Duration-Dependent Asymmetry in Photoionization of H atoms in Few-Cycle Laser Pulses

The photoionization of H atoms irradiated by few-cycle laser pulses is studied numerically. The variations of the total ionization, the partial ionizations in opposite directions, and the corresponding asymmetry with the carrier-envelope phase in several pulse durations are obtained. We find that besides a stronger modulation on the partial ionizations, the change of pulse duration leads to a shift along carrier-envelope （CE） phase in the calculated signals. The phase shift arises from the nonlinear property of ionization and relates closely to the Coulomb attraction of the parent ion to the ionized electron. Our calculations show good agreement with the experimental observation under similar conditions.     

多维测量结果不确定度评价方法初探

为解决以多维矢量形式存在被测对象的测量质量评定问题,该文应用测量不确定度理论和多元概率统计方法,将测量不确定度理论进行了向多维的拓展;对多维情况下的测量不确定度传播律进行了推导;论述了多维不确定度的表示方法及空间几何意义;提出了以多维不确定度比较不同测量结果质量的方法;并给出了常用多维测量方法,如等精度独立多维测量和不等精度独立多维测量的不确定度评定方法。理论分析及仿真算例表明,所提出的理论具有较完备的体系,能够满足测量实际中常用多维测量方法的不确定度评定需求。     

电话机产品测量不确定度评定的研究

本文简单介绍了测量不确定度的一般评定程序,并列举了电话机产品检测不确定度评定的实际应用案例,即电话机双音多频信号电平的测量结果的不确定度评定。     

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     

关于算子方程AX=XAX与AX=XA=XAX

用A的不变子空间作参数，给出了算子方程AX＝XAX的全部解。当A是单射或稠值域时，或者当A是正规算子时，给出了算子方程AX＝XA＝XAX的全部解。我们还给出正规算子X是算子方程AX＝XZ＝XAX的解的充分必要条件。     

广义不确定原理对一般静态黑洞熵的影响

把广义不确定原理引入黑洞熵的计算,采用薄膜brick-wall模型,对一般静态黑洞外部标量场的熵进行了计算,得到了熵计算公式.应用该公式结果表明,可以得到已知所有静态黑洞的Bekenstein-Hawking熵.作为比较和进一步研究,对视界面上的二维膜的熵进行计算,可以更方便和一般性地得到熵与视界面积成正比的结论,该讨论可直接表明黑洞熵就是其视界面上的量子态的熵.与原始brick-wall模型不同的是,这一结论是有限的,计算中无需引入截断,且小质量近似也可以避免.     

约束Hamilton系统的Poincaré-Cartan不变量

从正则形式作用量出发,导出了约束Hamilton系统(奇异拉氏量)的Poincaré-Cartan不变量,证明了该不变量与约束Hamilton系统的正则方程之间的等价性,纠正了某些作者工作中的错误。     

有界随机变量的次高斯性

通过建立一些重要的不等式，研究有界随机变量的性质，得出了重要结果：数学期望为零的有界随机变量是次高斯的，并得出参数τ的精确估计。最后应用这些结果构造一个非对称的次高斯变量，并研究了某些随机三角级数的性质，得到了很好的结果。     

对不均匀沉降引起墙体裂缝的分析

概述了墙体裂缝三种主要形式；分析了造成裂缝的因素；提出了防止不均匀沉降造成裂缝的措施。