类Kerr介质中双模SU(1,1)相干态场与Λ型三能级原子相互作用的量子统计性质

导出了类Kerr介质中双模SU(1,1)相干态场与Λ型三能级原子相互作用系统的态函数,研究了Kerr效应对Λ型三能级原子布居概率、双模SU(1,1)相干态场的互关联函数、Cauchy-Schwartz不等式及二阶相干度的影响.结果表明:Kerr效应使原子与光场的耦合减弱,原子布居的崩塌与复苏的周期缩短;在初始光场较弱和较强两种情况下,类Kerr介质对双模SU(1,1)相干态场两模间的相关性、相关程度以及光子的聚束与反聚束效应产生的作用有明显的区别.     

脉冲中立型时滞抛物方程的振动性

本文研究了一类脉冲中立型时滞抛物方程解的振动性及强振动性,获得了此类脉冲中立型时滞抛物方程解振动和强振动的代数判据.     

铁路先简支后连续梁极限承载力研究

采用等幅重复加载和按比例分级加载法,对3根铁路预应力混凝土先简支后连续模型梁进行破坏试验,对带有湿接缝的该类型结构极限承载力进行试验研究。将理论分析结果与试验结果进行比较,结果表明,疲劳荷载对带有湿接缝的该类型结构极限承载力的降低程度约为10%。     

浅谈30m预制T梁的常见问题与防治

本文介绍了镇胜高速公路第二合同段十三旗大桥和天生高架桥在30mT梁预T梁施工中遇到的一些常见问题及处理措施。     

AFS-230型双道原子荧光光度计的安装与验收

本文简述北京海光仪器公司生产的ＡＦＳ 2 30型双道原子荧光光度计安装条件的要求、安装过程应注意的问题以及如何调试验收指标。1　仪器安装1.1　拆箱检查包装箱有无变形和受损 ,取出仪器 ,检查外观有无损坏 ;对照装箱单检查各配套件及备件是否齐全。1.2　仪器使用环境条件室内工作温度 :15～ 35℃、湿度≤ 75 % ;仪器应远离强电磁场及冲击振动源 ;由于所测试的元素为有毒物质 ,为保证工作人员的安全 ,本仪器应配有强制排风系统。1.3　电源仪器供电电压为 (2 2 0± 2 2 )Ｖ、频率为 (5 0± 1)Ｈｚ的正弦交流电源 ,消耗功率 >10 0 0Ｗ ,电压…     

p型导电掺In的SnO_2薄膜的制备及表征

采用溶胶 凝胶提拉法成功地制备了p型导电掺In的SnO2 薄膜 .x射线衍射测试结果表明 ,掺In的SnO2 薄膜保持SnO2 的金红石结构 .吸收谱测试结果表明 ,掺In的SnO2 禁带宽度为 3 8eV .霍尔测量结果表明 ,空穴浓度与热处理温度有很大的关系 ,5 2 5℃为最佳热处理的温度 .铟锡原子比在 0 0 5— 0 2 0范围内 ,空穴的浓度与In的含量有直接的关系 ,并随In含量的增加而增加     

小型企业规模的有效性分析

在当代企业纷纷追求规模的不断扩大的同时，统计数据却显示企业平均规模不断下降的事实趋势。论根据数学、经济学与博弈论的有关理论对企业规模小型化的内在要求进行了探讨，分析的结论一致证明：粘型化规模在当代经济环境中是充分有效的。     

Chiral Parameter of Transparent Films Containing Polymer Cholesteric Liquid Crystal-R

The transparent film containing a kind of polymer cholesteric liquid crystal-R was fabricated by the freezing method. The optical polarization response of the film was investigated by a self-manufactured apparatus and its optical rotatory dispersion was measured by a novel technique at the wavelength from 35Onto to 66Onto.At various wavelengths, the chiral parameter of the film has been obtained. The results show that the chiral parameter decreases as the wavelength increases. The maximum and minimum chiral parameters are 0.0343 at the wavelength of 350 nm and 0.0058 at the wavelength of 660 nm, respectively. The obtained data indicate that this kind of polymer cholesteric liquid crystal-R is a promising candidate host material for solid optical chiral waveguides.     

Proton Fraction in Neutron Star Matter and Three-Body Force Effects

The three-body force effects on the equation of state and its iso-spin dependence of asymmetric nuclear matter and on the proton fraction in neutron star matter have been investigated[1] within Brueckner Hartree-Fock (BHF) approach by using a microscopic three-body force. It is shown that, even in the presence of the three-body force, the empirical parabolic law of the energy per nucleon vs. isospin asymmetry β=(N-Z)/A is fulfilled in the whole asymmetry range 0 ≤β ≤1 and also up to high density. The three-body force provides a strong enhancement of symmetry energy at high density in agreement with relativistic approaches. Thecalculated proton fraction in β stable neutron star matter is given in Fig.l, where the thick solid line is the BHF prediction using AV18 TBF, while the dotted one is the BHF result using AVis. The thin solid line is the prediction of the Dirac-Brueckner approach taken from Ref.[2]. The results extracted according to the phenomenological paramete rizations of the symmetry energy suggested in Ref.[3] are also plotted. It is seen from