核介质中核子–核子散射截面的BHF微观计算

在Brueckner-Hartree-Fock(BHF)框架下,计算了核介质中核子-核子(N-N)散射总截面.计算中,N-N相互作用势采用Paris势的可分离表示,单粒子谱采用连续选择.计算结果表明,质子-质子散射及质子-中子散射的总截面随核密度的增加而强烈地减小,特别是对低能散射.对结果作了简单的讨论,并与已有的一些计算结果进行了比较.     

在非相对论能量下介质中的核子－核子碰撞截面

在非相对论能量下，采用Ｓｋｙｒｍｅ有效相互作用，计算了在核介质中的核子－核子（Ｎ－Ｎ）碰撞截面，研究了它与能量及密度的依赖关系，以及不同Ｓｋｙｒｍｅ参数对所计算截面的影响．发现在低密度时，介质中的核子－核子碰撞截面大于经Ｐａｕｌｉ修正后的自由核子一核子碰撞截面．而当高密度时，总会在高于某一能量以后，介质中的Ｎ－Ｎ碰撞截面大于经Ｐａｕｌｉ修正后的自由Ｎ－Ｎ碰撞截面．     

核内核子－核子非弹散射截面（Ⅰ）

在与平均场、核内核子－核子弹性散射截面以及输运方程相统一的理论框架内推导了核内核子－核子非弹散射截面的解析表达式．其数值结果能很好地重现自由非弹截面的实验值，所计算的有效非弹截面与Ｄｉｒａｃ－Ｂｒｕｅｃｋｎｅｒ的计算结果相一致．     

核子相对论微观光学势、薛定谔等效势和平均自由程对核密度及温度的依赖关系

在Ｗａｌｅｃｋａ模型的基础上，应用热动力学理论和ＤｉｒａｃＢｒｕｃｋｎｅｒＨａｒｔｒｅｅＦｏｃｋ方法，研究了有限温度不同密度下核子相对论微观光学势及其相应的薛定谔等效势和平均自由程计算结果表明，核子薛定谔等效势和平均自由程对核密度的依赖相当敏感，当核密度增大时对核密度的依赖变得更为敏感     

中能重离子碰撞中同位旋相关核子-核子碰撞截面和同位旋相关平均场的探针

在最近几年我们通过使用同位旋相关的量子分子动力学模型（IQMD）系统的研究了同位旋相关的平均场和介质中核子－核子（N－N）碰撞截面对中能重离子碰撞（HIC）中碎裂和耗散的同位旋效应。我们发现原子核阻R和Qzz，中等质量碎片多重性Nimf和质子（中子）发射数Np(Nn）敏感的依赖于介质中N－N碰撞截面的同位旋效应，而弱的依赖于同位旋相关的平均场（对称势），这些物理量作为提取相对高能范围缺中子系统的同位旋相关介质中N－N碰撞截面的探针。我们也可以通过相对低能区到150MeV/u的前平衡核子发射中质比来提取关于对称势的知识和讨论它的同位旋依赖性。     

中能强子—核物理的现状与问题

中能强子与核的散射研究发现，400MeV以上似乎普遍存在着截面理论的现象，例如，质子－核（PA）散射、π介子－核（πA）散射、k介子－核（kA）散射的微分截面传统理论值比实验结果约代20％，引入相对论动力学可使PA散射理论结果大为改善，然而，在核子层次上的各种修正对介子－核散射的理论结果改善甚小，人们正在从更深入的非核子自由度寻找原因。     

用相对论VUU研究平均场和核—核子截面对高能和中能集体流的影响

用基于Ｗａｌｅｃｋａ的ＱＨＤ－Ｉ模型的相对论Ｖｌａｓｏｖ－Ｕｅｈｌｉｎｇ－Ｕｈｌｅｎｂｅｃｋ（ＲＶＵＵ）方程，分析了高能和中能重离子碰撞中的集体流，研究了用集体流探测核物质状态方程和核内核子－核子截面的可行性．     

核子-核子碰撞截面的参数化公式

核子-核子碰撞截面(σ_NN)是描述原子核反应模型中的重要物理量。 核子-核子碰撞截面包括质子-质子碰撞截面（σ_pp）、中子-中子碰撞截面（σ_NN）和中子 质子碰撞截面（σ_np）, 它们随着核子能量与核物质密度的改变而变化。人们在目前研究中提出了多种核子-核子碰撞截面关于能量和核物质密度的参数化公式,通过计算12C+12C的完全反应截面,比较了不同入射能量下使用各种核子-核子碰撞截面参数化公式对12C完全反应截面的影响。 The nucleus-nucleus cross sections(σ_NN) include the proton-proton cross section, neutron-neutron cross section, and neutron-proton cross section. σ_NN change with the variations of the incident energies and the densities. Some parameterizations of σ_NNas a function of incident energy and density have been proposed in the theoretical and experimental study of nuclear reactions. Through the calculation of reaction cross sections of 12C+12C at different energies, the effect of different σ_NN parameterizations in the reaction cross sections of 12 are studied.      

重离子反应中核子前平衡发射的同位旋效应

考虑了同位旋相关的对称能、库仑能及核子—核子碰撞截面，对反应４０Ａｒ＋４０Ａｒ（Ｅ＝２５ＭｅＶ／ｕ，ｂ＝０）进行了量子分子动力学模拟，讨论了同位旋效应对核子发射的影响．观察到前平衡发射的中子和质子的比率大于反应系统的中质比，发现对称能有利于中子的发射而阻碍质子的发射，而同位旋相关的核子—核子碰撞截面对中子和质子的发射都有利，但似乎更有利于质子的发射。     

基于色散光学模型的40Ca核子散射数据计算

对钙同位素核数据的研究具有重要的理论价值和应用前景,其中⁴⁰Ca作为天然钙最主要的同位素,是一种重要的材料核素.本文采用色散光学模型对球形核⁴⁰Ca的核子弹性散射数据进行计算.通过考虑色散光学模型势中实部势的非定域性以及虚部势的壳间隙结构,实现了对⁴⁰Ca相关核子散射数据的良好描述,其中包括中子总截面、核子弹性散射角分布以及分析本领.此外,本文计算了色散光学模型势的实部体积分,其随能量的变化图像在费米能附近出现了明显的色散峰结构.     

Cross sections for the n+d breakup reaction

The n+d breakup cross section has been measured between 8 and 22 MeV by integrating the energy distributions of breakup protons and recoil deuterons observed in a deuterated scintillator. The results obtained deviate from the trend suggested by recent measurements of the cross section for proton-induced breakup and favour predictions based on a local N-N potential having a hard core in the singlet state.     

The reaction mechanism of heavy ion scattering at intermediate energies

The contribution to the real and imaginary nucleus-nucleus (N-N) optical potential from nucleon-nucleon scattering in the medium is calculated in a local density approximation from a two Fermi sphere nuclear matter picture for the N-N collision. This reaction mechanism is shown to be dominant for ¹²C + ¹²C scattering at all considered energies (160 MeV < E_lab < 2250 MeV) giving a weakly energy dependent reaction cross section of about 900 mb. Inclusion of the collective 2⁺, 3^? excitations in a coupled channel calculations gives good agreement for both the measured elastic and inelastic 2⁺ cross section at E_lab = 1016 MeV. This fully microscopic parameter free calculation indicates that the energy dependence of the reaction cross section for this system is mostly due to the decrease of the collective contribution with increasing energy contrary to current theoretical models.     

Description of nucleon-nucleus scattering in the Dirac-Brueckner method

Elastic scattering of protons from nuclei is studied based on the Dirac-Brueckner approach. Effective N-N interactions in the nuclear medium are obtained by solving the relativistic Brueckner-Bethe-Goldstone equation in infinite nuclear matter. Relativistic optical potentials for p-⁴⁰Ca scattering at 200 MeV are calculated in the improved local density approximation. It is found that medium effects other than Pauli blocking reduce the strengths of scalar and vector potentials very much. Differential cross section and spin observables are calculated and compared with experimental data.     

Proton-neutron final-state interaction in the reaction 2H(p,pp)n at 6.4, 10.0, 15.9, 19.85 and 25.8 MeV

This paper presents and analyzes the results of measurements of the proton-neutron final-state interaction (FSI) at 6.4, 10.0, 15.9, 19.85 and 25.8 MeV. At each energy nine angular combinations were measured and for each experiment the cross section was measured along the whole kinematic curve. The data are compared with the predictions of S-wave rank-one and rank-two separable potential models. The potentials used in one of the models reproduce the experimental S-wave N-N phase shifts. Fairly large differences between experiment and theory are found in the FSI regions and in the other regions of the kinematic curves. These disagreements cannot be attributed to off-shell effects. The inclusion of the tensor force and the P-wave N-N interaction in the calculations reduces the disagreements considerably at the higher energies. However, systematic differences of 10% to 20% remain.     

Pion bremsstrahlung and critical phenomena in relativistic nuclear collisions

We investigate the dependence of pion bremsstrahlung on the deceleration of the nuclei in relativistic heavy ion collisions. The vicinity of an abnormal phase in nuclear matter can lead - owing to critical N-N scattering - to faster deceleration or decreasing transparency of the nuclei. This would result in a threshold enhancement of the pion bremsstrahlung cross section, which in turn can be used to search for abnormal nuclear states experimentally.     

Structure en bande du noyau 22Na: Le premier niveau Jπ = 6+

We investigate the two-body photodisintegration of ³He and its inverse, radiative p-d capture using bound-state functions corresponding to the N-N interaction being given by the Reid soft-core potential. For the two-body photodisintegration of ³He Coulomb effects and the final-state interactions between the proton and deuteron are not included. At low energy the shape of the angular distribution agrees well with experiment, but the 90° cross section exhibits an anomalous peak at 15 MeV due to electric dipole transitions connecting the deuteron and ³He D-states. The low-energy cross section is 25–40 % too small. The intermediate-energy angular distribution peaks too near the forward direction, and, contrary to experiment, has a minimum at 100°. At higher energy the 90° cross section in the center-of-momentum frame is at least an order of magnitude too small, but does display the correct energy dependence. This energy dependence is related to the properties of the bound-state wave functions and it is plausible that it will persist in an improved treatment (e.g. one which includes exchange currents) which properly accounts for the magnitude of the cross section. Contributions from the ³He S-states are negligible for photon energies between 100 and 150 MeV, but are dominant outside this energy region.     

A “4π-type” study of the reaction p(d,pp)n at Ed = 26.5 MeV

Experimental data on the three-nucleon reaction p(d, pp)n at E_d = 26.5 MeV obtained with the multidetector system BOL, covering most of the phase space, are presented. The data are compared with Faddeev calculations using a local S-wave potential for the nucleon-nucleon interaction. The calculated cross sections, which are in general not sensitive to the precise choice of the nucleon-nucleon potential, agree well with the data over the major part of phase space. We have, though, discovered a region in phase space with a strong discrepancy. In the same region, around a neutron c.m. angle of 140°, the calculations are sensitive to the N-N potential. Theoretical and experimental angular distributions in the p-n recoil c.m. subsystem for proton- neutron energies below 0.5 MeV agree in absolute magnitude, both being isotropic. For larger relative energies, a discrepancy develops, part of which might be related to missing higher par- tial wave components in the N-N interaction, rather than to Coulomb or S-wave scattering effects. The total breakup cross section has been deduced from the data as 169 ± 36 mb.     

动量相关作用对同位旋相关平均场的重要性

利用同位旋相关的量子分子动力学,通过原子核阻止研究了中能重离子碰撞中动量相关作用对于同位旋相关的平均场(对称势)的重要性.计算结果表明动量相关作用同时加强了原子核阻止对于对称势和核子–核子碰撞截面同位旋效应的灵敏性.但相对而言核子–核子碰撞截面对于原子核阻止的作用远大于对称势对于它的作用,等价于动量相关作用提高了原子核阻止对于核子–核子碰撞截面同位旋效应的灵敏性,而减弱了原子核阻止对于对称势的灵敏性.这样就把原子核阻止作为提取同位旋相关的核子–核子碰撞截面的一个探针.     

实验室动能4BeV左右的核子—核子散射

本文给出了带区近似下N-N散射振辐虚部的表示式。利用π-N低能散射的实验数据,计算了实验室动能为4BeV时带区4μ²2内谱函数对N-N散射总截面的贡献。对质子-质子散射得到和实验比较符合的结果,但是在3—4BeV.之间,中子-质子散射的总截面比质子-质子散射的总截面大得多。可以认为,这个结果表示较远的谱函数也很重要。 关键词：     

中子晕核引起核反应中的同位旋效应

利用同位旋相关的量子分子动力学(IQMD)对中子晕核，⁸He和¹⁰He引起核反应中重要的同位旋效应和松散的中子晕结构影响的平均特征进行了研究.因为IQMD中的互作用势和介质中核子-核子碰撞截面灵敏地依赖于碰撞系统的密度分布.而扩展的中子晕密度分布包含了中子晕核的同位旋效应和松散的中子晕结构的平均特征，从而将这些信息通过动力学碰撞带入到反应机理中. 为了清楚地鉴别中子晕核带入反应机理重要的同位旋效应和松散中子晕结构的影响，通过比较中子晕核和相等质量稳定弹核在相同入射道条件下，所得物理观测量之间的差别加以确定.计算结果确实发现具有初始晕核信息的中子扩展密度分布将重要的同位旋效应和松散中子晕结构带入到各种物理观测量中.例如与相等质量稳定相比，中子晕核的晕特征引起了原子核阻止的降低；并明显地增加了核子发射中子-质子比和同位旋分馏比. 关键词： 中子晕核 原子核阻止 核子发射中子-质子比 同位旋分馏比