缺中子130Pm和128Pr核的EC/β+衰变研究

171MeV³⁶Ar束轰击⁹⁶Ru靶由熔合蒸发反应生成了¹³⁰Pm和¹²⁸Pr核.由氦喷嘴快速带传输系统将反应产物送到低本底区.基于X-γ-t,γ-γ-t符合测量,首次建立了¹³⁰Pm的(EC+β⁺)衰变纲图.重新研究了¹²⁸Pr核的衰变,订正和补充了γ射线,建立了新的(EC+β⁺)衰变纲图.     

人工色荷电PG玻色子对B介子衰变中η′单举产率的增强

计算了人工色荷电PG玻色子π     

在J/ψ衰变中寻找新物理

北京谱仪(BES)已收集了2.5×10⁷个J/ψ事例,并计划增加到10⁸—10⁹个.本文综述近年来在BES上寻找新物理的研究,包括在J/ψ衰变过程中探测新的味改变中性流,CP破坏和轻子味破坏.     

RIBLL上的β+缓发粒子发射的在束测量

报道了在新建成的放射性次级束流线上完成的²⁰Na的β+缓发α粒子发射²⁰Na—→β^+　20Ne→¹⁶O+α的在束测量.通过飞行时间和能损符合的方法实现²⁰Na次级束流的在束鉴别与调制.在束和停束两个获取时段分别完成对次级束流和β+缓发粒子的记录.利用脉冲发生器和记数器实现²⁰Na缓发粒子衰变半衰期的测量.实验测量到²⁰Ne几个低能共振能级的衰变能量分别为2.69,3.09,4.74,5.54MeV,相对强度分别为100,4.15,1.10,15.20.测量到²⁰Na的β⁺缓发α衰变的半衰期为(459±7)ms,与现有的核数据基本上吻合.     

The Effects from the Complex Parameters on t→ch^0 Within the Minimal Supersymmetric Standard Model

We investigate the effects from complex parameters on the branching ratio (BR) of the flavor changing rare decay t→ch^0 contributed by the electroweak interactions in the framework of the minimal supersymmetric standard model with complex parameters. We study the dependence of the BR on the possible relevant additional parameter swhich could be the originalsources inducing CP-violation, i.e., the complex phase angles φμ and φAb in squark and chargino sectors and δ13 appearing in Cabibbo-Kobayashi-Maskawa matrix. We find that these parameters influence the BR obviously and the effects induced by φμ and φAb are much larger than by δ13. With the different chosen values of the complex parameters, the BR is in the range between 10^-10 and 10^-8, depending mainly on the phase angles of the higgsino mass parameter μ and the trilinear coupling Ab.     

ITER 试验包层模块活化计算与环境安全分析

运用聚变堆放射性计算程序FDKR 和衰变链数据库AFDC-DLIB, 计算了ITER 中国氦冷固态增殖试验包层模块设计中活化产物的放射性、衰变余热和潜在生物危害因子BHP 值。计算结果表明: 对于试验包层模块来说, 在500MW 聚变功率下运行一年, 停堆时的总放射性、余热和BHP 值分别为2. 10× 10¹⁶B_q 、5. 06 × 10^{- 3}MW 和 68. 6km³•( kW) ^{- 1}。结果表明: 中国氦冷实验包层模块不存在突出的安全问题。     

Magnetic Field Effect on β^＋ Decay in the Crusts of Accreting Neutron Stars

Based on shell model of nuclei, the influence of a high magnetic field on β^＋ decay in the crusts of accreting neutron stars is analyzed. The magnetic field effect on 54 Mn is discussed. The results show that a weak magnetic field makes little effect on β^＋ decay but a strong magnetic field （B 〉 10^11 G） improves β^＋ decay rates obviously. The conclusion derived will benefit to develop further research on nuclear astrophysics in the future.     

Radiative decay from doubly to singly excited states of He via generalization of Laguerre-type orbitals： A non-orthogonal formalism

By taking full account of the non-orthogonality of the orbitals between the low-lying doubly excited states ¹P^o and the singly excited states ¹S^e and ¹²D^e of He, the corresponding radiative decay rates have been investigated theoretically via analytic generalized Laguerre-type atomic orbitals at a nearly numerical multi-configuration self-consistent field accuracy in a general non-orthogonal configuration interaction scheme. From these rates, we calculate the VUV photon emission and metastable atom spectra, and both are found to be in good qualitative agreement with recent excellent measurements. We obtain, successfully, the enhancement of the VUV photon spectrum, experimentally observed at the energy of (2s4p-4s2p)/(2p,3d) ¹P^o as compared with other nearby lying states. The mechanism proposed by Odling-Smee et al is verified, implying that taking appropriate account of the overlap existing between orbitals of the low-lying doubly excited and singly excited states (especially important for the compact orbitals) can reveal basic physical dominant mechanism and is crucial in understanding these spectra.     

16O(α,γ)20Ne反应的实验研究

讨论了目前16O(α ,γ) 2 0 Ne反应的实验研究工作 ,并对2 0 Na β+—→2 0 N →16O +α的β+ 缓发衰变α能谱的相对强度值同文献进行了比较 ,讨论了低能激发能级、共振强度及其对共振截面的贡献、S因子的理论研究.The experimental investigations of 16 O(α,γ) 20 Ne reaction is reviewed. The energy spectrum of β + delay α decay were measured through the 20 Naβ +-→ 20 Ne *→ 16 O+α process, and the relative densities of α decays are compared with the reference s results. The low excitation energy levels, resonance strength and its contribution to the resonance crosses section are also discussed. Finally, we have calculated the reaction rate of the direct capture reaction.......     

基于智能检测不变像元的FY-3A/MERSI仪器响应衰变分析

提出一种智能方法来分析风云三号A星(FY-3A)中分辨率光谱成像仪(MERSI)的长期响应衰变。该方法通过使用迭代加权多元变化检测(IR-MAD)算法识别同一区域、不同时相卫星图像的不变像元,基于这些不变像元的信号变化评估仪器在该时段的响应衰变。先用IR-MAD方法分析图像场景的不变像元,通过两幅图像不变像元的正交回归获取仪器的相对衰变;再对多个图像对的长时间序列进行分析,采用多项式拟合获得传感器衰变随时间的变化曲线。采用所提方法研究了FY-3A/MERSI北非地区和中国西北部地区的数据,并与其他相关研究得到的仪器衰变结果进行比较。结果显示,所提方法与其他方法获取的仪器衰减规律具有良好的一致性(差异在2%以内),而且从北非地区与中国西北地区得到的结果相吻合(大部分通道的差异在1%以内),验证了本文方法的通用性与可重复性。