AMS measurement of In-situ produced cosmogenic 10Be in Loess Quartz in Luochuan

Loess is the most important and the most typical continental classic sediments of Quaternary. So the measurement of In-situ produced cosmogenic ¹⁰Be is expected to be used for the Loess stratigraphic age. But the production rate of In-situ produced cosmogenic ¹⁰Be in Loess quartz is very low. It requires very high sensitivity and accuracy of measurement. This work has measured the concentrations of ¹⁰Be of two layers in Loess section of Luochuan including L8, L9 and the concentrations of ¹⁰Be in (of) blank sample with the HI-13 AMS system at China Insitute of Atomic Energy(CIAE), then calculated the content of ¹⁰Be in loess quartz for each layer. The ratio of ¹⁰Be/⁹Be was found in the range of 10^－13. The background of ¹⁰Be/⁹Be was about 3×10^－14.     

产生超对称态的几种可能途径

在以前工作的基础上,计算了飞行 K^-奇异交换反应⁹Be（K^-,π^-）_A⁹Be 和¹³C（K^-,π^-）_A¹³C 的角分布.在平面波冲量近似下,计算了协同产生反应到达超核 _A⁹Be、_A¹³C 的奇异相似态和超对称态的微分截面的相对比,并且估算了这些微分截面绝对值.根据这些计算,讨论了通过奇异交换反应和协同产生反应产生超对称态的可能性.     

8Be核自发裂变的微观研究

应用双阱集团壳模型,提出⁸Be 自发裂交静力学位垒计算中扣除碎片相对动能的一种方式,计算了⁸Be 自发裂变位能曲面,并对库仑位及质心运动伪态的修正作了估算.定性地解释了⁸Be 的亚稳机制,并提供了从微观方式描述变裂的一种理论方式。     

Skyrme-Hartree-Fock计算11Be的晕结构

用形变的Skyrme-Hartree-Fock计算讨论了¹¹Be的晕结构. 通过引入绝热堵塞计算, 得到了¹¹Be的1/2⁺态有很大的形变, 得到的密度分布和实验值很好地符合. 还讨论了出现形变晕态的波函数密度分布和角动量大小等问题.     

12C+112,124Sn反应中靶核中子数对出射粒子截面的影响

实验研究了入射能量E_l=70.0MeV的¹²C+¹¹²Sn和¹²C+¹²⁴Sn两个反应. 使用ΔE-E半导体探测器, 测量了两反应中出射的α、Li、Be、B各粒子的能谱和角分布. α粒子的角分布可以通过假定存在三种机制的α组份得到定性的解释. Li、Be、B的角分布为擦边角成峰, 无前角成峰组份.     

一种可能的新型反应机制——双α直接转移反应

假定8Be是由两个在组态空间相邻的α粒子组成的, 因而获得在余核中⁸Be集团的谱密度正比于核表面α粒子预形成几率P_α的平方. 利用改进了的EFRDWBA重叠积分的参数化方法^[1—2], 我们计算了²⁰⁹Bi(¹²C, α)²¹⁷Fr反应中出射的α粒子的角分布和双微分能谱, 而且通过拟合实验数据提取了在²¹⁷Fr核表面的α粒子的预形成几率, 结果与由α衰变数据提取的预形成几率在计算误差范围内一致. 这个事实说明, ²⁰⁹Bi(¹²C, α)²¹⁷Fr可能是双α直接转移反应.     

能量稍高于库仑位垒12C+209Bi反应实验数据的补充分析

本文利用部分熔合机制,给出了一种可能的解释,说明为什么在入射能量稍高于库仑位垒的¹²C+²⁰⁹Bi反应中⁸Be转移几率较大,α转移几率却几乎可以忽略。     

重离子引起的单质子转移反应40Ar(11B, 10Be)41K

测量了50MeV的¹¹B束在40Ar上的弹性散射角分布和单质子转移反应⁴⁰Ar(¹¹B, ¹⁰Be)⁴¹K的微分截面. 用光学模型拟合了弹性散射截面. 用包含反冲效应的精确有限程扭曲波玻恩近似(EFR-DWBA)分析了微分截面, 提取了谱因子.     

关于Λ-α有效相互作用以及超核6He与9Be的研究

本文用给出⁵He的Λ结合能实验值的Λ-α有效相互作用, 统一地用超球谐函数方法的绝热近似, 研究了超核⁶He的双Λ结合能与⁹Be的Λ结合能. 得到的结果比较满意的.     

Measurements of stellar and explosive nuclear astrophysics reactions

This paper described the nuclear astrophysical studies using the unstable ion beam facility GIRAFFE in CIAE, by indirect measurements. We measured the angular distributions for some single proton or neutron transfer reactions, such as ⁷Be(d,n)⁸B, ¹¹C(d,n)¹²N, ⁸Li(d,p)⁹Li and ¹³N(d,n)¹⁴O in inverse kinematics, and derived the astrophysical S-factors or reaction rates of ⁷Be(p,γ)⁸B, ¹¹C(p,γ)¹²N, ⁸Li(n,γ)⁹Li, ¹³N(p,γ)¹⁴O by asymptotic normalization coefficient, spectroscopic factor, and R-matrix approach at astrophysically relevant energies. Some most recent progress of nuclear astrophyiscal work in CIAE are also summarized.     

OBEP在某些有限核的Hartree-Fock计算中的应用

本工作以忽略了自旋轨道耦合项和张量项的单玻色子交换势作为核子-核子的相互作用势, 用Hartree-Fock方法计算¹⁶O、¹²C和⁸Be的基态结合能、核半径和粒子波函数, 得到了令人满意的计算结果.     

尝试利用导致连续态的α转移反应提取重核表面的α集团的预形成几率

本文完善了T.Udagawa和T.Tamura等人^[1]发展的参数化方法, 利用EFR-DWBA程序分析导致连续态的²⁰⁸Pb(¹²C, ⁸Be)²¹²Po的α转移反应的实验双微分能谱, 从中提取了在²¹²Po核表面α粒子的预形成几率, 结果与由α衰变实验数据提取的预形成几率在计算误差范围内一致.     

粲Λ-核子相互作用和粲Λ核结合能

本文用Hartree-Fock方法计算了Λ超核⁵_ΛHe与⁹_ΛBe的Λ的结合能及粲Λ(Λ_c)核⁵_ΛHe与⁹_ΛBe的Λ_c的结合能. 在使前两者的Λ结合能之比与后两者的Λ_c结合能之比相等时, 定出Λ_c与核子的相互作用约为Λ与核子的相互作用的4/5. 用此相互作用计算了1p壳Λ超核和Λ_c核的结合能, 结果表明核芯A≥4的Λ_c核是存在的.     

Structure of A=11 double-Λ hypernuclei studied withthree-body forces

The energy levels and ΛΛ bond energy of the double-Λ hypernucleus ¹¹Be are calculated considering two- and three-nucleon forces. The interactions between the constituent particles are contact interactions that reproduce the low-energy binding energy of the nuclei. Effective action is constructed to involve the three-body forces. In this paper, we compare the binding energy result that is obtained with the experimental and other modern nucleon-nucleon potentials. The results of all the schemes agree very well, showing the high accuracy of our present ability to calculate the many-nucleon bound state with three-body forces. The experimental value of B_{Λ Λ}(_ΛΛ¹¹Be)=20.83 MeV seems to be more compatible with our calculated value of B_ΛΛ(_ΛΛ¹¹Be)=19.31 MeV in comparison with the calculated result of 18.23 MeV by Hiyama et al.     

128Ba激发态的观测

通过反应¹²⁰Sn(12C,4nγ)¹²⁸Ba, 用在束γ测量方法研究了¹²⁸Be的激发态. 从935.0keV γ射线确认了第二个12⁺态, 但它仍不属于基态带. 另外还新观测到224.8keV和632.7keV的带间跃迁, 并确认它们是由负宇称带向基态带的跃迁.     

12C+209Bi生成的Fr和At同位素激发函数测量

用能量为60—72MeV的¹²C束轰击²⁰⁹Bi靶,测量了Fr和At同位素的激发函数,确定了²¹³Fr和²¹⁴Fr分别是²⁰⁹Bi(¹²C,4n)Ac²¹⁷和²⁰⁹Bi(¹²C,3n)Ac²¹⁸的反应产物Ac同位素再经一次α衰变后形成的;而^214mFr可能是复合核蒸发中子和一个α粒子即(¹²C,α3n)机制产生的.²¹¹At主要是多核子转移反应（例如⁸Be转移）的贡献.将蒸发中子反应的实验结果用Jackson公式进行了拟合.     

Preparations for the study on the cluster structure of 16C

In order to look for a proposed cluster structure of ¹⁶C, simulation work was made. The simulation of the reaction dynamics give the resolution of the excitation energy on ¹⁶C which was reconstructed prior to breakup. The excitation energy resolution is typically ~200 keV at 2 MeV above the two body decay threshold for ¹⁶C→¹²Be+⁴He. Moreover,some performances of detectors tested using ²⁴¹Am α source are also reported.     

Isospin dependence of projectile fragmentation and neutron-skin thickness of neutron-rich nuclei

By investigating the cross section distributions of fragments produced in the 140 A MeV ^40,48Ca+⁹Be and 1 A GeV ^124,136Xe+Pb reactions, the isospin dependence of projectile fragmentation in fragment production is studied. In the framework of the statistical abrasion-ablation model, the 1 A GeV ¹³⁶Xe+²⁰⁸Pb reaction is calculated. By adjusting the diffuseness parameter in neutron density distribution of ¹³⁶Xe, we find the isospin dependence of projectile fragmentation in fragment production is sensitive to the neutron-skin thickness of the projectile nucleus.     

α粒子的准弹性敲出反应

使用独立α粒子模型波函数, 在eikonal扭曲波冲量近似下, 对入射能量为100MeV的准弹性敲出反应¹²C(p, pα)⁸Be进行了计算. 理论结果较好地与实验符合, 从而进一步地检验了独立α粒子模型的可靠性.