35MeV／u~(36)Ar+~(112,124)Sn反应中中等质量碎片关联函数的入射道依赖

测量了35MeV／u36Ar+112,124Sn反应中小角关联出射的中等质量碎片(IMF)约化速度关联函数．结果表明36Ar+124Sn反应系统中的约化速度关联函数在小约化速度处的反关联程度比36Ar+112Sn反应系统中的强,表现出明显的入射道依赖性．考察出射粒子对的单核子总动量时,发现这种差异主要来自于高动量粒子对的贡献．用三体弹道理论模型MENEKA分别计算了两个系统的IMF发射时标,在36Ar+112Sn反应系统中约为150fm／c,而在36Ar+124Sn反应系统中,约为120fm／c．同位旋相关的量子分子动力学计算表明,36Ar+124Sn系统中IMF的发射时间谱比36Ar+112Sn系统略有前移,相应地,其中心密度从最高点随时间的下降亦比36Ar+112Sn系统略快．

30MeV/u~(40)Ar+~(112,124)Sn反应中态布居核温度的同位旋效应

用 13单元望远镜探测器阵列测量了 30MeV u40 Ar +112 ,12 4Sn反应中小角关联粒子 ,由两体符合事件提取了α α关联函数 .用三体弹道理论模型MENEKA计算本底关联函数 ,用Monte Carlo方法计算探测效率函数 ,在扣除本底产额并考虑探测效率的修正后 ,对不同同位旋反应系统 40 Ar +112 Sn和 40 Ar+12 4Sn提取的相对态布居核温度分别是 4 .18±0 .2 50 .2 1MeV和 4 .10±0 .2 20 .2 0 MeV ;考察态布居核温度和粒子能量的关系时 ,观察到两个系统的发射温度均随着粒子能量的增加而降低 ,缺中子系统40 Ar +112 Sn中由低能时的 5 .13±0 .3 00 .2 6MeV降低到高能时的 3.87±0 .3 70 .2 9MeV ,丰中子系统 40 Ar +12 4Sn中由低能时的 5 .39±0 .3 00 .2 6MeV降低到高能时的 3.32±0 .2 80 .2 3 MeV .用激发热核衰变过程的同位旋选择性对这种同位旋相关性进行了解释

35MeV/u~(36)Ar+~(124)Sn反应中类弹产物的同位素分布特性

测量了 35MeV u36Ar +12 4 Sn反应中 5 .3°处类弹产物的同位素分布 ,观察到随着出射动能的增加 ,产物的平均中质比逐渐减小而接近弹核的平均中质比 .同位旋相关的量子分子动力学计算表明 ,随着反应时间的增加 ,类弹产物的平均出射动能逐渐减小而平均N Z值则逐渐增大 .另外 ,碰撞参数也影响类弹产物的同位素组成 :随着碰撞参数的减小 ,类弹产物的平均N Z值减小 .

30MeV/u~(40)Ar+~(112,124)Sn反应中的同位素产额比与核温度

系统研究了 3 0MeV u40 Ar+ 1 1 2 ,1 2 4 Sn反应中的轻粒子同位素产额比随角度和初始激发能的变化关系 .对于两个反应体系 ,均观察到3He 4He和6Li 7Li的产额比随角度的增加而增加 ,6He 4He和8Li 7Li随角度的增加而减小 .统计发射的运动学效应不能完全符合实验结果 .各种单同位素产额比与靶核的N Z比有关 ,表现出同位旋效应 ,而由双同位素比提取的核温度几乎没有靶核相关性

30MeV/u~(40)Ar+~(112,124)Sn反应后角能谱温度的同位旋效应

在 30MeV/u4 0 Ar +112 ,12 4 Sn反应中用平行板雪崩计数器实现了前冲余核的测量 .在不同的线性动量转移下用运动源模型拟合了后角的3 He,α和6He能谱 ,发现3 He的能谱斜率温度在12 4 Sn系统中高于112 Sn系统 ,而6He的温度在112 Sn系统中更高 ,α粒子在两个系统中没有明显差别 .用热核粒子蒸发过程衰变道的选择性对这种同位旋相关性进行了解释 .GEMINI的计算不能重现实验结果

35MeV/u~(36,40)Ar+~(112,124)Sn反应中同位旋自由度的弛豫

35MeV/u 36 ,40　Ar+ 112 ,12 4Sn反应中 ,在前角 5°和 2 0°观测到丰中子核与稳定核的产额比随粒子出射动能的增加而减小 ,而缺中子核与稳定核的产额比随动能的增加而增加 .对于某种元素 ,随着动能的减小 ,其平均中质比逐渐由弹核N/Z向靶核N/Z过渡 .这些现象表明在这样的入射能量下 ,周边或近周边碰撞过程中同位旋自由度没有完全达到平衡 .这种行为对两个靶核系统是相似的 ,但是同位素产额比的绝对值在 5°没有靶核相关性 ,而在 2 0°处却表现出明显的靶核相关性 .

在40MeV/u时~(112)Sn+~(112)Sn和~(124)Sn+~(124)Sn中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，研究了~(１１２)Ｓｎ＋~(１１２)Ｓｎ和~(１２４)Ｓｎ＋ ~(１２４)Ｓｎ两个反应系统在入射能量 Ｅ＝４０ＭｅＶ／ｕ时的多重碎裂。计算结果能与 实验值定性符合。观察到两个反应系统中，中等质量碎片多重性、中子多重性、 荷电粒子多重性与轻荷电粒子多重性之间的关联存在着明显的差别。另外，通 过与膨胀蒸发源模型及同位旋相关的渗透模型分析结果的比较，发现这种差别 主要是由同位旋相关的反应动力学所造成的。

Entrance channel dependence of the correlation function of IMFs in Ar-36+Sn-112,Sn-124 at 35MeV/u

The reduced velocity correlation functions of the Intermediate Mass Fragments (IMFs) were measured in the reactions of Ar-36+ Sn-112,Sn-124 at 35MeV/u. The anti-correlation at small reduced velocities is more pronounced in Ar-36+ Sn-124 system than that in Ar-36+ Sn-112 system. The difference of the correlation functions between the two reactions is mainly contributed by the particle pairs with high momenta. A three-body Coulomb repulsive trajectory code (MENEKA) is employed to calculate the emission time scale of IMFs for-the both systems. The time scale is 150fm/c in the Ar-36+ Sn-112 system and 120fm/c in the Ar-36+ Sn-124 system, respectively. A calculation based on an Isospin dependence Quantum Molecular Dynamics code (IQMD) reveals that the emission time spectrum of IMFs is shifted slightly leftwards in Ar-36+ Sn-124 compared with that in the Ar-16+ Sn-112 system, indicating a shorter emission time scale. Correspondingly, the central density of the hot nuclei decreases faster in Ar-36+ Sn-124 than in Ar-36+ Sn-112

Isospin diffusion and equilibration for Sn plus Sn collisions at E/A=35 MeV

Equilibration and equilibration rates have been measured by colliding Sn nuclei with different isospin asymmetries at beam energies of E/A = 35 MeV. Using the yields of mirror nuclei of Li-7 and Be-7, we have studied the diffusion of isospin asymmetry by combining data from asymmetric Sn-112 + Sn-124 and Sn-124 + Sn-112 collisions with those from symmetric Sn-112 + Sn-112 and Sn-124 + Sn-124 collisions. We use these measurements to probe isospin equilibration in central collisions where nucleon-nucleon collisions are strongly blocked by the Pauli exclusion principle. The results are consistent with transport theoretical calculations that predict a degree of transparency in these collisions, but inconsistent with the emission of intermediate mass fragments by a single chemically equilibrated source. Comparisons with quantum molecular dynamics calculations are consistent with results obtained at higher incident energies that provide constraints on the density dependence of the symmetry energy.

Constraints on the symmetry energy and neutron skins from pygmy resonances in Ni-68 and Sn-132

Correlations between the behavior of the nuclear symmetry energy, the neutron skins, and the percentage of energy-weighted sum rule (EWSR) exhausted by the pygmy dipole resonance (PDR) in Ni-68 and Sn-132 are investigated by using different random phase approximation (RPA) models for the dipole response, based on a representative set of Skyrme effective forces plus meson-exchange effective Lagrangians. A comparison with the experimental data has allowed us to constrain the value of the derivative of the symmetry energy at saturation. The neutron skin radius is deduced under this constraint.