Shell effect and capture cross sections in the synthesis of superheavy nuclei

The shell effect is included in the improved isospin dependent quantum molecular dynamics model in which the shell correction energy of the system is calculated by using the deformed two-center shell model.A switch function is introduced to connect the shell correction energy of the projectile and the target with that of the compound nucleus during the dynamical fusion process.It is found that the calculated capture cross sections reproduce the experimental data quantitatively at the energy near the Coulomb...     

神光II升级装置波前传输计算模型与验证

基于衍射理论和神光II升级激光装置的光路结构及光学元件波前像差,建立了激光装置光束波前像差传输计算模型,用以获取在实验中难以取得,但对激光系统设计和安全运行非常重要的变形镜校正面型、放大器动态波前像差、空间滤波器波前像差和焦斑形态等过程数据。利用该模型对激光装置常规运行时的静态传输、变形镜加压静态传输和大能量发射3种状态下的波前传输进行理论分析,计算结果与实验测量相一致,并在此基础上对变形镜未加压大能量发射波前传输进行计算。计算模型可用于指导相关器件的设计,优化激光运行控制模式,有利于提高激光装置输出波前质量。     

Energy partition in nuclear fission

A scission point model (two spheroid model TSM) including semi-empirical, temperature-dependent shell correction energies for deformed fragments at scission is presented. It has been used to describe the mass-asymmetry-dependent partition of the total energy release on both fragments from spontaneous and induced fission. Characteristic trends of experimental fragment energy and neutron multiplicity data as function of incidence energy in the Th — Cf region of fissioning nuclei are well reproduced. Based on model applications, information on the energy dissipated during the descent from second saddle of fission barrier to scission point have been deduced.     

入射粒子与靶相互作用中电子能损的高阶修正

研究了在较高能入射离子（He离子、 12_C离子）与靶相互作用中电子能量损失的物理机制, 分别探讨了电子能量损失中的相对论修正、 壳修正、 密度修正以及Barkas效应和Bloch效应等修正的贡献, 发现壳修正、 Barkas效应修正和Bloch效应修正在能量小于100 MeV时是重要的, 而相对论修正和密度修正是在能量大于100 MeV时起作用。 加入各种修正项之后, 电子阻止本领的计算结果和实验值（ICRU49）符合更好。 The mechanisms of electronic energy loss in the process of incident particles interaction with Si and Al₂O₃ at proper energies are investigated. The contribution to the electronic energy loss from high order corrections, such as the relativistic correction, the shell correction, the density correction, the Barkas effect correction and the Bloch effect correction are discussed respectively. It is found that the shell correction, the Barkas effect correction and the Bloch effect correction are important at low energies, the relativistic correction and the density correction are important at high energies. The calculated results with these higher order corrections are in good agreement with the experiment data (ICRU49).     

Some Properties of Si,Ge, and α-Sn Using Pseudopotential Theory

The pseudopotential theory beyond second order with our well establishedsingle parametric model potential is employed to compute total crystalenergy, static bulk modulus, energy band gap at the point X on theJones-zone face and pressure-volume relation (equation of state underpressure) of Si, Ge and α-Sn using Nagy's static local field correction function. The results are compared with those obtained using few other local field correction functions. The present results of total energy are in good agreement with the experimental data. Bulk modulus calculated byNagy's screening function is perfectly matching with the experimentalresults for Ge and α-Sn. Some deviation is found in the value of energy band gap.     

Electronic Stopping Power for 0.05--10MeV Protons in a Group of Organic Materials

Electronic stopping powers for 0. 05-10 MeV protons in a group of organic materials are systematically calculated. The calculations are based on Ashley＇s dielectric model, and an evaluation approach of optical energy loss function is incorporated into Ashley＇s model because no experimental optical data are available for most of the organic materials under consideration. The Barkas-effect correction and Bloch correction are included. The proton stopping powers for the considered organic materials except for mylar in the energy range from 0.05 to 10 MeV are presented for the first time. The results may be useful for studies of various radiation effects in these materials and for space research.     

A relativistic quark-diquark model for the nucleon

We developed a constituent quark-diquark model for the nucleon and its resonances using a harmonic oscillator potential for the interaction. The effects due to relativistic kinetic energy correction are studied. Finally, charge form factor of the model is calculated and compared with experimental data.      

Binding energy for inhomogeneous nuclear matter

For a spatial finite nuclear density distribution a binding energy formula is developed. A modified Thomas-Fermi method which deduces the mixed density by taking into account an anisotropic local momentum space occupation is used. This method presents the binding energy as a functional of the proton and neutron density distributions. It was possible within this framework to derive in a consistent way the energy correction terms due to density inhomogeneities. The structure of these energy correction terms is shown and an estimate is given for the adjustable parameters of this model to fit the experimental nuclear masses.     

Analysis of fission excitation functions and the determination of shell effects at the saddle point

A method is proposed to deduce the shell correction energy corresponding to the fission transition state shape of nuclei in the mass region around 200, from an analysis of the first chance fission values of the ratio of fission to neutron widths, (Γ _f /Γ _n )₁. The method is applied to the typical case of the fissioning nucleus²¹²Po, formed by alpha bombardment of²⁰⁸Pb. For the calculation of the neutron width, the level densities of the daughter nucleus after neutron emission were obtained from a numerical calculation starting from shell model single particle energy level scheme. It is shown that with the use of standard Fermi gas expression for the level densities of the fission transition state nucleus in the calculation of the fission width, an apparent energy dependence of the fission barrier height is required to fit the experimental data. This energy dependence, which arises from the excitation energy dependence of shell effects on level densities, can be used to deduce the shell correction energy at the fission transition state point. It is found that in the case of²¹²Po, the energy of the actual transition state point is higher than the energy of the liquid drop model (LDM) saddle point by (3 ± 1) MeV, implying significant positive shell correction energy at the fission transition state. Further, the liquid drop model value of level density parametera is found to be a few per cent smaller for the saddle point shape as compared to its spherical shape.     

质子与裂变核238U反应的理论计算

利用球型光学模型、耦合道理论、核内级联、激子模型、蒸发模型、带宽度涨落修正的Hauser-Feshbach模型,Bohr-Wheeler裂变理论,对入射能量从阈能到200 MeV的p+²³⁸U各种反应进行了计算,计算结果和实验符合较好.     

利用改进的Glauber模型对非奇异核核反应总截面数据的拟合

在对反应总截面的理论计算中,现有的理论计算值与实验数据在高能区可以很好的符合，但在中能区理论值低于实验值约10％—20％.通过对计算核反应总截面的Glauber模型加入有限程修正，并对输入的核物质密度分布采用双参数的费米密度分布形式.计算结果表明，理论计算值对于没有奇异结构的核在低中能区和高能区，都与实验数据很好符合.     

On the quantum corrections to the virial coefficients of the equation of state of a fluid

The first quantum correction to the virial coefficients of the equation of state of a fluid is derived in the presence of a weak three-body potential ?(i, j, k). Results for the third and fourth virial coefficients are given. Representing the potential energy of interaction of a pair and a triplet, by the Lennard-Jones (12-6) model and the triple dipole dispersion potential model of Axilrod and Teller, the first quantum correction to the third virial coefficient is calculated for many values of T*. The theoretical result is compared with the experimental data of helium.     

Center-of-mass correction and rotational correction in covariant density functional theory

Center-of-mass(c.m.) correction and rotational correction in even-even Ge isotopes are systematically investigated within the triaxially deformed relativistic Hartree-Bogoliubov model using the PC-PK1 force. The shell effect and deformation effect on the microscopic c.m. correction and rotational correction are discussed, and the importance of both corrections on reproducing the binding energy is demonstrated.     

On oblate-prolate transition in the ground state rotational band of light mercury isotopes

The transition from an oblate to a prolate shape in the ground state band of even mass Hg isotopes and in the ground states of the chain of odd mass Hg isotopes are studied. The shape is found by minimizing the deformation energy which is calculated by means of Strutinsky's shell correction method. The rotational energy corresponds to the axialsymmetric rotator. The moment of inertia is calculated with the help of the cranking model. Pairing and hexadecupole deformation are included. The results are in good agreement with the available experimental data.     

面向浑浊水体叶绿素a浓度遥感反演的光谱基线校正

根据浑浊水体中悬浮物的光学性质,提出使用线性基线校正方法来削弱水体光谱中的悬浮泥沙贡献。线性基线定义为450和750 nm的反射率值连线,基线校正为光谱反射率减去基线。2010年3月和2011年4月太湖梅梁湾水体的实测数据验证结果表明,光谱线性基线校正可以较好的提高叶绿素a浓度的反演精度,改进反演模型的诊断性。3月数据建立的波段比值反演模型中,校正前模型RMSE为4.11 mg·m-3,基线校正后模型RMSE为3.58 mg·m-3,同时,基线校正后模型残差的方差齐性和正态分布均有明显的改善。4月模型有类似结果,数据校正后的模型具有更小的误差。在没有水华发生的浑浊水体中,线性基线校正可以作为提高水体叶绿素a浓度反演精度的光谱数据处理方法。     

基于凸优化的激光诱导击穿光谱基线校正方法

在激光诱导击穿光谱定量分析中,基线是LIBS光谱信号的重要组成部分,由于受到实验参数设置及实验环境变化等影响,导致等离子体的发射谱线呈现不同程度的基线漂移现象,因此基线校正是光谱分析的重要环节。现有算法如多项式拟合通常需要设定关键参数,不具备自适应性。由于激光诱导产生的等离子体光谱信号的特征峰具有明显的独立性和稀疏性,以及基线具有低通特性,因此在凸优化约束框架下,提出了非参数化基线校正模型。同时,利用高效率的迭代算法来保证结果的收敛性。首先对23个高合金钢样本的光谱信号进行基线校正,然后以合金钢样本中的铬(Cr)元素为分析对象,并选取11条分析线进行定量分析。分别采用PLS和SVM定量模型进行训练和预测,并且与传统方法相比较,证明了所提出方法可以提高定量分析精度。     

Models for high-energy inclusive processes and screening in deuterium

The screening correction to the high energy (p_lab > 10 GeV/c) elastic hadron-deuteron scattering amplitude is discussed. It is found that the correction cannot completely be calculated using as input only the data for cross sections of inclusive reactions on free nucleons. Nevertheless measurements of high energy screening corrections provide sensitive tests for models of inclusive processes. In particular elastic screening does not dominate over the inelastic screening if, as indicated by recent fits, the triple pomeron coupling does not vanish for three mass-zero pomerons. If this is the case, the theory of high energy elastic scattering on heavier nuclei would have to be reconsidered. The discussion is illustrated by a numerical calculation for elastic πd scattering in the 10GeV–2000 GeV energy range.     

Single particle models in the shell correction approach

We investigate the dependence of the shell correction energy on the parameters as they occur in the Nilsson model and the single particle model with a Woods-Saxon potential. We give criteria, how these parameters should be chosen in order that the shell correction energies become fairly model-independent. The different models yield now a value of about ?20 MeV for²⁰⁸Pb, substantially larger than in previous work. Its relation to the remainder of the mass formula fit is discussed. We find that shell energies have an extremum. The minimum occurs close to the conventional parameter values (except the potential diffuseness of the protons) and close to the minimum of the total binding energy. The minimum in shell energy corresponds to a maximum bunching of single particle states. The gross properties of these extremal shells agree considerably better with the experimental spectra (for both the neutrons and the protons) than those of conventional model parameters.     

噪声修正的混响反演海底反射系数幅值参数

利用一种噪声修正方法解决低混噪比条件下混响数据反演海底反射系数幅值参数偏差的问题。将全波动混响理论中的混响非相干平均强度,叠加海洋环境噪声平均强度,获得包含噪声的混响平均强度理论,分析背景噪声平均强度对反演海底反射系数幅值参数的影响。数值仿真表明,背景噪声平均强度的叠加使得混响平均强度衰减趋势减缓,导致海底反射系数幅值参数反演结果偏小,混响噪声比越低,影响越明显。提出一种噪声平均强度相减的修正方法,对混响噪声比为[0,6] dB的混响平均强度数据进行修正,利用修正后的混响数据反演得到偏差较小的海底反射系数幅值参数。对比浅海混响实验数据衰减至不同混噪比时反演所得海底反射系数幅值参数,以及经噪声修正后的反演结果,验证了本文提出方法的可行性。      

连续谱X射线在ICT中的能谱硬化修正模型

X射线ICT中,由于连续谱X射线源在穿过物质时,能量较低的射线优先被吸收,也即较高能量的X射线的衰减系数比较低能量的X射线的衰减系数小,射线随透射厚度增大,变得更易穿透,也就是发生了能谱硬化现象。如不加修正,必引起赝像。文中对能谱硬化现象进行实验和理论上的分析,探讨了在均匀物质中, X射线的衰减系数与透射厚度的关系, 提出新的能谱硬化修正方法和严谨精确的能谱硬化修正模型。