Cd+离子5s2S1/2→5p2P3/2电子碰撞激发截面和退激辐射光子极化度的理论研究

本文采用全相对论扭曲波方法计算了Cd⁺离子5s²S_1/2 → 5p²P_3/2电子碰撞激发总截面、磁能级的激发截面以及退激辐射光子极化度. 详细讨论了电子关联效应对激发截面以及退激辐射光子极化度的影响. 我们发现, 在低能碰撞部分(<10 eV), Core-价关联对电子碰撞激发截面的贡献非常重要, 与不考虑Core-价关联的结果相比, Core-价关联的计算结果使得激发截面降低了1/2到2/3; 在高能碰撞部分(>80 eV), Core-价关联的贡献不是非常明显, 但与不考虑Core-价关联的结果相比, 其激发截面也降低了15%. 然而, 对于退激辐射光子极化度, Core-价关联的贡献非常小, 其影响是可以忽略的.     

原子簇La8-xBaxCuO6的原子磁矩和自旋极化的电子结构研究

利用MS-Xα方法研究了化合物La_2-yBa_yCuO₄的原子磁矩和自旋极化的电子结构.理论计算得到母相氧化物La₂CuO₄的Cu原子磁矩为0.37μ_B，与实验值0.48±0.15μ_B基本一致. 研究结果显示, 由于Ba原子对部分La的替代，使构成化合物的基本原子簇La_8-xBa_xCuO₆的 关键词： 电子结构 自旋极化 磁矩 态密度 超导电性     

Gruhn-Hess两体势修正模型向列相液晶微滴的Monte Carlo模拟

基于Gruhn-Hess两体势修正模型,用Monte Carlo方法模拟向列相液晶微滴.Gruhn-Hess两体势是空间各向异性的,修正模型的势参数依赖于液晶的弹性常数K₁₁、K₂₂、K₃₃及表面弹性常数K₁₃.假设向列相液晶微滴具有自由表面,在低温下计算分子二阶序参数和切向内禀强度在微滴内不同区域的变化,并与Gruhn-Hess两体势模型一作对比分析.结果表明:附加K₁₃项的修正模型在微滴表面产生内禀锚定,其大小决定了内禀易取向方向及内禀锚定强度的大小,且内禀强度的大小与K₃₃/K₁₁值有关;空间不完整的向列相液晶微滴由内层到外层有序度逐渐降低.     

自旋反转同步辐射的高阶量子修正

本文讨论电子的同步辐射使其自旋横向极化的效应, 用两种方法导出光子反冲对自旋反转辐射几率的高阶量子修正. 计算表明这种修正使最终的极化率减小而使弛豫时间增长.     

高次谐波的Guo-Åberg-Crasemann理论及其截断定律

将Guo-Åberg-Crasemann形式散射理论推广到高次谐波产生过程, 获得了高次谐波产生概率公式. 利用这一公式, 计算了不同惰性气体原子的高次谐波谱. 理论分析和数值计算显示高次谐波有新的截断定律q_cħω = (9 -4√2) U_p + (2√2-1) I_p ≈ 3.34 U_p + 1.83 I_p, 其中, U_p 为电子的有质动能, I_p 为原子电离能, ħω 为激光光子能量, q_c 为高次谐波的截断阶数. 这一截断定律与近期Popmintchev等 (Popmintchev et al. 2012 Science 336 1287) 的实验观测符合得很好.     

激光同步辐射光源的辐射条件

激光同步辐射光源是一种新型的X射线光源，它利用高强度激光与相对论电子束发生康普顿散射，从而在电子的运动方向上辐射出X射线．本文在考虑电子的反冲基础上，利用康普顿散射研究了激光同步辐射光源（LSS）辐射光子的精确波长和能量；同时发现，对于背散射情况，只有当种子激光的波长λ1大于电子的物质波波长λm时才能发生LSS辐射；最后给出LSS辐射的极值波长λ2max=h/（m0γv）和极值能量εc2max=βε3.     

合肥储存环谐波超辐射自由电子激光的数值计算

 采用数值模拟的方法，结合合肥同步辐射自由电子激光的实际参数，并考虑了三维空间效应及束流能散度、发射度等影响，计算了电子束的能量调制、密度调制及谐波超辐射等物理过程。     

抛物量子线中强耦合极化子的有效质量

采用改进的线性组合算符法、Lagrange乘子和变分法,在考虑电子与LO声子相互作用情况下,研究了抛物量子线中强耦合极化子的有效质量和光学声子平均数。通过数值计算,讨论了约束强度ω₀和拉格朗日乘子u对极化子的有效质量m^*和光学声子平均数N及极化子振动频率λ的影响。计算结果表明:有效质量m^*和光学声子平均数N及极化子振动频率λ都随着约束强度ω₀和拉格朗日乘子u的增加而增大。     

等离子体中四光子的相干散射

本文应用动力学方法计算了均匀非磁化等离子体的电子二级非线性密度涨落,得到了三波在等离子体中相互作用的三级非线性极化率X⁽³⁾和第四波K₄=K₁-K₂+K₃,ω₄=ω₁-ω₂+ω₃的散射功率,与通常的非相干汤姆逊散射相比,其散射信号要大得多,因此,相干四光子散射可以作为等离子体诊断技术的一个重要方法,本文还指出,文献[4]的结果是本文计算的一个简单情况。 关键词：     

北京正负电子对撞机(BEPC)同步辐射实验厅辐射剂量水平的测定

本文描述了北京正负电子对撞机(BEPC)同步辐射实验厅内辐射的来源和特点,辐射测量方法及其测量结果.通过对东、西两个实验厅的辐射剂量水平随时间和空间变化的分析,得出一个重要的结论:同步辐射实验厅内辐射剂量水平与实验厅相对正负电子束流注入点的位置、屏蔽墙厚度、束流注入的时间和效率有密切关系.     

Polarization of coherent synchrotron radiation from an electron beam rotating in a plasma

After eliminating reflections from the walls of the plasma container, we observed polarization of the coherent synchrotron radiation from a relativistic electron beam rotating in a plasma. Several features of the polarization agree well with calculations based on the single particle synchrotron radiation theory. A particular polarization ratio (Fig. 3) does not, however. We deduce from this direct diffraction of the radiation by the beam electrons. This is strong evidence for beam-particle bunches of size cm. Also, there must be some absorption of the extraordinary wave to account for the observations. We suggest a way to apply these results to measure the pitch angle of the beam.Work supported by Army Research Office.     

等离子体中相对论电子的同步曲率辐射特性研究

根据同步曲率辐射理论推导了在等离子体环境中,不同磁场条件下的相对论性电子的吸收系数和发射系数表达式，计算了电子的发射强度，并且在此基础上研究了同步曲率辐射机制的脉泽效应.研究了两种磁场位型，第一种是强度均匀但弯曲的磁场，第二种是偶极磁场，结果发现了一些偶极磁场下特有的辐射特性.考虑到在天体的环境下电子具有的不同的能谱分布，分别选用了三种典型的能谱分布(幂率分布，高斯分布，热分布)进行了研究，通过计算负吸收和脉泽放大效应在发射强度上的表现后， 发现在某些天体物理环境中，同步曲率辐射在等离子体中的确存在脉泽放大效应.这些研究结果对太阳系中行星外层辐射的研究和宇宙中的射电高亮温度等问题的研究可能提供有益的帮助. 关键词： 同步曲率辐射 负吸收 脉泽效应     

Lienard-Wiechert potentials and synchrotron radiation from a relativistic spinning particle in pseudoclassical theory

For a relativistic spinning particle with an anomalous magnetic moment, Lienard-Wiechert potentials are constructed within the pseudoclassical approach. Some specific cases of the motion of a spinning particle are considered on the basis of general expressions obtained in this study for the Lienard-Wiechert potentials. In particular, the intensity of the synchrotron radiation from a transversely polarized particle moving along a circle at a constant speed is investigated as a function of the particle spin. In the specific case of particles having no anomalous magnetic moment and moving in an external uniform magnetic field, the resulting expressions coincide with familiar formulas from the quantum theory of radiation. The spin dependence of the polarization of synchrotron radiation is investigated.     

超精细结构效应对辐射光谱圆极化特性的影响

在相对论多组态Dirac-Fock方法和密度矩阵理论的基础上,利用发展的全相对论扭曲波程序,系统研究了超精细结构效应对纵向极化电子碰撞激发过程以及退激发辐射光谱圆极化特性的影响.计算得到了类氦Sc~(19+)和~(205)Tl~(79+)离子1s~2 ~1S_0→1s2p ~3P_2超精细结构层次上M_F能级的碰撞强度,考察了辐射衰变过程中发出特征光子的极化特性,并分析了E1-M2量子干涉效应以及电子-电子间相互作用的相对论修正对退激发辐射光子圆极化度的影响.     

Investigation of a method to calculate spontaneous radiation spectra from relativistic electrons in undulators

Undulators are key devices to produce brilliant synchrotron radiation at the synchrotron radiation facilities.In this paper we present a numerical computing method,including the computing program that has been developed to calculate the spontaneous radiation emitted from relativistic electrons in undulators by simulating the electrons' trajectory.The effects of electron beam emittance and energy spread have also been taken into account.Comparing with other computing methods available at present,this method has a few advantages with respect to several aspects.It can adopt any measured or arbitrarily simulated 3D magnetic field and arbitrary electron beam pattern for the calculation and it's able to analyze undulators of any type of magnetic structure.It's expected to predict precisely the practical radiation spectrum.The calculation results of a short period in-vacuum undulator and an EllipticaUy Polarized Undulator (EPU) at Shanghai Synchrotron Radiation Facility (SSRF) are presented as examples.     

合肥800MeV电子储存环同步辐射特性

以石英卤钨灯作为光谱辐照度标准光源，测量了在３００－８００ｎｍ波段的合肥ＭｅＶ电子储存环同步辐射的相对光谱分布；并在４０５ｎｍ波长处测量了辐射源的角分布和偏振特性，在实验误差范围内，测量结果与理论计算值相符，相对光谱分布偏差为１．５％，角分布和偏振特性偏差小于５％。     

高能电子在强激光场中的同步辐射获得超短X射线脉冲

 研究了逆流相对论高能电子与强激光脉冲相互作用的同步辐射过程,当电子具有合适的初速度且传播方向与激光的传播方向相反时,电子在激光脉冲中心作圆周运动。由于电子的运动半径比传统同步辐射环中电子的运动半径小几个数量级,因此电子的辐射能量大大增加。研究发现此过程可以获得阿秒和泽秒X射线脉冲;同时发现随着入射电子初能量的增加和激光能量的增强,获得X射线脉冲脉宽越来越短,强度越来越大。这使得激光同步辐射可以成为一种强大的短波长短脉宽的辐射光源。     

Synchrotron resonance maser

Attention is drawn to an obscure formula derived from relativistic quantum electrodynamics in the mid-'60s by Sokolov and Ternov for induced absorption and emission from highly relativistic electrons in a static uniform magnetic field. From their results, we develop handy formulae and graphs to help in preliminary designs for radiation sources to operate at high synchrotron harmonics. Approximate design parameters are given for 100 kW oscillators operating at wavelengths below 3mm, employing magnetic fields of less than 12 kG. It is shown that the Sokolov-Ternov formula can also be deduced from classical relativistic plasma wave theory, but for a numerical factor in one term. This term is shown to describe a gain mechanism which has apparently received scant notice in the gyrotron literature.     

Polarization control of microwave emission from high powerrectangular cross-section gyrotron devices

Results are summarized of experiments on a gyrotron utilizing a rectangular-cross-section (RCS) cavity region. The major issue under investigation is polarization control of microwave emission as a function of magnetic field. The electron beam driver is the Michigan Electron Long Beam Accelerator (MELBA) at parameters: V=0.8 MV, I_diode=1-10 kA, I_tube=0.1=0.5 kA, and t_e-beam=0.4-1.0 μs. The annular e-beam is spun up into an axis-encircling beam by passing it through a magnetic cusp prior to entering the RCS interaction cavity. Experimental results show a high degree of polarization in either of two orthogonal modes as a function of cavity fields. The RCS gyrotron produced peak powers of 14 MW in one polarization (TE₁₀) and 6 MW in the cross-polarized mode (TE ₀₁). Electronic efficiencies for this device reached as high as 8% with transverse efficiency of 16%. Experimental results on the beam alpha (α=V_⊥/V_∥) diagnostics, where alpha is the ratio of the e-beam's transverse velocity to its parallel velocity, agree well with the single electron trajectory code. MAGIC code results are in qualitative agreement with microwave measurements. Microwave emission shifts from the dominant fundamental mode polarization (TE₁₀□ ), to the next higher order mode polarization (TE₀₁□) as the solenoid magnetic field is raised from 1.4-1.9 kGauss. Frequency measurements using heterodyne mixers support mode identification as well as MAGIC code simulations     

Sm_2Co_(17)型永磁合金的辐照效应研究

Sm_2Co_(17)型永磁合金大量使用在上海同步辐射光源储存环的永磁型波荡器上,在受到长期辐照后会发生磁性能损失的现象,进而影响同步辐射光的品质.为了探索其潜在的微观机理,本文首先对Sm_2Co_(17)型永磁合金所处混合辐射场的粒子及相关物理量进行了计算分析,确定引发磁性能损失的主要粒子是中子.然后采用Ar离子模拟中子辐照损伤的方法对其进行辐照,采用透射电镜对其辐照前后的微观形貌及微观结构进行了研究探讨,采用振动样品磁强计对永磁合金辐照前后的饱和磁化强度进行了分析对比,并讨论了微观结构演化与宏观磁性能变化的联系.结果表明,Ar离子辐照后Sm_2Co_(17)型永磁合金饱和磁化强度的不可逆损失与微观结构变化有直接的关系,其2:17相从单晶结构转变为非晶结构是造成其磁性能损失可能的微观机制.