96MeV 16O+64Ni反应机制的研究

在96MeV ¹⁶O离子轰击下,测量了¹⁶O+⁶⁴Ni反应出射碎片(α直至O元素)的Wilczynski图和角分布,并提出DIC截面和反应时间等物理量;讨论了反应的DIC特征;看到了出射碎片α和Li主要来源于复合核蒸发的迹象.     

16O+115In反应的全熔合与非完全熔合

在92和71MeV ¹⁶O离子与¹¹⁵In的相互作用中,用核化学技术测量了20个反应余核的角分布和微分射程分布.分析了这些余核的生成特征,指出随着碰撞参数的增加,反应机制从全熔合经过质量和动量转移逐渐减小的非完全熔合向直接反应连续演变.与¹⁶O+⁶⁵Cu反应相比,¹⁶O+¹¹⁵In反应中非完全熔合的贡献显著增加.     

124MeV下16O+16O弹性散射的折叠模型

¹⁶O+¹⁶O弹性散射在124MeV能量下最新的全角区的实验角分布,可以被建立在¹⁶O的α结构基础上的折叠模型很好地再现.     

16O+94Zr和16O+116Sn的弹性散射角分布测量

用北京Q3D磁谱仪及其重离子焦面探测器系统测量了两个体系的14个弹性散射角分布,即¹⁶O+⁹⁴Zr体系在52,57,59,62,72,82和92MeV 7个能量点及¹⁶O+¹¹⁶Sn体系在57,59,62,67,72,82和92MeV 7个能量点的弹性散射角分布.用耦合道理论的ECIS计算程序拟合数据,初步观察到了“阈反常”现象.     

质子散射对16O原子核α结构的检验

利用质子散射作为手段对¹⁶O的α粒子结构模型进行了检验.基于4α结构模型,对跨度整个中能区的质子与¹⁶O核的弹性角分布进行了无自由参数的计算.理论与实验基本符合.     

基于上海激光电子γ源的天体核合成关键反应12C(α,γ)16O的反应率研究

正在研制的上海激光电子γ源是MeV量级的高品质γ光束线站，基于该装置可以开展一系列核天体物理实验, 从而更准确的确定各天体核合成反应的反应率. 本文研究了天体核合成中的关键反应¹²C(α,γ)¹⁶O的反应率. 根据多组实验和理论截面数据分别计算了反应率, 并给出了这些反应率计算结果的平均值和统计误差. 根据该结果拟合了理论反应率的解析形式, 确定了新的参数. 进而给出俘获反应¹²C(α,γ)¹⁶O在He燃烧环境下的反应率和误差, 并讨论了电子屏蔽效应对天体反应率的修正.     

97MeV 16O轰击51V靶出射α粒子的测量与理论分析

用不同种类的粒子望远镜测量了97MeV ¹⁶O+⁵¹V反应中出射的α粒子.得到了单举α粒子能谱、角分布、E-θ平面内的d²σ/dEdΩ截面等高图及速度平面内的d²σ/PCdEdΩ截面等高图.区分了复合核蒸发的α粒子与直接机制发射的α粒子.用激子模型对预平衡发射的α粒子贡献进行估计,得到的预平衡发射和复合核蒸发分别在α粒子总产额中所占的比份.     

11Li的三体模型

考虑了¹¹Li的奇异性质和泡利原理后,引入了一个新的n-⁹Li等效相互作用.在(n+n+⁹Li)模型的基础上完成了变分计算.给出了¹¹Li作为三体系统时的形状、一体密度和相应的形状因子.对¹¹Li的核物质均方半径也作了计算.结果与实验是相符的.     

垒下16O+232Th裂变碎片角关联模拟

使用Monte-Carlo模拟计算了垒下¹⁶O+²³²Th系统转移裂变和复合核裂变碎片角分布及角关联.转移过程、熔合过程和裂变过程分别用半经典模型、耦合道模型及鞍点过渡态统计模型进行模拟.考虑了各物理量分布产生的运动学效应及裂前中子发射和裂后碎片粒子蒸发对碎片角分布及角关联的影响.模拟结果和实验测量的分布相一致.使用折叠角技术借助Monte-Carlo模拟区分转移裂变和复合核裂变是可能的.考虑了转移裂变和裂前中子发射的影响,复合核裂变碎片角分布各向异性异常仍然存在.     

超核13C17O低激发态的研究

本文从唯象的Λ-α相互作用位和¹²C、¹⁶O的独立α粒子模型波函数出发,采用折迭位方法,求出了Λ-¹²C、Λ-¹⁶O等效相互作用位的解析表示,在此基础上计算了超核¹³C、¹⁷O的低激发态能量和自旋轨道耦合效应所引起的¹³C第一激发态的能级劈裂,并对Λ-¹²C、Λ-¹⁶O等效相互作用位和¹³C、¹⁷O的有关问题进行了分析和讨论.     

Spectroscopy of A = 16 from 13C(6Li,t)16O

The ¹³C(⁶Li, t)¹⁶O reaction has been studied at 34 MeV. Selective population of narrow states is observed up to 21 MeV excitation in ¹⁶O. This reaction populates strongly both unnatural-and natural-parity states that have little or no ¹²C + α₀ width. The measured angular distributions are compared with Hauser-Feshbach and finite-range DWBA calculations. Reasonable agreement with the DWBA calculations is found for most of the states strongly populated. The widths of the narrow states populated in the 16–20 MeV excitation region are presented. Comparison of the present data with that from medium-energy inelastic scattering and other multiparticle transfer reactions is made.     

The reaction 16O(6Li,d)20Ne at 75 MeV

The angular distributions of the reaction ¹⁶O(⁶Li, d)²⁰Ne at 75 MeV for transitions to members of the ground state band are well fitted by exact finite-range DWBA calculations assuming a direct α-cluster transfer and yield spectroscopic factors in good agreement with shell-model predictions.     

Comparative study of the selectivity displayed by (6Li,d) and (16O, 12C) reactions

Four-particle-transfer processes induced by the (⁶Li, d) and (¹⁶O, ¹²C) reactions to strongly excited 0⁺ states are compared. Although the selectivity displayed by these reactions is similar, the corresponding relative cross sections are rather different. These results emerge naturally from a simple microscopic model.     

Alpha-particle strengths from the 16O(6Li,d)20Ne reaction

The ¹⁶O(⁶Li, d)²⁰Ne reaction has been studied at bombarding energies of 20, 32 and 38 MeV. The α-particle spectroscopic strengths have been extracted for levels up to 12.15 MeV in excitation. Nondirect processes appear to contribute significantly to all levels at 20 MeV and to high spin levels (6⁺ and 8⁺) at 32 MeV. Strengths extracted for members of the ground state band assuming (sd)⁴ transfer are unequal at both 32 and 38 MeV, in marked contrast to theoretical predictions. To explain this, particle-hole correlations in ¹⁶O(g.s.), inelastic channel coupling in the reaction and perhaps other effects as well, have to be considered. Strengths extracted for members of excited bands and α-decay reduced widths compare poorly with each other and with simple SU(3) predictions.     

A study of the 18O(6Li,d)22Ne reaction at 32 MeV

Results from a study of the ¹⁸O(⁶Li, d)²²Ne reaction at a ⁶Li energy of 32 MeV are reported. The L-dependence of the shapes of the measured angular distributions provide a check on recent J^π assignments for some of the high-lying levels in ²²Ne. A finite range distorted wave analysis assuming a direct cluster transfer has been used to extract from the data α-particle spectroscopic strengths for most of the natural parity levels populated below 8 MeV of excitation. These strengths are compared with theoretical predictions for those few states for which a definite correspondence can be made between the calculated and experimental levels of ²²Ne. For transitions to the members of the ground-state band, the observed strengths disagree with the predictions. This disagreement has also been observed in the ¹⁶O(⁶Li, d) reaction and its cause is not understood. It is in marked contrast with the good agreement found for (⁶Li, d) reactions on targets of mass 20 ≦ A ≦ 24.     

Microscopic study of heavy-particle transfer reactions: The (16O, α) reactions on 16O and 28Si

The transfer reactions ²⁸Si(¹⁶O, α)⁴⁰Ca and ¹⁶O(¹⁶O, α)²⁸Si have been studied within the framework of the two-channel generator coordinate method. The geometry of the reactions has been discussed in terms of the cross-channel overlap kernels of the generating functions. A clear connection between maxima in the reaction rate and entrance channel resonances has been established. A two-step reaction mechanism involving quasimolecular resonances of inelastic ¹⁶O-¹⁶O channels is discussed as a possible explanation for narrow structures seen in the ¹⁶O(¹⁶O, α)²⁸Si reaction cross section.     

Elastic scattering of tritons by 16O

Angular distributions and excitation functions have been measured for the ¹⁶O(t, t) reaction from 1.4 to 3.7 MeV triton energy using a differentially pumped gas target. The observed resonances have been analysed with the Humblet-Rosenfeld theory. It appears that the 13–15 MeV excitation range of the compound system of ¹⁹F is dominated by several levels of large triton partial width. Levels populated in the three-particle transfer reaction (⁷Li, α) on ¹⁶O are compared with the resonances.     

Unnatural parity levels populated in the 16O(6Li,d)20Ne reaction

The ¹⁶O(⁶Li, d)²⁰Ne reaction to the 2^?, 4.97 MeV, 3^?, 5.63 MeV, and 4^?, 7.01 MeV members of the K^π = 2^? band has been studied. Angular distributions were measured at 32 MeV from 7.5° to 145° (lab). Excitation functions were measured at 15° (lab) and 145° (lab) from 31 to 33 MeV and 31.75 to 32.5 MeV, respectively. Results of multi-step and compound nuclear calculations are compared to the data. At this incident energy, both mechanisms appear to contribute to the population of the unnatural parity levels.     

Sequential and simultaneous transfer in the reactions 18O(p,t)16O, 48Ca(t,p)50Ca and 90Zr(t,p)92Zr

The effects of sequential transfer of a pair of neutrons in the reactions ¹⁸O(p, t)¹⁶O, ⁴⁸Ca(t, p)⁵⁰Ca and ⁹⁰Zr(t, p)⁹²Zr are found to be sizeable. Channel spin-orbit distortion is an important feature of the calculations of the ¹⁸O and the ⁴⁸Ca reactions.     

Coupled-channels study of projectile and target excitation in the scattering of 6Li from 12C and 16O

Coupled-channels calculations are presented tor elastic and inelastic ⁶Li + ¹²C scattering at E_c.m. = 16 MeV and 20 MeV, and for ⁶Li + ¹⁶O at 18.7 MeV. Excitation of states within ⁶Li, ¹²C and ¹⁶O are treated with rotational, rotation-vibration and vibrational models only. The 3⁺⁶Li and 2⁺¹²C states are strongly coupled to the elastic scattering and reduce the strengths of both the real and imaginary potentials. The 3^?16O state reduces only the strength of the imaginary potential. All other states are weakly coupled and have little effect on each other or the potential. The data are reasonably well described, with there being some preference for the 3^? state in ¹²C to be K = 0. Excitation of the 0₂⁺ state in ¹²C requires a combination of β-vibration and monopole breathing-mode form factors. The deformation lengths found are in poor agreement with those deduced from electron or proton scattering.