawed, due to the use of an incorrect expression for radiation heat loss rate from the particles in this regime, and unjustified neglect of particle sublimation heat loss. Using the currently best available carbon sublimation rate expression and physical parameters, the relative importance of heat conduction, thermal radiation, and sublimation heat loss from an isolated carbon particle was investigated for different ambient pressures, particle temperatures and particle diameters. To ensure particle radiation heat loss is dominant over conduction and sublimation the ambient pressure and the particle temperature should be kept respectively lower than 10^-4 atm and below about 2800 K. Under these conditions the effective temperature of a particle ensemble containing non-aggregated polydisperse primary particles to the power of -4 is proportional to the mean value of the particle absorption function, provided the particles are in the Rayleigh regime in the near infrared. The effect of aggregation on particle absorption and emission is briefly discussed. PACS 44.10.+i; 44.40.+a; 61.46Df     

近空间升华法制备CdS多晶薄膜的研究

系统地研究了近空间升华法(CSS)制备CdS薄膜沉积速率的影响因素。发现CdS薄膜的沉积速率随升华源温度的升高而增大,但随衬底温度和沉积气压的上升而下降。对所制备样品的结构、表面形貌和光谱透过率特性进行了测试,结果表明：(1)不同氧分压下沉积的CdS薄膜沿(103)晶向择优生长。CdCl₂氛围下退火后,(103)晶向的优势得到进一步加强;(2)不同氧分压制备的CdS薄膜致密且粒径均匀,晶粒的大小随着衬底温度的升高而增大,但薄膜的粗糙度也随之增大;(3)随着CdS薄膜厚度的减小,可见光中短波段的透过率有所增大,有利于提高太阳电池的短波光谱响应。并将CSS制备的CdS多晶薄膜用于CdTe太阳电池的制作,获得了10.29%的光电转换效率,初步验证了该制作工艺的可行性。     

Sublimation inside an elastoplastic material

Thermodynamic and kinetic approaches for sublimation inside elastoplastic material under tensile stress are developed for large strains. Various conceptual problems related to irreversible plastic deformation are addressed for a spherical bubble. They include definitions of the thermodynamic driving forces and activation energies, nontraditional concepts of a critical nucleus, path dependence of its appearance, modes of its growth (sublimation or expansion due to loss of mechanical stability), and the possibility of reverse transformation. The kinetic relationships between sublimation pressure and temperature are obtained.     

Characteristics of the heating dynamics of a graphite conductor taking into account the skin effect

Calculations for a one-dimensional model of RF heating of a cylindrical graphite conductor have been carried out. The heating dynamics are analyzed in the general form. Conductor temperature profiles and the times for heating up to the graphite sublimation temperature as a function of current and frequency have been obtained. A model of conductor heating with partial return of the energy irradiated by the conductor surface has been considered. Frequency and current ranges have been determined to carry out this graphite sublimation method in a chamber with reflecting walls. The problem is associated with carbon vapor production and subsequent synthesis of fullerenes and other carbon structures.     

Formation of the second layer of krypton on the cleavage face of calcium iodide; Further evidence of the importance of entropy in physisorption

From the analysis of a set of stepped adsorption isotherms of krypton on the cleavage face of calcium iodide, it is concluded that, above 70.5 K, a second adsorbed monolayer is formed, having an apparent molar energy (algebraic value) and entropy higher than those of the bulk phase of the adsorbate. The differences in energy and entropy are exceptionally high for a second layer, and consequently, when the temperature is lowered below 70.5 K, the pressure corresponding to the second step becomes higher than the sublimation pressure and the step disappears. This unusual observation of a second dense monolayer existing only because of its high entropy, again emphasizes the fundamental importance of entropy in physical adsorption. It is secondarily noted that the isotherms present evidence of interparticle condensation occurring at high relative pressures.     

冻干过程中升华界面温度测量方法的研究

压力测温技术是基于在平衡状态下,冰晶温度与其饱和蒸汽压为单值函数这一基本规律,在升华干燥过程中,突然中断从冻干室流向冷阱的水蒸汽流,通过测量冻干室内压力回升情况去推算升华界面温度的一种非接触式测温方法。与热电偶或热敏电阻测温相比,压力测温技术即不破坏冻干样品的结构,又能够较为准确地反应出移动升华界面的温度,并能判断升华干燥过程终点。文中分析了升华界面温度测量的意义与困难,建立了压力测温技术的数学模型与分析方法,并通过实验研究了压力测温技术。     

Work functions and sublimation entropies of the elements

A phenomenological relationship between the work functions and the sublimation probabilities is shown to hold for most of the solid electron-conducting elements at the same vapor pressure. According to this relationship, the sublimation probabilityf increases exponentially with decreasing work functionW, i.e.,f∝exp(−W/W _o), whereW _o=0.60 eV. On the basis of a direct evaporation model, it follows that the work function is directly proportional to the sublimation entropy. This connection between two quantities, which seemingly refer to either electrons or atoms, respectively, is explained by expressing the sublimation entropy as the difference between the entropies of the gas and solid phases in equilibrium, and by deriving implications on the material properties contained in these individual entropies. The work function can thus be related to the second derivative of the crystal energy with respect to the atomic radius, which is corroborated by a universal relation between the work functions and the compressibilities for over 60 elements. For elements with a simple electron structure, the second derivative of the energy-atomic-radius dependence is essentially determined by a truly electronic property, namely the Fermi energy. It is shown that the Fermi energy variation is accompanied by a sufficient variation of the electron affinity in order to account for the appropriate work function change. For elements with a more complicated electron structure, a case-by-case study of the second derivative of the energy-atomic-radius dependence is required.