大能量损失几何条件下剩余电子屏蔽效应的理论研究

通过考虑末通道 中剩余电子的屏蔽效应,用BBK模型及修正方案在大能量损失小动量转移几何条件下对电子电离氦原子的三重微分截面进行了计算,并从物理本质上系统地研究和分析了剩余电子的屏蔽效应在大能量损失几何条件下对三重微分截面所产生的影响.     

730 eV电子碰撞He原子(e, 2e)电离的三重微分截面

考虑初态He原子电子间的关联效应、末态敲出电子与剩余束缚电子间的关联效应和末态屏蔽效应, 计算和分析了在共面、大能量损失和小动量转移这一特殊几何条件下730eV电子离化He原子的三重微分截面. 所得结果与Stevenson等人的相对实验数据和CCC理论计算结果进行比较发现: 所得到的理论曲线能够反映实验数据给出的三重微分截面的结构特征.     

730 eV电子碰撞He原子(e, 2e)电离的三重微分截面

考虑初态He原子电子间的关联效应、末态敲出电子与剩余束缚电子间的关联效应和末态屏蔽效应, 计算和分析了在共面、大能量损失和小动量转移这一特殊几何条件下730eV电子离化He原子的三重微分截面. 所得结果与Stevenson等人的相对实验数据和CCC理论计算结果进行比较发现: 所得到的理论曲线能够反映实验数据给出的三重微分截面的结构特征.     

非共面索末菲参量对三重微分截面的影响

考虑末通道He⁺中剩余电子的屏蔽效应之后,在非共面几何条件下利用3种不同的修正方案,详细地比较并研究了不同索末菲参量在非共面双对称几何条件下对He原子 (e, 2e) 反应中三重微分截面所产生的影响.讨论了产生这种影响的物理本质. 关键词： 非共面 双对称几何条件 三重微分截面 索末菲参量     

大能量损失几何条件下末态屏蔽效应和交换效应的理论研究

用BBK（Brauner, Briggs, Klar）模型和修正后的BBK模型在大的能量损失几何条件下对氦原子的三重微分散射截面进行了理论计算和研究,并把计算结果与Catoire等的实验测量结果以及Stevenson等的最新实验测量结果进行了比较,对作者早期文章的理论推论进行了验证,并对交换效应作了系统的研究. 关键词： binary峰 recoil峰 屏蔽效应 交换效应     

垂直入射几何条件下氦原子(e,2e)反应的理论研究

用BBK模型和修正后的BBK模型在电子垂直入射几何条件下对氦原子的三重微分散射截面进行了理论计算,并把计算结果与实验测量结果进行比较,对截面的结构进行了分析,并对交换效应进行了系统的研究. 关键词： DS3C模型 中间峰 屏蔽效应 交换效应     

H原子(e,2e)反应中电子角分布的理论研究

使用3C和DS3C模型,计算了不同入射能情形下电子入射离化H原子的三重微分截面,并对截面的结构进行了分析.结果表明:角分布基本上由两个峰组成,即binary峰和recoil峰.两个峰的形状和位置对两个出射电子的能量分配及探测的几何条件十分敏感.更进一步,末态电子与电子的排斥对形成观测到的角分布有显著的贡献,在不同几何条件下,三体相互作用通过不同散射幅的不同权重控制了干涉花样.此外,对直接和交换效应也都进行了研究. 关键词： 角分布 binary峰 recoil峰     

Ag+(4d10)离子三重微分截面的研究

用自旋平均静态交换势下的三体扭曲波波恩近似计算了d轨道电子(Ag+(4d10))在共面非对称几何条件下的三重微分截面, 结果表明在高入射能的条件下, 随散射电子角度θa的增加, binary峰和recoil峰分裂的个数都会增加, 电子的电离振幅会随之下降, d电子的三重微分截面比s, p电子的复杂.     

电子垂直入射电离氦原子碰撞机理的理论研究

用3C模型和修正后的3C模型在低能、两个出射电子等能分享几何条件下,对电子垂直入射碰撞电离氦原子的三重微分散射截面进行了理论计算,并把计算结果与实验测量结果进行了比较,系统研究了(e,2e)反应中各种屏蔽效应对氦原子三重微分散射截面的影响,同时对截面中形成各峰的碰撞机理做了详细的探讨.研究结果表明:在入射能较低时,各种屏蔽效应对氦原子的三重微分散射截面幅度以及角分布均存在一定影响,并且形成各峰的碰撞机理直接影响截面的变化规律.     

电子碰撞电离离子三重微分截面的计算

解决了包含四个合流超几何函数的数值积分问题,从而给出了计算电子碰撞电离离子三重微分截面的通用方法,适合于中、高入射能量下的各种几何条件。计算了对称和不对称几何条件下电子碰撞电离He⁺离子的三重微分截面,并与其它理论结果作了比较。     

关于"太阳在银河系中所受引力与到银心距离r的关系"的讨论

讨论了银道面内的引力场强分布和太阳在银河系中所受引力与到银心距离r的关系，指出引力场强g并不是与r的平方成反比，这是由于银河系的大小和形状不能忽略造成的．强调了万有引力定律的适用条件．     

On the predictability of the positions of the convergence zones in the ocean

The disagreement between the experimental and calculated positions of the first convergence zone are known from many publications. The most probable cause for such a disagreement, namely, the incorrect specification of the input data for the calculations, is considered. The lack of simultaneity between the hydrological surveys of the region and the acoustic experiments is emphasized. The experimental data obtained by the author in five ocean regions are presented. These data characterize the diurnal variability of the distance from the source to the nearest boundary of the convergence zone. The relations proposed by different researchers for calculating the sound speed from the temperature, salinity, and hydrostatic pressure are analyzed. It is shown that these relations lead to a substantial difference in the estimated depth dependence of the hydrostatic gradient of the sound speed. The position of the first convergence zone is calculated for the propagation conditions determined by vertical temperature and salinity profiles with the subsequent recalculation of these profiles into sound speed profiles by using eight different formulas known from the literature. It is shown that different formulas lead to different values of the distance to the first zone; this difference is substantially greater than that between the calculations and experiment. The necessity of improving the recalculation relations in view of the experimental data on sound propagation in natural oceanic waveguides, including the data on the actual positions of the convergence zones, is emphasized.     

On the calculation of the bremsstrahlung in the region of the plasma frequency

On the basis of the classical theory of radiation produced in incomplete Coulomb interaction, a formula is derived for the coefficient of the bremsstrahlung of fully ionized plasma. In the region of rectilinear approximation a comparison is made with the results of the quantum formula derived from the Born approximation. Furthermore, the influence of dispersion upon the emission coefficient is taken into account; some relations for the region of dispersion are given.     

Dependence of the Intensity of the Spectral Lines and the Composition of the Sample and the Plasma Parameters of the Unipolar Arc

The investigation was made of the dependence of the intensity of Tl, Ga, Mo, Mg, Mn, Sn, Bi, Ni, Zn, Pt and Au spectral lines and the plasma parameters (temperature T, electron concentration n_e, degree of 6 ionnization α) from concentration of lithium additive.     

Extracting the wavefunction of the LSP at the LHC

We consider associated production of squarks and gluinos with the lightest supersymmetric particle (LSP), or states nearly degenerate in mass with it. Though sub-dominant to pair production of color SU(3)-charged superpartners, these processes are directly sensitive to the wavefunction composition of the lightest neutralinos. Exploiting event-shape variables - including some introduced here for the first time - we are able to identify the composition of the LSP by selecting events involving a single high-pT jet recoiling against missing transverse energy. We illustrate the proposed technique on a set of benchmark cases and propose methods for applying these results in more realistic experimental environments.     

Set the controls for the heart of the Sun

In this paper we describe experiments conducted with high-power lasers that are attempting to replicate, for a very short time and in miniature, conditions found in the Sun. Experiments to date have reached conditions in the outer part of the Sun. To reach the Sun's centre requires compression of material to very much greater than solid density and heating to over ten million degrees. To achieve this, a new class of experiments and a new generation of high-power lasers are required.     

On the Question of the Source of the Apokamp

Technical Physics - The object of this work is the apokamp—a new type of plasma jet, which is formed from a bright offshoot emerging at the bending point of a channel of a high-voltage...