Neutron halos in the excited states for N=127 isotones

Properties of the ground states and the excited states of N=127 isotones are investigated by using the nonlinear relativistic mean field theory with the interactions PK1. By analyzing the rms of proton and neutron, the single particle energies of valence nucleon and the density distributions of neutron, proton and the last neutron, it can be found that there exists a neutron halo in the excited states of 3d5/2, 4s1/2 and 3d3/2 in 209Pb. It is also predicted that there exists a neutron halo in the excited states of 3d5/2, 4s1/2 and 3d3/2 in 207Hg, 208Tl, 210Bi and 211Po.     

Neutron halos in the excited states for N=127 isotones

Properties of the ground states and the excited states of N=127 isotones are investigated by using the nonlinear relativistic mean field theory with the interactions PK1. By analyzing the rms of proton and neutron, the single particle energies of valence nucleon and the density distributions of neutron, proton and the last neutron, it can be found that there exists a neutron halo in the excited states of 3d5/2, 4s1/2 and 3d3/2 in ²⁰⁹Pb. It is also predicted that there exists a neutron halo in the excited states of 3d5/2, 4s1/2 and 3d3/2 in ²⁰⁷Hg, ²⁰⁸Tl, ²¹⁰Bi and ²¹¹Po.     

同位旋效应对F同位素s-d能级间隙的影响

在单粒子势模型的框架下, 计算了O同位素和F同位素的基态和某些低激发态的能级值、均方根半径值及密度分布。通过在伍兹 萨克逊势中引入同位旋依赖项, 研究了同位旋效应对F同位素s-d能级间隙的影响。理论计算得到的均方根半径值和自旋宇称值与实验结果一致。尤其是, 理论计算能够实现16F, 15F和14F中2s_1/2与1d_5/2质子能级间的反转, 且F同位素中s-d质子能级间隙及其整体变化趋势与已知实验结果符合较好。此外, 理论结果表明17F的(1/2)+第一激发态为单质子晕态。 The level structures of O and F isotopes are investigated in the framework of the single particle potential model. The isospin effect on the s d level spacing in F isotopes is studied by introducing an isospin dependent term in the depth of the Woods Saxon potential. The theoretical results of RMS radii and spin parity values are in agreement with the experimental data. In particular, the level inversion between proton levels of 2s_1/2 and 1d_5/2 in 16F, 15F and 14F is reproduced. The global tendency of the s-d level spacing agrees with the observed fact. In addition, the study confirms the one proton halo structure in 17F(2s_1/2).     

镜像核13N-13C 和15N-15O中的激发态晕或皮(英文)

用非线性相对论平均场对两对镜像核13N-13C 和15N-15O进行了研究. 发现无论在基态还是激发态， 用两套参数所得的结合能都跟实验值很接近. 计算结果显示13N的第一激发态（2s1/2）和第三激发态（1d5/2）各存在一个非束缚的质子晕， 而13C的第三激发态（1d5/2）存在一个弱束缚的中子皮. 另外研究表明, 在另一对镜像核15N-15O的第二激发态（2s1/2）和第一激发态（2s1/2）分别存在一个中子晕和质子皮. Properties of two pairs of mirror nuclei 13N-13C and15N-15O are investigated by using the nonlinear relativistic mean field theory. It is found that all the calculated binding energies with two different parameter sets are very close to the experimental ones for both the ground states and the excited states. The calculations show that the first excited state (2s1/2) and the third excited state (1d5/2) in 13N are both unbound resonances with proton halo structure, whereas the third excited state (1d5/2) in 13C is weakly bound with a neutron skin. It is also predicted that there has a proton halo in the second excited state (2s1/2) of 15N as well as a neutron skin in the first excited state (2s1/2) of 15O.     

Proton Halo or Skin in the Excited States of Light Nuclei

Properties of nuclei 13,15,N and 9B are investigated in the relativistic mean-field theory with NLz and NL3 force parameters.The calculated binding energies are very close to the experimental ones.The calculations show that the first excited state (1p1/2) in 9B,the first excited state (2s1/2)in 13 N and the second excited state(2s1/2) in 15N are weakly bound .In particular,for 13N and 15N,the proton density distributions in the two above excited states have a long tail and the rms radii of the last proton are greatly larger compared with their respective matter radii.It is predicted that a proton halo exists in the first excited state of 13N and in the second excited state of 15N,respectively.It also indicates that the first excited state in 9B is a proton skin state.     

Investigation of Exotic Structure of the Largely Deformed Nucleus ^23A1 in the Relativistic-Mean-Field Model

A candidate for proton halo nucleus ^23A1 is investigated based on the constrained calculations in the framework of the de[ormed relativistic mean tield (RMF) model with the NL075 parameter set. It is shown by the constrained calculations that the ground state of ^23A1 has a large deformation that corresponds to the prolate shape. With that large deformation, the non-constrained RMF calculation predicts that there appears an inversion between the 2s1/2 [211] and ld5/2 [202] shells. The valence proton of ^23A] is weakly bound and occupies 2s1/2 [211] and ld5/2 [202] with the weights of 56% and 29%, respectively. The calculated RMS radius for matter is in agreement with the experimental one. It is also predicted that the difference between the proton RMS radius and the neutron one is very large, This suggests that there exists a proton hMo in ^23Al.     

Theoretical Analysis of the Exotic Structure of ^17F

The first excited state and the ground state of ^17F are studied with the asymptotic normalization coefficient method. The results show that the probabilities of the last proton being out of the binding-potential in both the states are P = 59.71% and P = 27.61%, respectively. This means that the last nucleon in both the states of ^17F is far-extended beyond the range of nuclear force, especially in the first excited state. This result is also verified by the calculation of the density distributions of the last proton in ^17F. It is quantitatively confirmed that the first excited state of^1TF is a nuclear halo state and its ground state is a proton skin state.     

Density effect of the neutron halo nucleus induced reactions in intermediate energy heavy ion collisions

Using an isospin-dependent quantum molecular dynamics (IQMD) model, we study the 15C induced reactions from 30-120 MeV/nucleon systematically. Here the valence neutron of 15C is assigned at both 1d5/2 and 2s1/2 states respectively in order to study the density effect of reaction mechanism. It is believed that the existent neutron halo structure at the 2s1/2 state of 15C will affect the light particle emission evidently. In our calculation, the different density distributions of 15C at two states are calculated by relativistic mean field (RMF) model and introduced in the initiation of IQMD model, respectively. It is found that some observables such as emission fragmentation multiplicity, emission neutron/proton ratio and emission neutrons’ kinetic energy spectrum are sensitive to the initial density distribution.     

超重核的壳结构

在相对论连续谱Hartree Bogoliubov(RCHB)理论框架下,在质子数Z=100—140和中子数N=Z+30—2Z+32等偶偶核中进行了超重球形双幻核的探索.采用的有效相互作用为NL1,NL3,NLSH,TM1,TW 99,DD ME1,PK1和PK1R.基于对双核子分离能(S2p和S2n)、双核子能隙(δ2p和δ2n)、壳修正能量(Epshell)、对能(Eppair和Enpair)和有效对能隙(Δp和Δn)等物理量和能shell和En级结构的分析,预言了可能的质子幻数和中子幻数,并观察到在超重核区壳的弱化现象. The magic proton and neutron numbers are searched in the superheavy region with proton number Z=100 —140 and neutron number N=(Z+30) — (2Z+32) by the relativistic continuum Hartree-Bogoliubov (RCHB) theory with interactions NL1, NL3, NLSH, TM1, TW99, DD-ME1, PK1, and PK1R. Based on the two-nucleon separation energies S_(2p )and S_(2n) , the two-nucleon gaps δ_(2p) and δ_(2n), the shell correction energies E~p_(shell) and E~n_(shell), the pairing energies E~p_(pair) and E~n_(pair), and...     

Isospin effect of the in-medium nucleon-nucleon cross section in excited nuclear reactions

Using relativistic mean field theory, the neutron and the proton density distribution of 56Ni nuclei could be obtained in the ground state and the excited state. Based on the framework of the quantum molecular dynamics model, the 56Ni nuclei have been simulated in ground state and in the neutron or proton excited state. We then used the three different states of 56Ni to collide with the 56Ni in the ground state. To discuss the evolution of the nuclear stopping in different reactions, two kinds of different excited nuclear reactions were studied at different reaction energies and at different impact parameters. Studies have shown that the nuclear stopping of an excited nuclear reaction is sensitive to the isospin-dependent in-medium nucleon-nucleon cross section, compared with the response value of the ground state nuclear reaction. So, it is better for the excited nuclei to extract the isospin dependence of nucleon-nucleon cross section information.     

High Accuracy Calculation for Excited-State Energies of H Atoms in a Magnetic Field

Using the recently developed finite-basis-set method with B splines, excited states of H atoms in a magnetic field have been calculated. Energy levels are presented for the ten excited states, 2s₀, 3d'₀, 3p₀, 3p_-1, 3d_-1, 4d_-1, 3d_-2, 4d_-2, 4f_-2, and 5f_-2 as a function of magnetic field strengths with a range from zero up to 2.35 ×10⁶ T. The obtained results are compared with available high accuracy theoretical data reported in the literature and found to be in excellent agreement. The comparison also shows that the current method can produce energy levels with an accuracy higher than the existing high accuracy method [Phys. Rev. A 54 (1996) 287].Here high accuracy energy levels are for the first time reported for the 3d'₀, 4d_-1, 4d_-2, 4f_-2, and 5f_-2 states.     

氩气含量对介质阻挡放电中单丝等离子体温度的影响

在空气与氩气组成的混合气体放电中,首次研究了由中心点和外层晕组成的单丝。从照片中观察单丝结构,发现混合气体中氩气所占的比例越重,单丝的直径随之越小,同时中心点和外层晕的亮度有明显的差异,说明中心点和外层晕可能处于不同的等离子体状态。实验对单丝结构进行了光学时空分辨测量,研究了中心点和外层晕两层结构的微观特性。利用发射光谱法,详细地研究了该单丝结构的中心点和外层晕的等离子体参数随氩气含量的变化关系。实验根据氮分子第二正带系(C3Π_u→B3Π_g)谱线计算了中心点和外层晕的分子振动温度;通过氮分子离子N+₂(391.4 nm) 第一负带系谱线与氮分子N₂(394.1nm)谱线强度比,反映中心点和外层晕的电子平均能量随氩气含量的变化关系;利用氩原子763.2 nm(2P₆→1S₅)和772.077 nm(2P₂→1S₃)两条谱线的相对强度比法,估算了中心点和外层晕的电子激发温度。结果表明：中心点的光信号对应着第一个电流脉冲, 且其光信号较弱;而外层晕的光信号同时对应着第一个和第二个电流脉冲, 且其光信号较强。在相同的氩气含量条件下,外层晕比中心点的分子振动温度、电子平均能量以及电子激发温度均要高。随着氩气含量从30%逐渐增大到50%,中心点和外层晕的分子振动温度是逐渐减小的,而电子平均能量和电子激发温度均是逐渐增大的。     

团簇离子在固体中能损的非线性效应

研究了每核子能量为 2 6 0— 4 5 0keV的H₊2,H₊3,H₊4 H₊5和H₊7团簇离子在金膜中的能损 .发现团簇离子中平均每个质子的能损大于相同速度的单质子能损 ,即能损比大于 1,且随团簇离子的大小和速度的增加而增加. The energy losses of cluster ions H₊2,H₊3,H₊4 H₊5 and H₊7with energy of 260-450 keV/p in solid films have been measured. It has been found that the energy loss per proton in clusters is larger than that of single proton with the same velocity as clusters, that is, the energy ratio is larger than 1. Energy ratio increases with increasing the cluster size and velocity.     

用电子散射研究丰质子核的质子晕结构

理论和实验结果都表明¹⁷F的第一激发态有质子晕存在.用相对论平均场理论和Eikonal近似研究了质子晕核¹⁷F的第一激发态的电子弹性散射过程. 计算了¹⁷F的第一激发态的电荷形状因子,并与¹⁶O和¹⁹F的结果进行了对比和讨论.结果显示质子晕的存在会使中等转移动量的电荷形状因子产生明显的变化,并且使低转移动量的电荷形状因子趋于降低.这说明电子散射对质子晕的存在是非常敏感的,表明可以用电子散射对奇特核的质子晕结构进行更精细的研究.     

NaK(61Σ+)与H2碰撞传能中的H2的振转态分布

光学-光学双共振激发NaK至61Σ+高位电子态,研究了NaK(61Σ+)与H₂的电子-振转能量转移。利用相干反斯托克斯拉曼散射(CARS)光谱技术检测H₂的振转态分布。扫描CARS谱表明H₂在(1,1),(2,1),(2,2),(2,3),(3,1),(3,2),(3,3)和(3,5)振转能级上有布居。对于(3,1), (3,2), (3,3)和(3,5)能级,扫描CARS谱峰值直接给出布居数之比。对于(1,1), (2,1), (2,2)和(2,3)能级,扫描CARS谱峰值给出二个可能的布居数之比,利用一个速率方程组,由时间分辨CARS轮廓可以得到真实的比值。用n₁～n₈分别表示H₂的(3,1), (2,1), (1,1), (3,3), (2,3), (2,2), (3,2)和(3,5)能级上布居密度,得到n₂/n₁～n₈/n₁分别为0.51,0.97,0.45,0.18,0.10,0.26和0.31。利用Stern-Volmer公式,得到61Σ+态的总退布速率系数为(2.1±0.4)×10-10 cm3s-1, 由H₂各振转能级布居数之比,得到61Σ+-(1,1), (2,1), (2,2), (2,3), (3,1), (3,2), (3,3)和(3,5)转移速率系数(10-11 cm3·s-1单位)分别为5.4±1.6,2.8±0.8,0.6±0.2,1.0±0.3,5.6±1.7,1.4±0.4,2.5±0.8和1.7±0.5。     

介质阻挡放电中单晶胞白眼斑图的光谱研究

在介质阻挡放电系统中,空气和氩气混合气体的实验条件下,第一次实现了只具有一个单元结构的白眼斑图。该斑图的结构从中心位置向外依次为：中心点,围绕中心点的环和环外六个点。由于出现该单晶胞白眼斑图时的电压较低,而本实验采用的水电极中的水的比热容大,具有良好的吸热性,这使斑图在放电过程中放电气隙间的气体的温度没有升高,并且放电现象没有发生变化。因此在实验过程中,单晶胞白眼斑图在长时间放电的情况下并没有使其等离子体状态发生改变。由普通照相机所拍摄的图片可以看到,单晶胞白眼斑图的中心点,围绕中心点的环和环外六个点的亮度有明显不同。在不同压强下该斑图的稳定性有所不同,并且中心点,围绕中心点的环和环外六个点的亮度随压强的变化有所不同。鉴于此,本实验采用了发射光谱法,研究了单晶胞白眼斑图中不同位置处(中心点、环及外围六个点)的等离子体温度随压强的变化关系。其中,分子振动温度使用氮分子第二正带系(C3Π_u→B3Π_g)的发射谱线来计算;电子激发温度利用氩原子763.26 nm(2P₆→1S₅)与772.13 nm(2P₂→1S₃)两条谱线强度值进行比较的方法进行研究;电子密度利用氩原子696.57 nm(2P₂→1S₅)谱线的展宽来测量。发现在同一实验条件下,单晶胞白眼斑图的中心点的电子激发温度、电子密度和分子振动温度均最低,环外六个点相应的电子激发温度、电子密度和分子振动温度次之,环相应的电子激发温度、电子密度和分子振动温度均最高;随着气体压强从40 kPa增大到60 kPa,单晶胞白眼斑图不同位置处的电子密度增高但分子振动温度和电子激发温度均降低。本实验结果有助于进一步研究自组织斑图形成的机制。