相对论连续谱Hartree-Bogoliubov理论对滴线原子核结构的研究

回顾了相对论连续谱Hartree-Bogoliubov理论对奇特核结构的描述.包括对¹¹Li晕核的微观描述,并发现了其形成机制是由于Cooper对从1p_1/2轨道被散射到2s_1/2轨道;预言了滴线核的新现象——由6个中子组成的巨晕,给出了形成晕现象的条件为弱束缚与低离心位垒;解释了实际核中的赝自旋对称性;自旋轨道分裂与势能位垒弥散的关系;经典禁区内粒子对晕的影响;超重元素的结构研究等.     

轻丰中子核反应中子集团产生截面的理论研究

采用Boltzmann-Langevin方程研究了能量为35MeV/u的¹⁴Be, ⁸He,⁶He,¹¹Li,¹⁷B,¹¹Be,¹⁹C与¹²C靶的反应,计算了产生中子集团的截面, 发现^14,Be与¹²C靶反应产生⁴n的截面与实验值符合得很好. 通过这几个入射核与¹²C靶形成中子集团截面的对比, 发现核的晕中子越多产生中子集团的截面越大, 晕中子数相同时, 质量数越大产生中子集团的截面越大.中子集团可能主要来自晕核子.     

同位旋效应对N=9同中子素能级间隙的影响

在单粒子壳模型下, 研究了N=8及N=9同中子素的基态性质. 通过在伍兹--萨克逊势深中引入同位旋依赖项, 考虑了同位旋效应对核平均势的影响. 理论计算的均方根半径和自旋宇称值与实验结果整体上符合较好, 尤其是N=9同中子素中的2s_1/2与1d_5/2中子能级间的能级反转得到了较好的解释. 计算结果还显示在¹⁴B和¹⁵C基态中存在单中子晕.     

推广的Glauber理论及其在晕核散射中的应用

介绍了推广到晕核散射的Glauber理论,并用其研究晕核¹⁴Be的散射问题.弹核的密度分布分别采用谐振子密度分布和相对论平均场理论计算得到具有两个晕中子结构的密度分布,对晕核模型的多重积分采用蒙特卡洛数值积分方法.计算了不同能量下¹⁴Be,¹²Be与靶核¹²C散射的反应截面,并与实验结果进行比较,¹⁴Be的两个中子采用具有晕中子密度分布的理论计算与实验符合较好,而采用不具有晕中子密度分布的结果与实验值相差较大.     

自相似结构壳模型

为了扩展以简谐振子为基矢的常规壳模型(SM)计算到晕核,提出了自相似结构壳模型(SSM).通过对简谐振子动能项和势能项的重度规以及单粒子平均场模拟,可以得到SSM中的单粒子轨道有态相关的圆频率,在SSM中,晕核大的均方根半径、厚的中子皮以及Borromean晕核⁶He、¹¹Li和¹⁴Be的束缚态性质能够再现出来.     

丰中子核105Mo单中子带结构的识别

通过对重核²⁵²Cf自发裂变产生的瞬发γ谱的测量, 对丰中子核¹⁰⁵Mo的能级结构进行了研究. 除确认与扩展了基带转动带外, 新识别了3个转动带, 它们分别被指定为建立在Nilsson能级3/2⁺[411], 1/2⁺[411]和5/2⁺[413]轨道上的单中子激发带, 并对这些集体带的特性进行了讨论.     

25MeV/u 6He在9Be靶上引起的双中子转移

报道了经仔细设计的150MeV ⁶He+⁹Be实验,并在质心系大角度处测量¹⁰Be和¹¹Be同位素产物的实验数据.鉴别得到相应于单中子转移的371个¹⁰Be事件,同时观测到了相应于双中子转移的5个¹¹Be事件.由此得到相应微分截面分别为(0.11±0.02)mb/sr(θ_cm≈137.4°)和(1.0±0.7)μb/sr(θ_cm≈133.4°),结果表明在所研究的反应体系中,单中子转移截面要比双中子转移截面约大100倍.在⁶He由⁵He-n和α-2n组成的集团模型下,利用零力程扭曲波玻恩近似(DWBA)的计算程序,在数量级上重现了单、双中子转移反应的实验数据     

丰中子核113Ru集体转动带的识别

通过对重核²⁵²Cf自发裂变产生的瞬发γ谱的测量,对非常丰中子核¹¹³Ru的能级结构进行了研究,建立了较高自旋态的能级纲图,识别了基于中子h_11/2轨道激发产生的集体转动带,最高自旋态达31/2h.还发现了另一个可能基于9/2^－能级的集体转动带,对新建立的¹¹³Ru的集体带的一些重要特性进行了讨论.     

晕核11Li,14Be和17B的进一步研究

在三体模型的基础上,采用汤川作用势,进行变分计算,进一步研究了晕核¹¹Li,¹⁴Be和¹⁷B的基态性质,给出了晕中子密度分布的一个解析表达式.理论计算结果与最新的实验数据一致.     

94Mo高自旋态能级纲图

通过重离子融合蒸发反应¹⁶O(⁸²Se+4n)⁹⁴Mo布局了⁹⁴Mo核的高自旋态.利用多探头探测器阵列GASP进行了在束γ测量,从而重新研究了⁹⁴Mo核的高自旋态能级结构.基于新发现的一些重要的连接跃迁,对⁹⁴Mo核的高自旋态能级纲图做了重要修改.将新的能级结构与壳模型计算进行了比较和讨论.结果表明要正确的描述94?Mo核的高自旋态(自旋值大于14)能级结构,应考虑价中子在d_5/2,g_7/2和h_11/2轨道上的激发.     

晕核反应总截面和密度分布

利用考虑了量子修正、库仑修正、核子–核子碰撞同位旋效应和假定有效原子核密度分布后得到的改进的Glauber理论,计算了晕核与稳定核反应总截面,研究了晕核结构对反应总截面的影响.结果发现对于¹¹Be,¹⁴Be和¹¹Li等入射核,必须考虑它们的晕核结构和利用自由的核子–核子碰撞截面才能得到与实验符合的反应截面,并可依据反应总截面来确定晕核的密度分布和均方半径等信息.     

The neutron halo structure of 17B studied with the relativistic Hartree-Bogoliubov theory

The properties of neutron-rich boron isotopes are studied in the relativistic continuum Hartree-Bogoliubov theory in coordinate space with NL-SH, PK1 and TM2 effective interactions. Pairing corrections are taken into account by a density dependent force of zero range. The binding energies calculated for these nuclei agree with the experimental data quite well. The neutron-rich nucleus ¹⁷B has been predicted to have a two-neutron halo structure in its ground state. The halo structure of ¹⁷B is reproduced in a self-consistent way, and this halo is shown to be formed by the valence neutron level 2_s1/2.     

自相似结构壳模型

为了扩展以简谐振子为基矢的常规壳模型（ＳＭ）计算到晕核，提出了自相似结构壳模型（ＳＳＭ）．通过对简谐振子动能项和势能项的重度规以及单粒子平均场模拟，可以得到ＳＳＭ中的单粒子轨道有态相关的圆频率，在ＳＳＭ中，晕核大的均方根半径、厚的中子皮以及Ｂｏｒｒｏｍｅａｎ晕核和的束缚态性质能够再现出来。     

Nuclear structure near the drip line studied by RNB

The use of radioactive nuclear beams (RNB) has provided an opportunity to study nuclei far from the stability line. Reaction studies using intermediate and high-energy (30–1000 AMeV) radioactive beams have revealed new structures of nuclei that are not seen in nuclei near to the stability line [1]. One such new structure is the neutron halo, a long low-density tail of the neutron distribution [2]. It has been observed in neutron drip-line nuclei, such as⁶He,¹¹Li and¹¹Be. The neutron halo has put light on many new structure problems. Among those, recent studies of a softE1 mode, a low-frequency oscillation of halo neutrons against the core, are discussed in the following section in connection with a recent (p, p′) reaction measurement [3]. Also, the effect of changes in single-particle orbitals on halo formation is discussed [4]. Another new finding is the formation of neutron skins in neutron-rich unstable nuclei [5]. The relation between the equation-of-state (EOS) of asymmetric nuclear matter and the neutron-skin thickness as well as the density distribution of nuclei far from the stability line is discussed in the last section.     

晕核~（11）Li，~（14）Be和~（17）B的进一步研究

在三体模型的基础上，采用汤川作用势，进行变分计算，进一步研究了晕核１１Ｌｉ，１４Ｂｅ和１７Ｂ的基态性质，给出了晕中子密度分布的一个解析表达式．理论计算结果与最新的实验数据一致．     

α-clustering in Be isotopes

The Be chain of isotopes is investigated within the Sernimicroscopic Algebraic Cluster Model (SACM). For that the SACM is extended to odd-mass p-shell nuclei. We show that the main features of the Be isotopes can be well explained. Though for the neutron halo nucleus ¹¹Be some problems remain, the shell model still can describe the rough structures of these nuclei. In ¹¹Be a shell inversion takesplace reflecting the high deformation of the system. The quadrupole—quadrupole interaction plays a dominant role in p-shell nuclei.     

Two-body and three-body halo nuclei

We have extracted the nuclear asymptotic normalization coefficients (ANC) for the virtual transitions B→A+N via some transfer reactions and the radioactive nuclear beam experiments. With these coefficients, root-mean-square (rms) radii for the valence particle in some possible halo nuclei have been calculated. The values of rms radii extracted with ANC approach are nearly model-independent, hence are a good quantity for the investigation of nuclear halo. In addition, we have also calculated the rms radii for the two valence neutrons in some three-body systems in terms of the relationship between the radii of valence particle, core nucleus and nuclear matter. With two conditions for nuclear halo formation, we have examined these extracted rms radii. The results show that 11Be(1/2+, g.s), 12B(1-, 2.621 MeV), 13C(1/2+, 3.089 MeV), 14C(0-, 6.903 MeV), 14C(1-, 6.094 MeV), 15C(1/2+, g.s) and 19C(1/2+, g.s) with the valence particle in the 2s ground or excited state are the neutron halo nuclei, whereas 17F(1/2+, 0.495 MeV) and 21Na(1/2+, 2.423 MeV) are the proton halo nuclei in the excited state. For three-body systems, except the well-established two-neutron halo nuclei 6He and 11Li, 14Be and 17B might be the two-neutron halo nuclei as well.     

Self-Similar Strcture Shell Model

In Order to extend the conventional shell model(SM) calculation with harmonic oscillator bases to halo nuclei, a self-similar, structure shell model(SSM) is proposed. The SSM is achieved by a rescaling of both the Kinetic and potential energy term of the harmonic oscillator and a mean field imitation, so that the single particle orbit in SSM has state (orbit) -dependent frequency. The large r. m. s. radius and the thick neutron skin for halo nuclei as well as the bound state properties of Borromean nuclei such as ⁶He, ¹¹Li and ¹⁴Be can be reproduced.