25MeV／u^6He十^9Be破裂反应的α碎片发射

测量了在25MeV／u^6He轰击^9Be靶的破裂反应产生的α碎片双微分截面及角分布，并在Ser—ber模型的框架下计算了在破裂反应中衍射破裂与擦去过程的贡献，并对结果进行了讨论．结果表明基于包含衍射破裂和擦去过程的Serber模型可以对^6He的直接反应进行较好地描述，擦去过程的贡献远大于衍射破裂的贡献．相对于^6Li而言，^6He较大的去2n微分截面源于它的弱束缚特性。     

Polar Interface Optical Phonon Modes and Froehlich Electron－Phonon Interaction Hamiltonians in an Arbitrary Layer－Number Quantum Well System

By using determinant method as in our recent work, the IO phonon modes, the orthogonal relation for polarization vector, electron-IO phonon F~6hlich interaction Hamiltonian, the dispersion relation, and the electron-phonon coupling function in an arbitrary layer-number quantum well system have been derived and investigated within the framework of dielectric continuum approximation. Numerical calculation on seven-layer AlxGal-xAs/GaAs systems have been performed. Via the numerical results in this work and previous works, the general characters of the IO phonon modes in an n-layer coupling quantum well system were concluded and summarized. This work can be regarded as a generalization of previous works on IO phonon modes in some fLxed layer-number quantum well systems, and it provides a uniform method to investittate the effects of IO phonons on the multi-layer coupling quantum well systems.     

Structures of（ΩΩ）0＋and（[1]Ω）1＋in Extended Chiral SU（3） Quark Model

The structures of (ΩΩ)0 and ([1]Ω)1 are studied in the extended chiral SU(3) quark model in which vector meson exchanges are included. The effect from the vector meson fields is very similar to that from the one-gluon exchange (OGE) interaction. Both in the chiral SU(3) quark model and in the extended chiral SU(3) quark model,di-omega (ΩΩ)0 is always deeply bound, with over one hundred MeV binding energy, and ([1]Ω)1 ‘s binding energy is around 20 MeV. An analysis shows that the quark exchange effect plays a very important role for making di-omega (ΩΩ)0 deeply bound.     

Ground-State Properties ,of C, O, and Ne Isotopes in Hartree——Fock-Bogoliubov Calculation with Gogny Interaction

Ground-state properties of C, O, and Ne isotopes are described in the framework of Hartree-Fock-Bogoliubov theory with density-dependent finite-range Gogny interaction D1S. We include all the contributions to the Hartree-Fock and pairing feld arising from Gogny and Coulomb interaction as well as the center of mass correction in the numerical calcu/ations. These ground-state properties of C, O, and Ne isotopes are compared with available experimental results, Hartree-Fock plus BCS, shell model and relativistic Hartree--Bogoliubov calculations. The agreement between experiments and our theoretical results is pretty well. The predicted drip-line is dependent strongly on the model and effective interaction due to their sensitivity to various theoretical details. The calculations predict no evidence for halo structure predicted for C,O, and Ne isotopes in a previous RHB study.     

溶液中CO…CO+体系相互作用的理论研究

在B3LYP/6-311+G水平上利用SCRF方法中的Onsager model模型考察了CO…CO+体系在两种介质(水和苯)中可能存在的相互作用复合物,发现由于H2O与CO+之间存在较强的相互作用,在水中仅能存在一种稳定结构,而在苯溶液中存在三种稳定的复合物.通过消除基函数引起的叠加误差(BSSE)和零点振动能(ZPVE)的校正,精确求算出三种复合物在两种介质中的相互作用能,表明溶剂的性质对复合物的稳定性有着重要的影响.     

多组态Dirac-Fock方法与准相对论组态相互作用方法的比较研究

利用多组态Dirac-Fock(MCDF)方法与准相对论组态相互作用方法,分别详细计算了低Z、中Z和高Z原子(离子)各个壳层上电子的束缚能、平均轨道半径、总束缚能、激发能、精细结构能级以及类Ne等电子系列离子的2p53s 1,3P1-2p6 1S0跃迁能,并且对这两种方法的结果进行了数值比较.     

与运动原子相互作用的场的压缩效应

采用量子光学中时间演化算符方法，研究了与运动原子相互作用的场的压缩效应，揭示了光场的初始平均光子数和场模结构参数对光场压缩特性的影响，结果表明：适当选择系统参数，可获得在时间上持续压缩的压缩光。     

利用V型原子与单模光场的非共振相互作用制备四光子相干态

提出了一种利用简并V型三能级原子与振幅很大的单模相干光场的远离共振相互作用,制备四光子相干态的有效新方案.同时证明了在相同的条件下,按照相同的方法不能制备出四成分以上的相干态的叠加态, 即当在腔中注入的第三个原子的速度与第二个原子的速度相等时,腔场将保持这种四光子相干态不变.     

HL-1M装置等离子体与ICRH发射天线的相互作用

ICRH实验的一个比较突出的问题就是杂质。杂质的产生与ICRH发射天线同等离子体的相互作用和RF脉冲的发射有着不可忽视的联系。对HL－1M装置的ICRH发射天线在两年多实验中的变化作了简要的介绍和讨论，并对今后ICRH发射天线的设计提出了一些建议。     

甘氨酸与水分子间相互作用的理论研究

在密度泛函(DFT)B3LYP/6_311++G(3d,3p)水平,对中性甘氨酸的最小点结构Ip和H2O分子间可能存在的氢键复合物进行全自由度能量梯度优化,发现了三个氢键极小结构A、C和E,其中结构A为最稳定结构,它是H2O与甘氨酸的羧基(-COOH)形成两个氢键的结构,具有C1对称性.分别采用密度泛函理论(DFT)和MP2方法,在6-311++G(3d,3p)水平,对结构A的结构和结合能进行了比较计算,得到结合能ΔEDFT为-41.88 kJ/mol,ΔEMP2为-40.34 kJ/mol.