利用同质异位素产额比提取对称能的近似方法

在修改的Fisher模型框架下, 利用同质异位素产额比和结合能方程中对称能系数与温度比率的关联, 可以提取对称能系数与温度的比值。 利用3种不同的近似方法得到了重离子核反应产生丰中子余核的对称能系数与温度比（a_sym/T）,并研究了相关物理量对a_sym/T的影响。结果表明, 库仑能对提取丰中子余核的a_sym/T影响较小,且参考核的选取对a_sym/T的提取也有一定的影响。 In the framework of the modified Fisher model, correlations between the symmetry energy coefficient in semi classical mass formula to temperature (a_sym/T) and the isobaric yield ratio in Heavy ion collisions are established. a_sym/Tof neutron rich fragments are extracted using these correlations. It is found that the Coulomb energy term has little effect on a_sym/T of fragments, while the reference isobars adopted have great influence on the extracted a sym/T of fragments.     

Extraction of Nuclear Matter Properties from Nuclear Masses by a Model of Equation of State

The extraction of nuclear matter properties from measured nuclear masses is investigated in the energy density functional formalism of nuclei.It is shown that the volume energy a1 and the nuclear incompressibility Ko depend essentially on μ_nN + μ_pZ - 2E_N,whereas the symmetry energy J and the density symmetry coefficient L as well as symmetry incompressibility Ks depend essentially on μ_n - μ_p,where μ_p ＝μp - ∂E_c/∂Z,μ_n and μ_p are the neutron and proton chemical potentials respectively,E_N the nuclear energy,and E_c the Coulomb energy.The obtained symmetry energy is J ＝ 28.5 MeV,while other coefficients are uncertain within ranges depending on the model of nuclear equation of state.     

Evidence for a smooth onset of deformation in the neutron-rich Kr isotopes

The neutron-rich nuclei 94,96Kr were studied via projectile Coulomb excitation at the REX-ISOLDE facility at CERN. Level energies of the first excited 2(+) states and their absolute E2 transition strengths to the ground state are determined and discussed in the context of the E(2(1)(+)) and B(E2;2(1)(+)→0(1)(+)) systematics of the krypton chain. Contrary to previously published results no sudden onset of deformation is observed. This experimental result is supported by a new proton-neutron interacting boson model calculation based on the constrained Hartree-Fock-Bogoliubov approach using the microscopic Gogny-D1M energy density functional.     

Re-visit N/Z Ratio of Free Nucleons from Collisions of Neutron-Rich Nuclei as a Probe of EoS of Asymmetric Nuclear Matter

The N/Z ratio of free nucleons from collisions of neutron-rich nuclei as a function of their momentum is studied by means of isospin-dependent Quantum Molecular Dynamics. We find that this ratio is not only sensitive to the form of the density dependence of the symmetry potential energy but also its strength determined by the symmetry energy coefficient. The uncertainties about the symmetry energy coefficient influence the accuracy of probing the density dependence of the symmetry energy by means of the N/Z ratio of free nucleons of neutron-rich nuclei.     

Coulomb excitation of 68,70Cu: first use of postaccelerated isomeric beams

We report on the first low-energy Coulomb excitation measurements with radioactive Ipi=6- beams of odd-odd nuclei 68,70Cu. The beams were produced at ISOLDE, CERN and were post-accelerated by REX-ISOLDE to 2.83 MeV/nucleon. Gamma rays were detected with the MINIBALL spectrometer. The 6- beam was used to study the multiplet of states (3-, 4-, 5-, 6-) arising from the pi2p3/2 nu 1g9/2 configuration. The 4- state of the multiplet was populated via Coulomb excitation and the B(E2;6--->4-) value was determined in both nuclei. The results obtained illustrate the fragile stability of the Z=28 shell and N=40 subshell closures. A comparison with large-scale shell-model calculations using the 56Ni core shows the importance of the proton excitations across the Z=28 shell gap to the understanding of the nuclear structure in the neutron-rich nuclei with N approximately 40.     

Doppler shift as a tool for studies of isobaric analog states of neutron-rich nuclei: application to 7He

We have developed a new technique to study exotic neutron-rich nuclei via their isobaric analog states (IAS). We populate high-isospin states in resonant reactions of radioactive ion beams with protons. Characteristic gamma rays emitted from excited decay products were used to identify the population of the IAS. We show that information on the differential and total cross section for formation of the IAS can be extracted from the energy spectrum of the Doppler-shifted gamma rays. This technique was applied to the study of T=3/2 states in 7Li, which are analogs of states in 7He. The analog of the 7He ground state was clearly observed, whereas the presence of the analog of a narrow 1/2(-) state at 0.6 MeV excitation in 7He reported by M. Meister et al. [Phys. Rev. Lett. 88, 102501 (2002)] was excluded at the 90% confidence level. Evidence is presented for a broad 1/2(-) state at a higher excitation energy in 7He.     

The Friction and Diffusion Coefficients with Maxwellian Scatters

The Fokker-Planck coefficients for Coulomb interaction, or the friction coefficient (Δυ_α) (the average change in velocity) and the diffusion coefficient (Δυ_αΔυ_α), are evaluated by an appropriate variable change technique. This approach reduces the five-fold integral expressions of the Fokker-Planck coefficients to one-fold integral without meeting the divergence difficulties. A new Debye cutoff parameter Δυ_αmin, instead of the customary θ_min cutoff avoids the error incurred through the customary neglecting of velocity dependence of the Coulomb logarithm. The dominant terms of the new results are similar to Chandrasekhar's results. A non-dominant term, which can exceed the dominant one in the case of υ_α² > υ_βt²lnA is added for (Δυ_α||²).     

丰中子锰同位素的壳模型计算

利用球形壳模型和投影壳模型两种方法对Z≤28,N=40附近pf壳的丰中子核素的结构进行了一系列的研究。以丰中子的锰同位素为例讨论了对奇奇核58,60Mn的两种壳模型计算结果。结果显示,两种理论方法都很好地再现了58,60Mn实验上观测到的从低激发到高自旋态的能级。在对这两个同位素由中子g_9/2轨道闯入所产生的负宇称转动带进行描述时,两种理论计算也得到了一致的结果。通过对比,阐明了两种壳模型方法及其采用的有效相互作用在该丰中子核区的适用性,特别强调了中子g_9/2轨道的激发对于pf壳Z≤28丰中子核素结构的重要性。Recently,we have carried out a series of studies on the structures of pf shell neutron-rich nuclei around N=40 using the spherical shell model and the projected shell model respectively.As an example,these two types of shell model calculations for the neutron-rich odd-odd isotopes 58,60Mn are discussed in this paper.The results show that both the calculations reproduce the observed experimental energy levels from the lowexcitation states to the high-spin ones in 58,60Mn.Consistent results are also obtained by these two theoretical calculations when describing the negative-parity rotational band derived from the intruder neutron g_9/2 orbital in both isotopes.Through comparison,we show the applicability of these two shell model methods and the adopted effective interactions in the present neutron-rich mass region.The significance of the excitations from neutron g_9/2 orbital to the structures of the neutron-rich nuclei in pf shell with Z≤28 are especially emphasized in this paper.     

多铁材料HoMnO3中光学吸收和畸变驱动的第一性原理研究

六角钙钛矿结构锰氧化物HoMnO₃磁电效应的研究近年来已成为多铁性材料研究中极其重要的一个方面. 本文基于广义梯度近似下的密度泛函理论, 考虑电子自旋的非共线磁性结构, 计算研究了 d电子在位库仑作用和自旋-轨道耦合作用对HoMnO₃的电子结构、 轨道杂化和能态密度分布的影响. 结果显示, 当考虑在位库仑排斥势U作用时, 强烈的Ho 5d与O(3, 4) 2p以及Mn 3d与O(1, 2) 2p间的轨道杂化是驱动HoMnO₃发生铁电畸变的根源, 此时能隙和能带的分布为解释实验中发现的强烈的光学吸收峰提供了理论依据, 而自旋-轨道耦合使得Mn 3d-O(3, 4) 2p在 ab平面内的轨道交迭略有增强, 平面内部分能带简并消除, HoMnO₃材料呈现典型的间接性能隙绝缘体特征. 关键词： 磁电效应 铁电畸变 态密度 光学吸收     

THE CONVERSION OF GLUONS INTO QUARKS AND THE MULTIQUARK STATES

The rate for the conversion of the gluon into a color octet quark pair which subsequently forms a multiquark state with another quark pair or a gluon is discussed. The static potential in a [(QQ)₈(qq)_8,1] state where Q=c,b and q=u, d is studied in the MIT bag model. It is shown that the repulsive Coulomb force between Q and Q is dominant at small QQ separations, which would significantly suppress the QQ wave function at the origin. For the charm quark (Q=c) the ratio of |Ψ(O)|² for the ordinary (QQ)₁ to that for the(QQ)₈ in the [(QQ)₈(qq)_8,1] state is estinated to be 2-5. Therefore the assumption |Ψ₈(O)|²=|Ψ₁(O)|² would lead to an overestimation for the rate of g*→QQ and it is necessary to take the suppression effect of the repulsive Coulomb force into consideration.     

RADIATIVE DECAYS OF CHAKMONIUM AND CONSTITUENT QUARK MASSES

The problems of both El and M1 transitions of charmonium are discussed in the nonrelativistic potential model. It is found that these problems could be resolved by assuming larger constituent quark masses. With m_c=2.50GeV, m_b=5.84GeV in the typical linear plus Coulomb potential model we get satisfactory results for the mass spectra, the El and M1 transition rates, and the relative values of leptonic widths for the ψ and T families. The implication of the large constituent quark masses is also discussed.     

Cs(6P)+(Ne,N2)碰撞能量转移

在气体样品池条件下,研究了Cs(6P3/2) (Ne,N2)碰撞能量转移过程.用调频半导体激光器激发Cs原子至Cs(6P3/2)态,在不同的Ne或N2气压下,测量了直接6P3/2→6S1/2荧光和转移6P1/2→6S1/2荧光,对于6P3/2与Ne的碰撞,电子态能量仅能转移为Ne原子的平动能.在与N2的碰撞中,向分子振转态的转移是重要的.利用速率方程分析,可以得到碰撞转移速率系数,对于Ne,6PJ精细结构碰撞转移速率系数为1.45×10-12cm3·s-1.对于N2,测量6P Ne和6P N2二种情况下荧光的相对强度比,确定精细结构速率系数为1.64×10-12cm3·s-1,6P态猝灭速率系数为4.88×10-12cm3·s-1.     

典型伪装材料高光谱特征及识别方法研究

针对某些特定环境下,伪装目标和背景目标出现的“异物同谱”现象,传统的可见光及多光谱遥感伪装识别存在局限性,为此,将高光谱应用到典型伪装材料的特征分析与识别。以北方地区常用丛林迷彩伪装网为研究对象,利用SVC HR1024光谱仪获取其不同浸水时间的可见光-近红外光谱,通过光谱相似性度量和包络线去除处理,分析揭示不同浸水条件下伪装网和北方典型植被光谱特征和敏感波段,并基于近红外波段构建光谱比值指数RCI,用于识别绿色植被环境中的伪装目标,最后通过高光谱成像实验获取仿真伪装环境高光谱图像,并利用高光谱图像对识别效果进行验证。结果显示：(1)不同浸水时间的丛林迷彩伪装网的光谱曲线基本形态相似,且反射率随浸水时间的增加而整体呈下降趋势;1 900 nm波段是伪装网反射光谱对含水量响应最为明显的波段,其光谱特征会因浸水处理而相似于植被,相似度从0.895提高到了0.939。(2)丛林迷彩伪装网和植被在可见光波段的相似度较高,光谱波动情况相似,但在近红外波段光谱特征差异明显。通过包络线统去除分析得出970, 1 190和1 440 nm波段附近处是丛林迷彩伪装网识别的敏感波段,且基于迷彩伪装网和各植...     

SeOx(x=1,2)的从头算势能曲线和光谱常数

采用从头算的多种方法和基组优化计算SeO_x(x=1,2)自由基的基态结构、谐振频率及离解能,优选出QCISD(T)/6-311+G(2df)、B3LYP/6-311G(3d2f)方法分别对SeO、SeO₂自由基进行计算,计算结果与实验结果吻合很好.对SeO自由基拟合出Murrell-Sorbie势能函数参数,计算出SeO自由基的光谱常数和力常数.计算出SeO₂自由基力常数,导出SeO₂自由基的多体展式势能函数,发现SeO₂自由基对称伸缩振动势能图中在对称的O+SeO→SeO₂反应通道上有一鞍点,其活化能约为48.24 kJ·mol^-1,O原子需要越过0.5 eV的能垒才能生成SeO₂的稳定结构.     

A POSSIBLE SOLITON-LIKE POLARON MODEL FOR SUPERCONDUCTORS Y1-xCaxBa2Cu3-xMxO7-δ(M=Fe,Ni)

Using 1+1 soliton-like polaron model of a deformable continuum, the critical temperature and the energy gap in high-temperature superconductors Y_1-xCa_xBa₂Cu_3-xM_xO_7-δ(M=Fe,Ni) are studied in the framework of finite temperature Green's function theory. The ratio 2Δ/k_BT_c=3.9 is obtained. Theoretical results are found in good agreement with the experimental data.     

聚合物分子与官能化纳米管相互作用及扩散特性的分子动力学模拟

用全原子分子动力学方法研究典型聚合物分子（PE,PEO和PP）与碳纳米管（CNT）及官能化碳纳米管（FCNT）界面的相互作用及扩散特性.动力学模拟显示：—CH₃官能团具有减弱CNT与PE和PP的相互作用,但是,—CH₃官能化后的CNT与PEO之间确有增强作用.分析含氧官能团（—OH和—COOH）官能化的CNT与PE,PEO和PP的相互作用,可知含氧官能团的确具有增强表面相互作用的功能,而且含氧原子越多,相互作用就越强.此外,—CH₃,—OH,—COOH官能化后的CNT与PE,PP和PEO体系的总能量均减少,而且能量满足—COOH < —OH < —CH₃.分析非键相互作用势（库仑能和范德瓦尔斯能）,可知库伦相互作用是增强界面相互作用的主要作用能.官能化后的CNT/PE,CNT/PEO,CNT/PP体系的扩散系数都明显减小,且扩散系数大小满足—COOH < —OH < —CH₃.     

铜原子单激发态3d104p 2P1/2的光电离(英文)

铜原子能级结构的理论计算具有非常大的挑战性。本文基于多组态Dirac-Hartree-Fock（MCDHF）方法和相对论组态相互作用（RCI）方法,通过三个大规模的关联模型计算了单激发态3d104p 2P_1/2、双激发态3d94s（3D）5s4D_3/2,1/2,3d94s（3D）5s 2D_3/2,3d94s（1D）5s 2D_3/2以及离子态3d10 1S₀能级和波函数。结果表明,铜原子能级结构对有限组态空间的选择极其敏感,双激发态3d94s（3D）5s 4D_3/2,1/2,3d94s（3D）5s 2D_3/2,3d94s（1D）5s 2D_3/2和离子态3d10 1S₀与单激发态之间的能量差相对于已有实验结果均存在大约-0.4 eV的偏差,而计算得到的共振电子能量与实验结果符合得较好。此外,根据辐射跃迁矩阵元和非辐射跃迁矩阵元计算了双激发态的Fano参数q,并基于Fano理论得到了铜单激发态3d104p 2P_1/2的总光电离截面,该理论考虑了直接光电离与光激发自电离之间的干涉效应,即共振3d94s（3D）5s 4D_3/2,1/2、3d94s（3D）5s 2D_3/2和3d94s（1D）5s 2D_3/2具有明显的非对称的Fano轮廓,表明光电离过程与光激发自电离过程之间的干涉对双激发态共振附近的光电离截面轮廓有着极其重要的影响。     

The Fermi matrix elements inferred from β-γ(CP) correlation measurements in Fe decay

Measurements have been made of the β-γ circular-polarization correlation paramter A for the 273 keV β-branch in the decay of ⁵⁹Fe. It has recently been established that each of the principal β-branches of ⁵⁹Fe involves ΔJ=0 and thus has a possible non-zero Fermi matrix element M_F which can be determined from the ƒt value and A. Previous β-γ (_CP) measurements on this nucleide have all employed the usual γ-ray scattering technique. This method is suitable for the 475 keV β-branch but does not produce an accurate measurement of the lower energy branch because of energy discrimination difficulties. A transmission polarimeter with γ-discrimination has been used in the present work to obtain clean data on the 273 keV β-1.29 MeV γ-cascade. Calibration with ⁶⁰Co (1.33 MeV) and ²⁸Al (1.79 MeV) yielded A = −0.154±0.023. This gives for the isospin impurity coefficient and the effective Coulomb matrix element of the 1.29 MeV state (1.1±1.4) × 10⁻³ and 9±11 keV, respectively.     

0(+)(gs) --> 2(+)(1) excitations in the mirror nuclei 32Ar and 32Si

We measured the strength of the 0(+)(gs)-->2(+)(1) excitations in the radioactive mirror nuclei 32Ar and 32Si using the techniques of intermediate-energy Coulomb excitation for 32Ar and inelastic proton scattering in inverse kinematics for 32Si. The 32Ar measurement, taken together with previously existing Coulomb excitation data for 32Si, yields the isoscalar and isovector multipole matrix elements for the 0(+)(1)-->2(+)(1) transition between T = 2 states in the A = 32 system. The proton scattering measurement for 32Si, when combined with the Coulomb excitation data for this nucleus, yields a ratio of neutron and proton matrix elements, M(n)/M(p), for 32Si.