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.     

19F+27Al深部非弹性碰撞产物的角分布

完成了19F+27Al深部非弹性碰撞产物的角分布测量.初步分析了反应产B,C,N,O,F,Ne,Na,Mg和Al的实验室系角分布,展现出深部非弹性反应机制的特点,显示了反应系统随时间的演化过程. Angular distributions of fragments produced in the deep inelastic collision of~(19)F+~(27)Al have been measured for incident energy of 114 MeV at θ_(lab)= 9~(o), 24~(o), 40~(o), 55~(o), 70~(o) and 85~(o). Angular distributions of dissipative products B, C, N, O, F, Ne, Na, Mg and Al are analyzed to provide an evolution process of the intermediate dinuclear system formed in the reaction.     

27Al+27Al重离子耗散碰撞中能量自关联函数的分析

测量了²⁷Al+²⁷Al耗散反应产物的激发函数,束流²⁷Al⁸⁺的入射能量从114MeV到127MeV变化,能量步长为200keV.探测角度覆盖了实验室系10°—57°的连续区域.用不同的理论模型分析了耗散产物的能量自关联函数.结果表明,反应所形成的中间双核系统的阻尼相干转动造成了激发函数中不可平滑的涨落结构,相干转动的阻尼来自量子混沌运动.     

16O+152Sm、184W准弹和弹性散射的位垒分布

利用¹⁶O束流轰击稳定形变靶¹⁵²Sm和¹⁸⁴W,在背角测量准弹散射和弹性散射激发函数,分别定出准弹和弹性位垒分布D^qel(E)和D^el(E).将结果与从已有的熔合激发函数、自旋分布及其相邻同位素¹⁵⁴Sm和¹⁸⁴W实验得出的位垒分布进行比较,得到相互自洽的结果,同时也用ECIS79程序作了耦合道理论计算.实验表明,靶的变形效应导致位垒分布是非对称的.     

16O+115In反应中余核的激发函数

在能量为51—97MeV的¹⁶O离子轰击¹¹⁵In的反应中,采用核化学技术测定了21个反应产物的激发函数,实验结果与复合核统计蒸发模型的Alice程序以及描述复合核统计蜕变过程的Monte-Carlo模拟计算值进行了比较.     

19F+208Pb近垒及垒下准弹反应

用电离室△E-E望远镜测量了¹⁹F+²⁰⁸Pb体系在88、91.93、96.98、102MeV6个能量点的准弹反应角分布,用ECIS程序拟合弹性散射角分布,得到该体系的光学势参数,观察到明显的“阈异常”现象,对转移反应角分布作了分析,得到了产物为C、N、O的转移反应的激发函数,此外,导出了3个主要转移反应道²⁰⁸Pb(¹⁹F、¹⁸O、¹⁵N、¹⁴C)的转移几率和最趋近距离的关系,得到斜率因子κ. 在单核子转移的情况下,κ值与半经典计算基本符合;而对于两核子以上转移的情况,k值小于理论值,存在着“斜率反常”的现象. 同时发现k值明显与能量相关,这无法用半经典理论解释.     

关于12C+16O反应的三体出射道的研究

我们用两个带电粒子符合方法研究了能量为56MeV的¹⁶O轰击¹²C的三体反应出射道,分别得到了两个不同的三体出射道:α₁+α₂+²⁰Ne和p+α+²³Na的反应Q值谱,两道之间的比为8:1,同时得到了α₁+α₂两维符合事件的投影谱,结果显示α+²⁴Mg是α₁+α₂+²⁰Ne出射道的主要中间过程.     

16O+24Mg熔合激发函数和深光学势

基于重离子碰撞中势共振的考虑,在光学模型的框架下,使用深光学势研究了¹⁶O+²⁴Mg全熔合激发函数中所呈现的粗共振结构和弹性散射角分布后角振荡上升的现象,并与核分子轨道模型的计算结果作了比较,对产生粗共振结构的原因进行了讨论.     

强子衰变过程J/ψ→ωπ+π－中的多道耦合

讨论了强子衰变过程J/ψ→ωπ⁺π^－包含的三个不同中间过程J/ψ→ωf₂(1270),f₂→π⁺π^－和J/ψ→b₁^±(1235)π⁺,b₁^±→ωπ^±的耦合问题.这种耦合效应的考虑对于精确测定共振态f₂和b₁^±的参数以及这些反应道的螺旋度振幅比是十分重要的.     

17F和18Ne与质子的弹性散射角分布

采用逆运动学方法对放射性核束¹⁷F和¹⁸Ne与质子进行弹性散射实验,得到了实验测量微分截面.用较准确描述放射性核素性质的CH89参数化的光学势为初始光学势,用扭曲波玻恩近似的理论计算程序DWUCK4和自动参数搜索程序ABOD对实验数据进行光学势参数理论拟合,得到了与实验数据相符合的光学势参数.将得到的光学势参数进行分析,得到了17F和18Ne实势相互作用均方根半径分别为3.239fm和3.317fm.     

27Al+27Al耗散反应中间双核系统的核温度

从²⁷Al+²⁷Al耗散反应产物的激发函数中提取能量相干宽度Г,再求出双核系统的核温度T,并用相干转动的概念进行以合与解释.     

Study of Proton Resonances in ~(22)Mg by Resonant Elastic Scattering of ~(21)Na+p and Its Astrophysical Implication in ~(18)Ne(α,p)~(21)Na Reaction Rate

Proton resonant states in ~(22)Mg have been investigated by the resonant elastic scattering of ~(21)Na+p.The ~(21)Na beam with a mean energy of 4.00 MeV/u was separated by the CNS radioactive ion beam separator(CRIB) and bombarded a thick(CH_2)_n target.The energy spectra of recoiled protons were measured at scattering angles of θ_(cm)～172° and 146°,respectively.A new state at 7.06 MeV has been observed clearly and another new one at 7.28 MeV is tentatively identified due to its low statistics.The proton resonant parameters were deduced from an R-matrix analysis of the differential cross section data.The astrophysical resonant reaction rate for the ~(18)Ne(α,p) ~(21)Na reaction has been estimated,and it is about five times larger than that assumed before.     

27Al+27Al耗散反应中激发函数的测量与统计性质分析

通过测量能量从114—120MeV、能量步长为200keV的重离子耗散反应²⁷Al+²⁷Al从θ(cm)=50°—90°的角分布和激发函数,在对所有宏观出射道积分的基础上,分析了重离子耗散反应中激发函数涨落的物理性质.     

30MeV/u 40Ar+58,64Ni和115In反应中中等质量碎片的角分布

在5°—140°范围内测量了30MeV/u ⁴⁰Ar束流轰击不同靶核(⁵⁸Ni、⁶⁴Ni、¹¹⁵In)后出射的中等质量碎片(IMF,Z=3—19)的角分布.用指数分布函数dσ/dΩ=N·exp(–θ/α)对出射碎片角分布分角区做了拟合.对3个反应系统分别提取出与相互作用时间有关的衰减因子α和与发射源强度有关的物理量N,讨论了α与N在不同角区与反应系统和出射IMF电荷数的关系.考察了角分布与同位旋自由度和反应系统对称性的关系.     

Langevin study of neutron emission in the reactions ^16O＋^181Ta and ^19F＋^178Hf^＊

The pre-scission neutrons measured in the reactions 16O 181Ta and 19F 178Hf are studied via a Langevin equation coupled with a statistical decay model. We find that because of the mass asymmetry of different entrance channels, the spin distributions of compound nuclei would be different, consequently, the measured neutrons in these two reactions would also different. This means that the entrance channel will affect the particle emission in the fission process of hot nuclei.     

Study of proton resonances in ~(18)Ne via resonant elastic scattering of ~(17)F+p and its astrophysical implication

The proton resonant properties in 18Ne, which determine the reaction rate of the key stellar 14O(α,p)17F reaction, have been studied by using a technique of proton resonant elastic scattering of 17F+p. A 4.22 MeV/nucleon 17F radioactive ion (RI) beam was produced via a projectile-fragmentation reaction, and separated by a Radioactive Ion Beam Line in Lanzhou (RIBLL). By bombarding a thick (CH2)n target, the energy spectra of the recoiled protons were measured by two ΔE-E silicon telescopes at the center-of-...     

Theoretical study of energy transfer in Rb(7S) + Rb(5S) and Rb(5D) + Rb(5S) collisions

We present results of theoretical studies of the non-resonant excitation transfer in Rb(7S) + Rb(5S) and Rb(5D) + Rb(5S) collisions at thermal collision energies. Rb₂ adiabatic molecular terms correlating with the 5S+7S, 5S+5D and 5P+5P states of separated atoms were calculated for internuclear distances R > 20 a.u. using asymptotic approximation. Mechanisms of collisional population and quenching of the 5D state were treated on the basis of the computed molecular terms, and the respective cross-sections were calculated. Theoretical cross-sections are in good agreement with the experimental values at thermal collision energies ( K). Received 13 November 1998 and Received in final form 22 November 1999