大口径非球面主反射镜的装调方法研究

针对大口径非球面主反射镜（简称主镜）的装调要求,对比分析常用大口径非球面面形检测方法,提出该类主镜检测面形的最佳方案。在主镜的装调过程中,通过对主镜的固定方式和主镜变形补偿这2个关键环节的阐述,总结主镜固定的难点及主镜变形的原因,提出一套全新的装调方案,以旋转消重力法进行检测,并用专用工装实时定心调节,再用辅料焊接法固定主镜与中心轴,最后采用辅助支撑对主镜组件进行最终固定修正。装调结果表明:对于大口径非球面反射镜,装调完成后的主镜面形精度Rms0.03（＝632.8 nm）。     

多体相互作用体系中的弛豫与扩散:一个尚未解决的问题

文章目的在于引起国内研究团体对一系列复杂相互作用体系中的弛豫和扩散的普适性进行关注.研究发现,无论是不同的化学结构(如无机物、有机物、聚合物、生物分子、胶体、金属和离子导电材料),还是不同的物理状态(如晶态、玻璃态、液体、熔体、混合体系和含水系统),以及不同的尺度(如从块体至纳米),这种普适性无处不在[K.L.Ngai.Relaxation and Diffusion in Complex Systems.NewYork:Springer,2011].该现象起源于多体系统的不可逆过程,取决于一些基本物理定律,与非简谐势引发的经典混沌有关.重新认识这种普适性不仅对众多不同领域的发展有利,而且能进一步弄清楚多体系统中的弛豫与扩散问题——一个重要而又未解决的物理问题.作者提出的耦合模型尽管不是一个严格而完整的答案,但却能够预测多体系统的弛豫和扩散特征,而且与实验结果吻合.基于该模型,绝大多数多体系统中的弛豫与扩散行为是相似的.该模型有望为这一难题的彻底解决奠定基石.     

Hadron spectroscopy from B-factories

We review the recent experimental results on hadron spectroscopy from B-factories focusing on the exotic charmonium-like states.Among them we discuss the X（3872）,Y（3940）,Z（4430） ＋,Z（4050） ＋,Z（4250） ＋ and Y（4140） states found in B-meson decays,the X（3940） and X（4160） states produced in double charmonium production,the Y（4260）,Y（4325）,Y（4660） and X（4630） states produced with initial-state radiation in e ＋ eannihilation and the X（3915）,Y（4350） states observed in two-photon collisions.     

边界元法求解金属凝固过程逆热传导问题

本文针对一个金属凝固过程的逆热传导问题,即由金属表面温度求其表面热流的问题,提出了一种基于边界元法的求解算法;并且利用离散化后的数值计算验证了该算法的有效性。     

Study of absorption and re-emission processes in a ternary liquid scintillation system

Liquid scintillators are widely used as the neutrino target in neutrino experiments.The absorption and emission of different components of a ternary liquid scintillator （Linear Alkyl Benzene （LAB） as the solvent,2,5-diphenyloxazole （PPO） as the fluor and p-bis-（o-methylstyryl）-benzene （bis-MSB） as wavelength shifter） are studied.It is shown that the absorption of this liquid scintillator is dominant by LAB and PPO at wavelengths less than 349 nm,and the absorption by bis-MSB becomes prevalent at the wavelength larger than 349 nm.The fluorescence quantum yields,which are the key parameters to model the absorption and re-emission processes in large liquid scintillation detectors,are measured.     

Aggregation Processes with Catalysis-Driven Decomposition

We propose a three-species aggregation model with catalysis-driven decomposition. Based on the mean-field rate equations, we investigate the evoIution behavior of the system with the size-dependent catalysis-driven decomposition rate J（i; j; k） = Jijk^v and the constant aggregation rates. The results show that the cluster size distribution of the species without decomposition can always obey the conventional scaling law in the case of 0 ≤v ≤ 1, while the kinetic evolution of the decomposed species depends crucially on the index v. Moreover, the total size of the species without decomposition can keep a nonzero value at large times, while the total size of the decomposed species decreases exponentially with time and vanishes finally.     

Experimental study of the time-resolved reflectivity of chromium film

The transient time-resolved reflectivity of chromium film is studied by femtosecond pump-probe technique with a 70-fs laser. Experimental results show that the reflectivity change increases with the power of the pump laser. The fast decrease of the reflectivity occurs between 0-200 fs which is mainly due to the electron-electron interaction. Subsequencely, the slower recovery of the reflectivity between 200-900 fs is mainly due to the electron-phonon coupling process. The reflectivity after 900 fs rises little to a near-constant value for the thermal equilibrium of the system. The experimental results can be explained properly with numerical simulation of the two-temperature model. It is helpful for understanding of the electron ultrafast dynamics in chromium film.     

极化子效应对ZnS/CdSe量子点三阶极化率的影响

在有效质量近似下,利用量子力学的密度矩阵理论,采用无限深势阱模型,从理论上计算了考虑极化子效应后在导带子带间跃迁时ZnS/CdSe柱型核壳结构量子点二次电光效应(QEOE)和电吸收过程(EA)的三阶极化率。通过数值计算,分析了电子-LO声子和电子-IO声子相互作用对ZnS/CdSe柱型核壳结构量子点二次电光效应和电吸收过程的三阶极化率的影响。结果表明,极化子效应对二次电光效应的三阶极化率χ⁽³⁾_QEDE和电吸收过程的三阶极化率χ⁽³⁾_EA都有很大影响,并且影响的大小与量子点的尺寸大小有关。     

地震动力:由巨观到微观——1999年台湾集集地震

决定地震发生时的断层破裂能量和了解一个断层带的孕育与发展都需要地震和地质数据的结合.在一个大地震的发生过程中,藉由地震仪的记录分析,了解地震断层破裂过程中其断层的几何破裂行为及其机制,甚至分析其运动学上的灾害行为.在地震源分析中文章作者将以上行为分析称为地震的巨观分析.而地震的微观分析,则是以探讨当地震断层及破裂前缘持续向前前进时,其所需的破碎能量及其形成的极小颗粒之断层泥的物理化学机制.此断层滑移带中的断层泥之物理机制、化学组成及地震断层滑移带厚度,皆为了解地震滑移时摩擦行为及能量释放的重要参数.地震的巨观及微观行为的结合分析,为地震学上重要的突破,使人们得以进一步了解地震破裂过程中的摩擦行为、温度及压力的变化,并探讨地震时造成的地表位移、速度及加速度行为.但断层滑移带的断层泥并小易获得,除非有清楚的深部断层几何,并能以深钻的方式取得断层泥材料进行分析.1999年7.6级的台湾集集大地震产生地表或近地表8-12m的滑移,此近地表的滑移足钻井容易达成的,因此提供一次难得的机会,得出大地震滑移带的断层泥了解大滑移断层的动力机制.而2008年四川汶川地震为另一了解此巨观与微观机制的地震.     

Vacuum Outer-Gap Structure in Pulsar Outer Magnetospheres

We study the vacuum outer-gap structure in the outer magnetosphere of rotation-powered pulsars by considering the limit of trans-field height through a pair production process. In this case, the trans-field height is limited by the photon-photon pair production process and the outer boundary of the outer gap can be extended outside the light cylinder. By solving self-consistently the Poisson equation for electrical potential and the Boltzmann equations of electrons/positrons and γ-rays in a vacuum outer gap for the parameters of Vela pulsar, we obtain an approximate geometry of the outer gap, i.e. the trans-field height is limited by the pair-production process and increases with the radial distance to the star and the width of the outer gap starts at the inner boundary （near the null charge surface） and ends at the outer boundary which locates inside or outside the light cylinder depending on the inclination angle.