氘核削裂反应的扭曲波近似处理

关于C¹²(d,p)C¹³(基态)削裂反应的角分布和极化,应用扭曲波方法进行了以下几种情况的讨论:(i)Born近似;(ii)质子受无l-s耦合项的光学势扭曲;(iii)氘核受黑体扭曲;(iv)氘核受黑体扭曲、质子受无l-s耦合项的光学势扭曲;(v)氘核受黑体扭曲、质子受有l-s耦合项光学势扭曲;(vi)氘核受硬球扭曲;(vii)氘核受硬球扭曲、质子受无l-s耦合项光学势扭曲,由分析的结果表明,不论是对角分布或者是对于极化而言,扭曲波方法都是一种比较好的近似。     

中子与116,118,120,122,124Sn反应非弹性散射的理论计算和分析

应用现有的中子与原子核Sn及其同位素反应的总截面,去弹性散射截面,弹性散射截面和弹性散射角分布的实验数据,获得一组普适的中子与Sn及其同位素反应的光学模型势参数.利用这组光学模型势参数,扭曲波玻恩近似理论,核反应Hauser-Feshbach理论和预平衡反应的激子模型,计算和分析了中子与^{116,118,120,122,124}Sn反应分离能级的非弹性散射截面和角分布.理论计算与实验数据进行了分析比较.     

电子碰撞原子(e,2e)反应的复极化势

研究包括连续通道等非处理通道的复极化势对(e,2e)碰撞过程三重微分截面的影响,即将耦合通道光学势方法得到的复极化势附加到畸变波玻恩近似方法的畸变势中,在靶态的HF近似下,计算了Ar原子和Ne原子在非共面对称几何条件下(e,2e)反应的三重微分截面.对于较高的入射能量,在实验的误差范围内,计算结果与电子动量谱的实验数据符合较好,复极化势的影响很小;对于较低的入射能量,复极化势的作用明显增大. 关键词： 复极化势 (e;2e)反应 三重微分截面 电子动量谱     

关于氘核削裂反应的动量近似理论

本文从普遍微扰公式出发,推导出氘核削裂反应的动量近似表示式。并在氘核内动量分布因子是δ函数的近似下,对于入射氘核能量为11.9Mev的C¹²(d,p)C¹³(基态)反应进行了数值计算。结果表明:动量近似理论是有可能解释中能削裂反应的。     

α转移反应的激发函数

本文研究了α转移反应~(28)Si(~(16)O,~(12)C)~(32)S的激发函数,构造了核轨道线性组合分子态的耦合道理论,计算结果与实验较好符合,与扭曲波玻恩近似理论结果比较有很大的改进.     

利用直接核反应研究轻丰中子核的奇特结构

直接核反应(包括弹性散射、非弹性散射、转移反应等)是研究丰中子核奇特结构的常用实验手段之一。以6,8He、11Li、11,12Be、14,15B、15,16C等N=8附近核的结构研究为例，综述了如何利用这几种反应从实验上研究丰中子核的奇特结构。利用6,8He，11Be等晕核在质子和氘靶上的弹性散射数据，拟合得到了这些反应体系的有效相互作用(光学势)。利用16C在质子和氘靶上的非弹性散射数据，抽取了16C 的形变参数，结果表明16C的形变不可忽略。利用单核子转移反应，定量研究了8He, 11,12Be等丰中子核基态及低占据态中的p-，s-，以及d-波成分的强度。结果表明:8He基态中的4个价中子，除了可以构成正常的 (0p_3/2)4 组态外，还有一定的几率构成($ 0 p_{3/2} $)2(0p_1/2)2组态；12Be的基态以d波闯入为主，而其临近的11Be的基态以s波闯入为主。     

中子与90,91,92,94Zr反应的理论计算和分析

根据中子与天然Zr及其同位素反应的总截面,去弹截面和弹性散射角分布的实验数据,得到一组普适的光学模型势参数;应用得到的光学模型势参数,光学模型,Hauser-Feshbach理论,预平衡反应的激子模型和扭曲波玻恩近似理论,系统计算和分析了中子与^90,91,92,94Zr反应的非弹散射角分布和双微分截面,理论结果与实验很好的一致.     

中子引起氘核破裂反应的实验研究

对25 MeV中子引起氘核破裂反应的中子-中子准自由散射和17.36 MeV中子引起氘核破裂反应的中子-中子末态相互作用进行了细致的研究。首先,以小于5%的不确定度,精确测量了25MeV中子-中子准自由散射出射的中子三重微分截面。实验数据用基于现实核子-核子势(CD-Bonn,Argonne!18,Nijm I和II)的理论计算配合Monte-Carlo模拟进行了分析。实验结果比基于CD-Bonn势的理论预言高(16.0±4.6)%,进一步证实了目前的理论在中子-中子准自由散射方面还无法准确描述实验数据。其次,通过运动学非完全测量,精确测量了17.36 MeV中子引起氘核破裂反应在0°角附近出射的质子能谱,用基于现实核子-核子势(CD-Bonn、Bonn-B和Nijm I)的理论计算以及Monte-Carlo模拟分析了所测得的质子能谱,确定了中子-中子散射长度ann=(-16.8±0.6)fm。     

中子与63,65Cu反应的理论计算

根据中子与天然Cu及其同位素反应的总截面, 去弹截面和弹性散射角分布的实验数据, 得到中子的光学模型势参数; 应用得到的光学模型势参数, 光学模型, 统一的Hauser-Feshbach和激子模型理论, 以及扭曲波玻恩近似理论, 系统计算和分析了中子与^63,65Cu反应的非弹散射角分布和双微分截面, 理论结果与实验很好的一致.     

氘核的微观光学势

本文采用双粒子格林函数方法,在忽略双粒子间直接相互作用时,得到双粒子格林函数的一级、二级质量算符为各个单粒子质量算符的和.采用核物质近似和Skyrme有效相互作用得到的核子微观光学势,用折叠公式计算了氘核的微观光学势.用所得到的学光势计算了氘核的弹性散射角分布和反应截面,与现有的一些实验数据进行了比较,发现反应截面能较好地符合实验,而弹性散射角分布符合实验较差.为了改进理论,又研究了双粒子间极化图对氘核微观光学势虚部的贡献.     

Intermediate energy deuteron-nucleus diffraction interaction

On the basis of diffraction scattering theory, elastic and inelastic deuteron-nucleus scattering, deuteron dissociation and stripping reactions have been studied at intermediate deuteron energies. The finite value of the nuclear surface diffuseness, Coulomb deuteron-nucleus interaction and internal deuteron structure have been considered in the analysis of differential and integrated deuteron-nucleus cross sections. The theoretically calculated deuteron cross sections are in good agreement with the experimental data.     

On the reversibility of stripping reactions

The basis for the equivalence of prior and post forms of the T-matrix in both the Born and the distorted wave Born approximations is here studied in a one-dimensional model that facilitates clarification of some of the underlying mechanism. One sees how important it is that changes in the wave functions bring it about that averages of different perturbing potentials over different regions can still be equal. The post form commonly employed for a (d, p) reaction makes it seem at first sight that the potential stripping the deuteron apart is the potential that holds it together. The prior form DWBA has as a perturbation the intuitively appealing interaction responsible for the classical break-up of the deuteron and contributing to the “surface reaction” nature of stripping.     

Alpha-spectroscopic factors in the DWBA

The analysis of α-transfer experiments in the frame of the Distorted Wave Born Approximation (DWBA) yields experimental values for the spectroscopic factors. We show that a consistent reaction theory leads to a theoretical formula for these spectroscopic factors which is different from the one conventionally used. The main point is that we take into account properly the effects of the antisymmetrization.     

Evidence for pair correlation effects in heavy ion reactions

The study of the ¹²C(¹⁴N,¹⁴N)¹²C reaction was performed at 28 and 35 MeV beam energies. The results were analyzed in the frame of the EFR-DWBA (Exact-Finite-Range Distorted Wave Born Approximation) assuming the simultaneous and sequential transfer of a np pair. The angular distributions, fairly reproduced in the first case, confirm the validity of the generalized BCS (Bardeen–Cooper–Schrieffer) theory to explain this behaviour. Moreover, this process could be regarded as a possible Nuclear Josephson Effect.     

Competition between neutron-proton rescattering and deuteron break-up in (d,np) reactions

Existing final-state interaction (FSI) theories predict observable rescattering effects in low-energy nuclear reactions with three or more particles in the final state. Obvious yields which could be attributed to this effect have only been reported in (d, np) reactions. However,n-p rescattering might be confused with the neutron-proton FSI following deuteron break-up since both contribute strongest at low relative neutron-proton energies. We have re-examined the (d, np) reactions on¹²C and⁴⁰Ca in a kinematically complete experiment making special effort to try to distinguish between rescattering and then-p FSI. Data have been taken within and outside the reaction plane at different bombarding energies. Attempts to simultaneously fit the detailed shapes of the proton spectra and the azimuthal angularn-p correlations with theoretical predictions in a consistent way were unsuccessful forboth reaction mechanisms. Improvements in the fits at particular energy and angle combinations were always at the expense of the agreement at other angles or energies. Therefore it must be concluded from our analysis that on the basis of calculations available at present the contributions fromn-p rescattering and deuteron break-up cannot be distinguished in a conclusive manner in the (d, np) experiments performed to date.     

Competition between neutron-proton rescattering and deuteron break-up in (d, np) reactions

Existing final-state interaction (FSI) theories predict observable rescattering effects in low-energy nuclear reactions with three or more particles in the final state. Obvious yields which could be attributed to this effect have only been reported in (d, np) reactions. However,n-p rescattering might be confused with the neutron-proton FSI following deuteron break-up since both contribute strongest at low relative neutron-proton energies. We have re-examined the (d, np) reactions on¹²C and⁴⁰Ca in a kinematically complete experiment making special effort to try to distinguish between rescattering and then-p FSI. Data have been taken within and outside the reaction plane at different bombarding energies. Attempts to simultaneously fit the detailed shapes of the proton spectra and the azimuthal angularn-p correlations with theoretical predictions in a consistent way were unsuccessful forboth reaction mechanisms. Improvements in the fits at particular energy and angle combinations were always at the expense of the agreement at other angles or energies. Therefore it must be concluded from our analysis that on the basis of calculations available at present the contributions fromn-p rescattering and deuteron break-up cannot be distinguished in a conclusive manner in the (d, np) experiments performed to date.     

Two-step process in proton inelastic scattering

Proton inelastic scattering exciting single-neutron states is calculated in the framework of the three-body model. The transition amplitude is approximately given by a sum of the one-step Born term and the pickup-stripping terms including the continuum p-n system propagation as well as the deuteron propagation in the intermediate state. The continuum contribution is not negligible at low energy and becomes as important as the terms at higher energies.     

间接测量天体物理S因子的特洛伊木马方法

天体环境下的核反应速率是各种关于天体核合成理论模型所需的输入量,对于了解天体核合成过程,以及宇宙的演化很重要。但是在天体温度下,核反应是在很低的能量上发生的。由于库仑位垒的作用,反应截面非常低,直接测量很难进行。通过测量合适的三体反应截面,特洛伊木马方法提供了一种提取感兴趣的低能两体反应截面的方法;而且,采用一系列近似可得到便于计算的理论公式。本文介绍特洛伊木马方法的原理及其在天体核反应中的应用。