Dirac Optical Potential of p-^14Be and Pronounced “Long-Tail” Shape

The Dirac optical potential for p-^14 Be elastic scattering is evaluated by the relativistic impulse approximation. Each of the real part and the imaginary part of the potential shows a pronounced “long tail” for the proton elastic scattering from halo nucleus ^14Be compared with the potentials for proton scattering from its adjacent nuclei ^12C and ^16O, which do not have halo structures.This kind of “long tail” phenomenon suggests another signature for halo nuclei.     

浮栅ROM器件辐射效应机理分析

分析了浮栅ROM器件的辐射效应机理，合理地解释了实验中观察到的现象.指出辐射产生的电子空穴对在器件中形成的氧化物陷阱电荷和界面陷阱电荷是导致存储单元及其外围电路出现错误的原因.浮栅ROM器件的中子、质子和⁶⁰Co γ辐射效应都是总剂量效应 . 关键词： FLASH ROM EEPROM 中子 质子 60Co γ')" href="#">⁶⁰Co γ 总剂量效应     

半导体带电粒子探测器的研制及其在空间物理中的应用

阐述了空间辐射环境监测的意义,描述了半导体带电粒子探测器的研制及由其组成的望远镜系统在空间物理中的应用,并给出了用此探测器在卫星上进行地球辐射环境监测、太阳质子事件和地磁暴探测的部分结果.     

14β-甲磺酰氧基对映-贝壳杉二萜重排反应

本文研究了一类具有15-C与16-C单键的14β-甲磺酰氧基对映-贝壳杉烷(烯)(6,7和8)在Zn-EtOH体系中的重排反应, 它们均能重排成6, 7, 5, 5并环系统的化合物3, 12, 13a和13b。8重排时生成一个8-OEt化合物, 为这类化合物重排时经过阳离子中间体提供了一个证据。     

e-A深度非弹性散射中胶子辐射振幅的新计算方法

在e-A深度非弹性散射过程中, 喷注穿过冷核介质时, 多重散射诱导胶子辐射会导致对碎裂函数的修正及喷注的能量损失.前期研究中关于计算e-A深度非弹性散射中胶子辐射振幅的两种方法: 螺旋振幅近似和微扰QCD严格计算都异常繁杂. 本文发展了一种新的方法, 可以方便计算出多重散射导致胶子辐射的振幅, 得到的碎裂函数的修正以及能量损失与严格计算的结果一致.     

He原子与HF分子碰撞截面的量子力学计算

用量子力学密耦近似方法计算了入射氦原子能量E=88?meV时,He-HF碰撞,弹性散射分波截面(00-00)和非弹性散射00-01及00-02分波截面.计算结果与公认较好的Moszynski等人的SAPT势比较接近.     

质子和中子有“远亲”了

美国能源部费米国家加速器实验室国际费米碰撞探测器（CDF）合作组的科学家23日说，他们利用Tevatron对撞机，成功地发现了两种罕见的粒子．经过鉴定，这两种粒子是最常见的质子和中子的“远亲”．     

New Levels in ^118Pd Observed in the β Decay of Very Neutron-Rich ^118Rh Isotope

We investigate the β decay of very neutron-rich ^118Rh isotope using on-line mass-separated sources which are produced by applying 25 MeV proton induced symmetric fission of natural uranium at the IGISOL facility. The β-γ and γ-γ coincidence spectroscopy is employed to establish the level scheme of daughter nucleus ^118Pd. Five low-lying new levels are identified for the first time with tentative spin and parity assignments based on the even-mass Pd systematics.     

Proton Fraction in Neutron Star Matter and Three-Body Force Effects

The three-body force effects on the equation of state and its iso-spin dependence of asymmetric nuclear matter and on the proton fraction in neutron star matter have been investigated[1] within Brueckner Hartree-Fock (BHF) approach by using a microscopic three-body force. It is shown that, even in the presence of the three-body force, the empirical parabolic law of the energy per nucleon vs. isospin asymmetry β=(N-Z)/A is fulfilled in the whole asymmetry range 0 ≤β ≤1 and also up to high density. The three-body force provides a strong enhancement of symmetry energy at high density in agreement with relativistic approaches. Thecalculated proton fraction in β stable neutron star matter is given in Fig.l, where the thick solid line is the BHF prediction using AV18 TBF, while the dotted one is the BHF result using AVis. The thin solid line is the prediction of the Dirac-Brueckner approach taken from Ref.[2]. The results extracted according to the phenomenological paramete rizations of the symmetry energy suggested in Ref.[3] are also plotted. It is seen from     

詹特切克生平简介

 威利鲍德·詹特切克(WillibaldJentschke),是位于汉堡附近的德国粒子物理实验室DESY的创立者,欧洲核研究组织(CERN)的前负责人,他过完90岁生日之后,于2002年3月11日逝世。詹特切克1911年生于维也纳,24岁获得核物理学博士学位,他在维也纳一直工作到1951年,然后他到了伊利诺斯州的恩巴拉大学,任回旋加速器实验室的负责人。1955年,当汉堡大学让詹特切克负责实验物理学研究时,他申请基金在德国建立现代的核物理研究设施。