殊途同归的光本性之争

 很久以来,人们对光就进行了各种各样的研究。光的本性到底是什么,这个问题长久以来困扰了很多有智之士。光的波动说笛卡儿（R.Descartes,1596～1650）就光的本性问题,在1637年提出两种假说。一种假说认为,光是类似于微粒的一种物质;另一种假说认为光是一种以“以太”为媒质的压力。虽然笛卡儿更强调媒介对光的影响和作用,但他的这两种假说为17世纪的微粒说和波动说的争论埋下了伏笔。17世纪中期,意大利的格里马第（F.Grimaldi,1618～1663）首先注意到衍射现象,这是光的波动理论的萌芽。     

用变形全息透镜实现变形分数傅里叶变换

利用一发散点光源和一束倾斜平行光制作出在两个垂直方向上具有不同焦距的变形全息透镜,且用此全息元件实现了变形分数傅里叶变换。变形全息透镜两个方向上的焦距随全息记录条件和再现条件而变化,分析了用这种全息透镜实现变形分数傅里叶变换的条件。实验表明,用该元件能够方便地实现任意级次的变形分数傅里叶变换。     

V型三能级原子与非经典光场作用中光场特性的变化

研究了V型三能级原子BEC与双模压缩光场相互作用系统中,忽略原子间相互作用和考虑原子间相互作用时光场的正交压缩和光子数压缩。结果表明,光场的正交压缩依赖于压缩参数,而光子数压缩与压缩参数、光场信号强度有关,在一定条件下,两种压缩可同时存在。原子间相互作用影响两种压缩的涨落随时间变化的周期,以及正交分量涨落随时间变化的幅度,而对光子数压缩涨落随时间变化的幅度几乎无影响。     

Nonlinear Effects for Bose Einstein Condensates in Optical Lattices

Cold atoms and, more recently, Bose-Einstein condensates （BEC＇s） in optical lattices have attracted increasing interest since their first realization. In particular, the formal similarity between the wavefunction of a BEC inside the periodic potential of an optical lattice and of the electrons in a crystal lattice has triggered theoretical and experimental efforts alike. Many phenomena from condensed matter physics, such as Bloch oscillations and Landau-Zener tunneling have been shown to be observable also in optical lattices. An important difference between electrons in a crystal lattice and a BEC inside the periodic potential of an optical lattice is the strength of the self interaction and hence the magnitude of the nonlinearity of the system. Electrons in a metal are almost noninteracting, whereas atoms inside a BEC interact strongly. A＇ perturbation approach is appropriate in the former case while in the latter the full nonlinearity must be taken into account. From this feature new physics is expected. Most experiments to date have been carried out in the regime of shallow lattice depth, for which the system is well described by the mean field Gross-Pitaevskii equation with a periodic potential. Moreover, the nonlinearity induced by the mean-field of the condensate has been shown, both theoretically and experimentally, to give rise to instabilities in certain regions of the Brillouin zone. These instabilities are not present in the corresponding linear system, i.e. the electron system. Experimental and theoretical results on the subject of nonlinear Landau-Zener tunneling and nonlinearity-induced instabilities in a Bose-Einstein condensate interacting with an external periodic potential will be presented.     

三维光晶格中玻色凝聚气体基态波函数及干涉演化

基于Gross-Pitaevskii方程，运用有效化学势概念，研究了囚禁在组合势(由磁阱和三维光 晶格组成)中玻色凝聚气体在三维光晶格中的分布规律，并由此得到玻色凝聚气体的归 一化基态波函数.在取消组合势和仅取消光晶格而保留磁阱的两种情况下，运用传播子方 法求解出玻色凝聚气体密度分布的解析表达式.取消组合势后，理论计算所得到的玻色凝聚 气体聚随时间的演化规律与Greiner等的实验结果相一致.仅取消光晶格而保留磁阱时，研 究表明玻色凝聚气体的干涉模式呈现周期性的振荡行为.此外，在磁阱为各向异性的情况下 ， 关键词： 玻色凝聚气体 磁阱 光晶格 干涉模式     

应该界定黑洞的“最大半径”和“最小半径”

 有关黑洞的习题在近几年的复习资料中经常出现,通过题中给出的一些有关物理量来估算黑洞的“最大半径”。那么什么是黑洞?一颗内部燃烧尽了的大质量恒星由于自身的引力作用,外壳不断向中心坍塌缩小,最后就会形成致密的黑洞。黑洞是宇宙中的实体微粒,它们的体积趋向于零,而密度几乎是无穷大,由于具有强大的引力,物体只要靠近这个微粒,就会被强大的引力吸入,连光也不能幸免。也就是说,没有任何信号能够从黑洞的作用范围内传出,人类无法看到里面的情形---对于观测者来说,那就是漆黑一片---这也是黑洞名字的由来。既然如此,那么衡量黑洞的大小只能用其作用范围(即“视界”)的“半径”来表示。     

Synthesis of 2-Acyl-2H-1,2,3-diazaphospholes and Their Diels-Alder Reaction with Cyclopentadiene

2H-1,2,3-Diazaphospholes 3a-3h were prepared from various ketone acylhydrazones and phosphorus trichloride in the presence of triethylamine. Compounds 3 underwent feasible hetero-Diels-Alder reactions with cyclopentadiene to afford the respective anellated [1,2,3]diazaphospholes 4a--4d as well as 4a‘--4d‘ in moderate yields. The endo rule in the reaction was observed under kinetic control conditions.     

与q形变玻色算符逆算符相关的相干态及其量子统计性质

讨论了ｑ形变玻色算符的广义逆算符作用于ｑ－相干态所得到的两类量子态的数学及量子统计性质。结果表明，ｑ－相干态的光子激发态不存在压缩但呈现反聚束效应，而ｑ－相干态的光子湮灭态却存在压缩但不呈现反聚束效应。     

稀有衰变B0(Bs)→γv(-v)分支比的计算

在标准模型中,三体稀有衰变B0(Bs)→γv(-v)只有通过箱图和企鹅图才可以发生.这个过程对于确定B介子的衰变常数及其波函数有着较重要的物理意义,由于这些衰变道的分支比较小,因此也是探测新物理理论的比较好的场所.利用B介子强衰变确定的波函数,得到B0(Bs)→γv(-v)的分支比的数量级是10-9(10-8),这些结果可以在未来的实验上得到检验.