28.7MeV/u的 14，16，18 O+7，9Be反应中的同位素分布研究

用同位旋相关的Boltzmann-Langevin方程研究了在入射能量为28.7MeV/u下,不同弹核^14O,^16O和^18O轰击不同靶核^7Be和^9Be的反应,计算了生成碎片的产生截面,发现用丰中子（缺中子）炮弹或丰中子（缺中子）靶进行反应,所得到的产物均有丰中子（缺中子）的碎片出现。同位素分布宽度和峰位与入射体系密切相关,产生碎片的电荷数越接近入射弹核的电荷数,则同位素分布的宽度越大,峰位偏离β稳定线值越远,其同位旋效应越明显。。     

28.7MeV/u的14,16,18O+7,9Be反应中的同位素分布研究

用同位旋相关的Boltzmann-Langevin方程研究了在入射能量为28.7MeV/u下,不同弹核¹⁴O,¹⁶O和¹⁸O轰击不同靶核⁷Be和⁹Be的反应,计算了生成碎片的产生截面,发现用丰中子(缺中子)炮弹或丰中子(缺中子)靶进行反应,所得到的产物均有丰中子(缺中子)的碎片出现.同位素分布宽度和峰位与入射体系密切相关,产生碎片的电荷数越接近入射弹核的电荷数,则同位素分布的宽度越大,峰位偏离β稳定线值越远,其同位旋效应越明显.     

同位旋依赖的动量相关作用对同位旋分馏的影响随入射道条件的演化

由量子分子动力学通常应用的动量相关作用公式出发，引入同位旋自由度后得到了在量子分子动力学中可用于数值计算的同位旋依赖的动量相关作用.并用这个公式较系统地研究了在它的作用下，同位旋分馏比的入射道效应和它们的动力学机理.结果表明所有入射道能量、碰撞参数以及所有的丰中子碰撞系统中子-质子比和质量条件下动量相关作用的同位旋依赖性对同位旋分馏过程产生了重要的同位旋效应，然而它没有明显改变同位旋分馏比对于对称势灵敏的依赖性，即在考虑动量相关作用的同位旋自由度后同位旋分馏比仍是提取同位旋非对称核物质状态方程的灵敏探针. 关键词： 同位旋分馏比 动量相关作用 重离子碰撞     

静态形变及动力学形变对GR的影响

在半经典近似框架下,利用Scaling变换,讨论了静态形变及动力学形变对同位旋标量巨四极共振(GQR)及同位旋矢量巨偶极共振(GDR)的影响.静态形变导致双峰分裂,计算结果和实验事实相一致,动力学形变则解决了不同K(K为角动量投影)间的所有简并.     

轻系统多重碎裂的同位旋效应

利用同位旋相关的量子分子动力学模型,对⁴⁰Ca+⁴⁰Ca和⁴⁰Ar+⁴⁰Ar系统在不同入射能量时,同位旋效应对多重碎裂的影响进行了讨论.低能区的多重碎裂由于多种同位旋相关的因素相互抵消,因此多重碎裂的同位旋效应不明显.随着能量的增加,同位旋相关的截面造成多重碎裂的明显差别.     

同位旋依赖的动量相关作用对同位旋分馏过程的影响和机理

在同位旋相关的量子分子动力学理论的基础上，引入同位旋自由度，将同位旋无关的动量相 关作用改造成为在同位旋相关的量子分子动力学中可用的同位旋依赖的动量相关作用．研究 了它在中能重离子碰撞中的作用和机理．研究结果表明，考虑同位旋依赖的动量相关作用后 ，对同位旋分馏过程有很大的影响，使同位旋分馏强度降低．降低的幅度随入射能量的增加 而迅速增加.特别是动量相关作用的同位旋效应与对称势的同位旋效应具有大体相同数量级 ．但两者具有完全不同的动力学机理．所以同位旋依赖的动量相关作用的研究对于定量的研 究同位旋非对称核物质状态方程是重要的. 关键词： 同位旋依赖的动量相关作用 同位旋分馏强度 重离子碰撞     

弹核碎裂反应中同位旋效应的系统研究

用统计擦碎模型对中能区不同弹靶体系在弹核碎裂反应中的同位旋效应和同位旋标度率现象进行了系统研究. 发现归一的同位素分布峰位差和约化的同位旋标度率参数随(Z_proj－Z)/Z_proj or (N_proj－N)/N_proj呈指数下降, 与反应系统大小无关. 指出约化的同位旋标度率参数可以用来研究中能重离子碰撞中反应系统的激发程度和非对称核物质的状态方程.     

中能重离子碰撞中同位旋相关核子–核子碰撞截面的灵敏探针

基于重质量弹核(放射性核或稳定核)打轻质量靶核的逆运动学效应,即反应产物主要集中在小角度的优点,利用同位旋相关的量子分子动力学模型,探寻了对于中能重离子碰撞过程中同位旋效应灵敏的物理观测量.计算表明,在入射能量约大于80MeV/u能区,中等质量碎片多重性随发射带电粒子总数之间的演化是提取介质中同位旋相关的核子–核子碰撞截面的灵敏物理量.     

同位旋非对称核物质性质与扩展的BHF方法(Ⅳ)单粒子势与有效质量

在扩展的同位旋相关的Brueckner-Hartree-Fock理论框架内,计算了同位旋非对称核物质中质子与中子的单粒子势和有效质量及其同位旋效应,并详细研究和讨论了基态关联对单粒子势和有效质量及其同位旋依赖的影响.     

同位旋和动量依赖的相互作用在重离子碰撞中的同位旋效应

引入同位旋自由度将同位旋无关的动量相关作用改造成同位旋和动量依赖的相互作用. 利用同位旋依赖的量子分子动力学理论研究了同位旋和动量依赖的相互作用对中能重离子碰撞中动量耗散和同位旋分馏的作用. 计算结果表明动量相关作用具有重要的同位旋效应，尽管它没有明显的改变原子核阻止(动量耗散)对于两体碰撞截面和同位旋分馏强度对于对称势的灵敏依赖性，但它对于以上两种灵敏性产生了明显的减弱作用. 故动量相关作用中同位旋效应研究对于定量的研究和确定同位旋非对称核物质状态方程是重要的.     

(γ, p) cross sections and isospin splitting of the giant dipole resonance in N = 50 nuclei

The differential (e, e'p) cross sections of ⁸⁸Sr, ⁸⁹Y, ⁹⁰Zr and ⁹²Mo have been measured at θ = 90°. The results are used to obtain the (γ, p) cross sections by correcting with the angular distribution data. The (γ, p) cross sections are compared with the (γ, n) cross sections. A resonance corresponding to the T_< GDR is found and another resonance is separated by fitting a Lorentz line with a width equal to that of the (γ, n) GDR. The ratios σ(γ, p)/σ(γ, n) and σ(γ, p₀)/σ(γ, p) show differences between the two resonances. The two GDR resonances are studied from the isospin splitting point of view. The sum rule and splitting energy of the (γ, p) GDR agree well with theory. However, when the sum of the (γ, p) and (γ, n) experimental data is taken, the results are too large to be explained by the T_> GDR.     

A study of the giant dipole resonance of vibrational nuclei in the 103 ≦ A ≦ 133 mass region

This paper presents a set of experimental data concerning the giant dipole resonance of nuclei (GDR) in the 103 ≦ A ≦ 133 mass region. The cross sections σ(γ,n) and σ(γ, 2n) were obtained in the energy region 8–30 MeV by means of a monochromatic photon beam produced by annihilation in flight of positons. This paper attempts also to give an interpretation of the experimental behaviour of the GDR for vibrational nuclei in the 103 ≦ A ≦ 133 mass region in terms of the simple dynamic collective model. In particular it is shown that the width of the GDR increases as β increases and as E₂₊ decreases and that the theoretically predicted spreading of the dipole strength is confirmed by our experimental results. As to the characteristic behaviour of the GDR above its peak value at E₀, we come to the conclusion that the actual state of the art in (γ, xn) research does not allow one to make an unambiguous choice between isospin splitting or electric quadrupole absorption. Finally the numerical evaluations of the different sum rules are given and some empirical results concerning the average energy of the GDR as a function of A are also presented.     

Evolution of the giant dipole resonance properties with excitation energy

The studies of the evolution of the hot Giant Dipole Resonance (GDR) properties as a function of excitation energy are reviewed. The discussion will mainly focus on the A ∼ 100-120 mass region where a large amount of data concerning the width and the strength evolution with excitation energy are available. Models proposed to interpret the main features and trends of the experimental results will be presented and compared to the available data in order to extract a coherent scenario on the limits of the development of the collective motion in nuclei at high excitation energy. Experimental results on the GDR built in hot nuclei in the mass region A ∼ 60-70 will be also shown, allowing to investigate the mass dependence of the main GDR features. The comparison between limiting excitation energies for the collective motion and critical excitation energies extracted from caloric curve studies will suggest a possible link between the disappearance of collective motion and the liquid-gas phase transition.     

Alpha-Decay Energy and Lifetime of New Superheavy Nuclei with Restored Wigner’s <Emphasis Type="Italic">SU</Emphasis>(4)-Symmetry

The alpha-decay energies and lifetimes for several alpha-chains of superheavy nuclei were calculated on the basis of Wigner’s mass formula. In this calculation, the contribution of spin–orbit interaction to the nuclear mass is disregarded, in which caseWigner’s spin–isospin symmetry is restored. The calculated alpha-decay energies agree with experimental data better than the results of other modern theoretical approaches. The alpha-decay energies are predicted for several isotopes of charge number Z = 120.     

Photoproton cross section of 34S

Measurements of the ³⁴S(γ, p) and ³⁴S(γ, np) cross sections are reported. The ³⁴S(γ, p) cross section shows two regions of strength, at 17 and 22 MeV, consistent with that seen in the ³⁴S(γ, n) cross section.A particle-hole calculation is made for the dipole absorption cross section in ³⁴S. The photoproton and photoneutron cross sections calculated on the assumption of statistical decay of GDR states under the constraints of isospin selection rules, agree well with those seen experimentally.     

Effects of the entrance channel mass asymmetry in fusion reactions

The symmetric and asymmetric fusion reaction systems forming the same compound nuclei 26Al,30Si,38Ar and 170Hf are investigated with the frame of improved isospin dependent quantum molecular dynamics model.The entrance channel mass asymmetry dependence of compound nucleus formation is found by analyzing the shell correction energies,the Coulomb barriers and the fusion cross sections.The calculated fusion cross sections agree quantitatively with the experimental data.The results indicate that compound nucleus formation is favorable for the systems with larger mass asymmetry because of the smaller Coulomb contribution to the fusion barrier.     

Isospin and symmetry energy study in nuclear EOS

This paper summarizes the isoscaling and isospin related studies in asymmetry nuclear reactions by different dynamic and statistical models. Isospin dependent quantum molecular dynamics model (IQMD) and lattice gas model (LGM) are used to study the isoscaling properties and isoscaling parameters dependence on incident energies, impact parameters, temperature and other parameters. In the LGM model, the signal of phase transition has been found in free neutron (proton) chemical potential difference Δµ_n or Δµ_p as a function of temperature, or in free neutron and proton chemical potential difference Δµ_n−Δµ_p. Density dependence of symmetry energy coefficient C _sym(ρ/ρ ₀) is also studied in the frame of LGM, with the potential parameters which can reproduce the nuclear ground state property, soft density dependence of symmetry energy is deduced from the simulation results. Giant dipole resonance (GDR) induced by isospin asymmetry in entrance channel is also studied via IQMD model, and the dynamic dipole resonance shows isospin sensitivity on the isospin asymmetry of entrance channel and symmetry energy of the nuclear equation of state (EOS). GDR can also be regarded as a possible isospin sensitive signature.

     

Isospin effect in photoproton reaction on heavy nuclei

The cross sections and energy distributions of photoprotons measured mainly with (e, e'p) reactions on heavy nuclei are summarized. Isospin effects in this reaction are discussed for the IAR and isospin splitting of GDR. These effects for the proton energy distributions are theoretically calculated with the simple shell model and the results show qualitative agreement with the experimental results. Detailed experimental results which can not be explained by the present theory are also discussed.     

A measurement of the 50Ti(γ, n) and 50Ti(γ, n0) cross sections

Measurements of the ⁵⁰Ti(γ, n) and ⁵⁰Ti(γ, n₀) cross sections have been made in the energy range of the giant dipole resonance (GDR). Assuming the GDR is split into two isospin components, approximated as Lorentzians, a calculation based on statistical decay of the GDR states is consistent with the experimental results.     

Giant resonances in exotic nuclear systems: What we expect and what we know

The characteristic features of γ-rays resulting from the decay of the Giant Dipole Resonance in very deformed, hot systems and in systems with a large isospin are discussed. For both cases there are recent theoretical predictions but very few if any data. With respect to hot, deformed systems it is argued that the discrepancy which exists between the measured and calculated asymmetry of the GDR γ-rays emitted in the fusion-fission process of hot actinide nuclei, might well be due to γ-emission during the saddle-to-scission stage of the fission process, that is from very deformed hot nuclear systems. The prospect of studying experimentally the behavior of Giant Resonances in systems with large isospin (=large neutron excess) is also discussed. Experiments on the GDR are feasible and will give information on the deformation of the emitting system.