25MeV/u 40Ar+93Nb反应中热核的激发能和核温度

利用半导体望远镜探测器和PPAC对25MeV/u ⁴⁰Ar+⁹³Nb反应中的带电粒子和余核进行了关联测量,对所得α粒子能谱用三源模型进行了拟合,并由余核飞行时间和粒子多重性得到热核激发能.通过对温度的修正,发现在本实验中有激发能E^*/A为4.3MeV,温度T_init为6.9MeV的热核形成.通过与其它实验结果的对比可以看出核物质在轻系统和重系统中行为的差异.     

形变对10.6MeV/u 84Kr+27Al反应裂变前粒子发射的影响

研究了形变效应对10.6MeV/u ⁸⁴Kr+²⁷Al反应中断前粒子发射的影响.发现通过测量的裂变前粒子多重性提取的裂变延迟时间将因此从20×10^－21s减少到5×10^－21s,表明增强的断前粒子发射有一部分来自形变效应的贡献.     

25MeV/u 40Ar+natAg、209Bi反应中热核的温度和激发能测量

在25MeV/u ⁴⁰Ar+^natAg、²⁰⁹Bi反应中,用4个PPAC和11组望远镜完成了关联裂变碎片与发射轻粒子的符合测量,角关联描绘为两个被探测到碎片折叠角θ_ff的函数,线性动量转移〈LMT〉由测量到的角关联推出.将符合测量得到的对应于不同窗的后角轻带电粒子能谱用Maxwell分布来拟合其谱的后沿,经过一些修正,由能谱得到热核的初始温度T_int,在考虑反应Q值和预平衡发射的修正之后,可以得到不同窗所对应的激发能.实验结果表明,在⁴⁰Ar+^natAg、²⁰⁹Bi反应的中心碰撞中激发能分别为4.2、2.4MeV/u,而温度达6.1、5.5MeV,在半中心碰撞中激发能为3.5、1.9MeV/u,温度可达5.8、4.8MeV.     

在30MeV/u 40Ar+159Tb、natAg反应中比较热核两种温度值

用双同位素产额比方法和能谱斜率方法,在110°对30MeV/u ⁴⁰Ar+¹⁵⁹Tb和^natAg反应得到的热核的温度进行了研究.对于不同的双同位素产额比,同位素温度值相同,为4.6MeV.能谱斜率温度随粒子或复杂碎片的不同而异.从α粒子能谱和质量数小于4的粒子能谱得到的斜率温度均是正常的,但是更重的碎片的斜率温度则高于极限温度Tlim,这可能是更重的碎片发射于复合核形成后的早期阶段,或者是库仑不稳定的发射.同时还分析了斜率温度高于极限温度T_lim的较重碎片能谱随探测角的变化.     

转动自由度对10.6MeV/u 84Kr+27Al反应中裂变前粒子增强发射的影响

在统计模型的框架内研究了In核在三维空间的转动自由度对10.6和8.5MeV/u ⁸⁴Kr+²⁷Al碰撞裂变前粒子发射的影响.发现对后一个轰击能,断前粒子发射不敏感于转动自由度;对前一个能量,转动自由度的引入使提取的裂变延迟时间从20×10^－21s减少到7.5×10^－21s,表明了它对裂变前粒子蒸发的影响,计算结果也表明仅有转动自由度并不能完全解释In核的断前粒子增强发射现象.发现了转动自由度在粒子发射中所起的作用对系统的激发能有一定的依赖关系.     

10.6MeV/u 84Kr+27Al反应中角动量对断点前粒子多重性的影响

用推广的裂变扩散模型研究了角动量对10.6MeV/u ⁸⁴Kr(²⁷Al,二体裂变)反应断点前粒子多重性的影响,发现阶点前粒子多重性和断点时间随着角动量的减小逐渐增大,而且绝大多数粒子是在鞍点前发射的. 对实验中二体裂变反应发生的角动量范围进行权重平均,得到了与实验一致的断点前粒子多重性. 同时还研究了影响断点前粒子多重性和断点时间的诸多因素.     

25MeV/u 40)Ar+209Bi裂变反应研究

实验对25MeV/u ⁴⁰Ar+²⁰⁹Bi体系的裂变反应,利用线性动量转移的分窗选择不同的激发能,研究裂变动能分布和质量分布与热核初始激发能的关系.实验证实激发能小于380MeV时裂变总动能分布与低激发能复合核相似.激发能大于380MeV时,最可几动能呈现出随激发增加而增加,并出现高能非对称性,而且质量分布宽度随激发能增加而迅速增大.     

35MeV/u 40Ar+197Au反应中复合核的激发能与温度

利用大面积位置灵敏气体探测器对35MeV/u ⁴⁰Ar+¹⁹⁷Au反应中形成的裂片进行了符合测量,由此得到了裂变复合核的速度分布.在大质量转移假设下扣除前平衡发射粒子的影响,得到复合核的激发能.另外利用望远镜探测器对反应中出射的轻带电粒子也进行了符合测量,并由后角α,p,d,t的能谱提取了复合核的温度.温度与激发能的关系没有表现出理论预言的相变特征.     

25MeV/u 40Ar+93Nb反应中热核巨共振研究

对25MeV/u ⁴⁰Ar+⁹³Nb反应形成的热核发射的γ射线、轻带电粒子和蒸发余核进行了符合测量,从余核的飞行时间和轻带电粒子能谱得出非完全熔合反应形成的热核的初始激发能.GDR γ衰变的产额在研究的激发能范围内保持不变.用统计模型CASCADE程序对实验结果进行分析. 讨论了引起GDRγ衰变产额饱和的原因.当假定热核激发能大于250MeV时无GDR γ发射,则可以用CASCADE程序很好地拟合E_γ大于12MeV的实验谱.     

40Ar+197Au(25MeV/u)产生的热核激发能与核温度的关系

对25MeV/u ⁴⁰Ar+¹⁹⁷Au反应系统裂变与后角轻粒子发射进行了符合测量,用裂变碎片折叠角和裂变碎片的飞行时间再构转移到类熔合核的线性动量.通过对线性动量转移和轻带电粒子能谱测量,给出从中心碰撞到周边碰撞产生的类熔合核的初始激发能、角动量和核温度,讨论它们的关系.发现了中心碰撞形成的类复合核的核温度已经接近饱和状态,接近多重碎裂的“准相变区”.     

~(236)U Multi-modal Fission Paths on a Five-dimensional Deformation Surface

In this paper, we develop a new path search algorithm which considers all the degrees of freedom and apply it on our calculated five-dimensional potential energy surface(PES) of~(236) U. Asymmetric and symmetric fission paths and barriers are obtained.     

238U(n,f)短寿命产物核累积产额的评价(英文)

为满足堆内或核爆中链式反应过程的燃耗值的计算需要，对裂变谱中子和14MeV中子诱发238U裂变的短寿命产物核的累积产额进行了评价。评价利用了所有可利用的实验数据， 经物理分析后， 使用AVERAGE程序加权平均， 用ZOTT程序进行同时评价， 给出了所要求能点的唯一最佳推荐数据， 并将评价结果与ENDF/B-VII， JEF-2.2， JENDL-3.2和CENDL-2的推荐数据进行了比较。 评价结果将用于CENDL-2的更新与升级。For reliable and consistent nuclear calculation, the cumulative yields for short lived fission products are evaluated based on the available experimental data for 238U fission induced by fission spectrum neutrons and ~14 MeV neutrons. The data are processed using codes AVERAGE for weighed average and ZOOT for simultaneous evaluation. The evaluated data are compared with those in the major international nuclear data libraries, including ENDF/B-VII, JEF-2.2, JENDL-3.2 and CENDL-2. The present evaluation will be used to improve and update the CENDL-2 library.     

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.     

Bremsstrahlung neutrino energy loss for ~(24)Mg, ~(28)Si, ~(32)S, ~(40)Ca, ~(56)Fe in strong electron screening

Based on WeinbergoSalam theory the bremsstrahlung neutrino energy loss for nuclei ~(24)Mg, ~(28)Si, ~(32)S, ~(40)Ca and ~(56)Fe are investigated in strong electron screening. Our results are compared with those of Dicus' and show that the latter are higher by 2 orders of magnitude in the density-temperature region of 10~8 g/cm~3 ≤ρ/μ_e≤10~(11) g/cm~3 and 2.5 ≤ T_9 ≤4.5. On the other hand, the factor C shows that the maximum differences are 99.16%, 99.13%, 99.12%, 99.055%, 99.040% corresponding to the nuclei ~(24)Mg, ~(28)Si, ~(32)S, ~(40)Ca and ~(56)Fe.     

High-lying excited states in ~(10)Be from the ~9Be(~9Be,~(10)Be)~8Be reaction

A transfer-reaction experiment of ~9Be(~9Be,~(10)Be)~8Be was performed at a beam energy of 45 Me V.Excited states in ~(10)Be up to 18.80 Me V are produced using missing mass and invariant mass methods.Most of the observed high-lying resonant states,reconstructed from theα+~6He and t+~7Li decay channels,agree with the previously reported results.In addition,two new resonances at 15.6 and 18.8 Me V are identified from the present measurement.The 18.55 Me V state is found to decay into both the t + ~7Lig:s: and t + ~7Li?(0.478 MeV) channels, with a relative branching ratio of 0:93 ± 0:33. Further theoretical investigations are encouraged to interpret this new information on cluster structure in neutron-rich light nuclei.     

Bremsstrahlung neutrino energy loss for ~(24)Mg,~(28)Si,~(32)S,~(40)Ca,~(56)Fe in strong electron screening

Based on Weinberg-Salam theory the bremsstrahlung neutrino energy loss for nuclei 24Mg,28Si,32S,40Ca and 56Fe are investigated in strong electron screening.Our results are compared with those of Dicus' and show that the latter are higher by 2 orders of magnitude in the density-temperature region of 108 g/cm3 ρ/μe 1011 g/cm3 and 2.5 T9 4.5.On the other hand,the factor C shows that the maximum differences are 99.16%,99.13%,99.12%,99.055%,99.040% corresponding to the nuclei 24Mg,28Si,32S,40Ca and 56Fe.     

Simulation of the fission dynamics of the excited compound nuclei ~(206)Po and ~(168)Yb produced in the reactions ~(12)C+~(194)Pt and ~(18)O+~(150)Sm

A two-dimensional dynamical model based on the Langevin equation was used to study the fission dynamics of the compound nuclei ~(206)Po and ~(168)Yb produced in the reactions ~(12)C+~(194)Pt and ~(18)O+~(150)Sm,respectively.The fission cross section and average pre-scission neutron multiplicity were calculated for the compound nuclei ~(206)Po and ~(168)Yb,and results of the calculations compared with the experimental data.The elongation coordinate was used as the first dimension and the projection of the total spin of the compound nucleus onto the symmetry axis,K,considered as the second dimension in the Langevin dynamical calculations.In the two-dimensional calculations,a constant dissipation coefficient of K and a non-constant dissipation coefficient have been used to reproduce the abovementioned experimental data.It is shown that the two-dimensional Langevin equation can satisfactorily reproduce the fission cross section and average pre-scission neutron multiplicity for the compound nuclei ~(206)Po and ~(168)Yb by using constant values of the dissipation coefficient of K equal to γκ=0.18(MeV zs)~(-1/2) and γκ= 0.20(MeV zs)~(-1/2)for the compound nuclei ~(206)Po and ~(168)Yb,respectively.     

Experimental research into the two-proton emissions from ~(17,18) Ne,~(28) P and ~(28,29)S

Two-proton emissions from the excited states of 17,18Ne, 28P and 28,29S were investigated experimentally by the radioactive beams bombarding on the 197Au target via the Coulomb excitation. The complete-kinematics measurements were actualized by the stacks of silicon-strip detectors and CsI+PIN array detectors. The invariant mass of final systems as well as the relative momentum, opening angle, and relative energy of the two emitted protons was reconstructed under the framework of relativ istic kinematics. V...