基于Schrdinger方程的耦合常数解析延拓方法

基于Schrdinger方程,利用耦合常数解析延拓方法研究了球对称的方势阱、Woods-Saxon势和谐振子势中的单粒子共振态的能量与宽度.分析了耦合常数的取值区间和Pade多项式阶数对计算结果的影响.结果发现,在适当的耦合常数取值范围内,随着Pade多项式阶数的增加可以得到稳定和收剑的单粒子共振态能量与宽度.     

BCK-代数中理想和对偶理想的运算∧和∨

若X是有界关联BCK-代数,≤是集的包含关系,则X的所有理想之集关于V和在序关系≤下是一个分配格,最小元为{O},最大元为X,所有主理想的集是它的一个子格, 关于对偶理想有类似结果。 利用上述结果证明了下列关系     

三轴形状原子核存在的可能证据

本文证明三轴形状(非轴对称形状)原子核两类转动惯量之间的关系不同于轴对称原子核的。作者对稀土区和锕系区近八十个偶偶核的能谱作了分析比较,结果支持了上述结论,从而说明三轴形状原子核可能具有的特征。本文以五个核为例加以说明。     

近窥切尔诺贝利隐藏的辐射“热点”

<正>由于切尔诺贝利仍然是地球上放射性污染最严重的地区之一,获得进入许可并不容易。研究人员花了四个月的时间获得使用无人机的安全许可,以及在工作期间需要佩戴的辐射剂量测量胶片徽章。2019年4月,英国布里斯托大学教授汤姆·斯科特(Tom Scott)和研究助理彼得·马丁(Peter Martin)等人乘着载有各种辐射探测器、无人机和防护设备的小型巴士,在向导引领下进入     

原子核层次的手征对称性

对称性及其破缺是基本的科学问题。手征对称性在自然界中广泛存在,大至星系旋臂、行星自转,小到矿物晶体、有机分子、基本粒子,都与手征对称性密切相关。原子核层次的手征对称性概念于1997年提出,随后成为核物理研究的热点问题。目前,实验上已经在核素图上的80,100,130和190质量核区发现了30多例可能具有手征对称性的原子核。简要介绍原子核中的手征对称性概念;手性原子核的预言、识别以及实验验证;并通过展示手性原子核结构的多样性（M_χD）,回顾了理论和实验研究进展;介绍最新发现的原子核中手性和空间反射对称性的联立自发破缺,对未来手性原子核研究的前景进行了展望。Symmetry and its breaking are basic scientific problems. Chiral symmetries are common in nature, for example, the macroscopic spiral arms of galaxies and the rotation of planets; the microscopic spirals of the mineral crystalline, the organic molecules and the elementary particles. The concept of chirality in atomic nuclei was first proposed in 1997. Since then many efforts have been made to understand chiral symmetry and its spontaneous breaking in atomic nuclei. Up to now, more than 30 candidates of chiral nuclei have been reported in the 80, 100, 130, and 190 mass regions. The concept of the chirality in atomic nuclei, the prediction, the signal, and the experimental verification of the chiral nuclei are briefly introduced; the recent theoretical and experimental progress are reviewed, in particular the existence of multiple chiral doublets (M_χD), i.e., more than one pair of chiral doublet bands in one single nucleus; the simultaneous spontaneous breaking of chiral and reflection symmetry in the newly observed atomic nuclei is introduced, together with a prospect on the future study on nuclear chiral symmetry.     

Shears mechanism in two-dimensional cranking relativistic mean field approach

Using the new two-dimensional cranking relativistic mean field (RMF) approach, the shears mechanism of magnetic rotation based on configuration πh²_11/2⊙νh^－2_11/2 in ¹⁴²Gd is microscopically and self-consistently examined by investigating the aligning angular momenta of the valence nucleons.     

Neutron star equation of state in density dependent relativistic Hartree-Fock theory

The equation of state of neutron stars is studied in the newly developed density dependent relativistic Hartree-Fock (DDRHF) theory with the effective interaction PKO1 and applied to describe the properties of neutron stars. The results are compared with the recent observational data of compact stars and those calculated with the relativistic mean field (RMF) effective interactions. The maximum mass of neutron stars calculated with PKO1 is about 2.45 M_⊙, which consists with high pulsar mass from PSR B1516+02B recently reported. The influence of Fock terms on the cooling of neutron stars is discussed as well.     

Structure change of 156Yb at high-spin states

High-spin states of ¹⁵⁶Yb have been studied via the ¹⁴⁴Sm(¹⁶O,4n)¹⁵⁶Yb fusion-evaporation reaction at beam energy 102~MeV. The positive-parity yrast band and negative-parity cascade have been extended up to higher-spin states, respectively. The characteristics of the negative-parity sequence above the 25^－ state may related to the excitation from the nucleon in the Z=64, N=82 core. The E-GOS curve for the positive-parity yrast sequence in ¹⁵⁶Yb indicate that this nucleus may undergo an evolution from quasivibrational to quasirotational structure with increasing angular momentum. The Cranked Woods-Saxon-Strutinsky calculations by means of Total-Routhian-Surface (TRS) methods has been made to understand this structure change.     

辐照与食品

虽然有人在担忧辐照食品的安全问题,但尚无研究表明能有效杀灭病原体的辐射剂量会对人类的身体健康产生危害．     

WLW原子核质量模型在γ过程研究中的应用

本工作利用最近提出的WLW宏观-微观原子核质量模型,在经典r过程框架下很好地描述了太阳系r过程核素丰度分布.与常用的FRDM质量模型相比,新计算更好地再现了A≈135和A≈180质量区的太阳系r过程核素丰度,尤其避免了其他相似计算中A=135附近出现的与观测不符的丰度峰问题.分析表明,这种差异可能暗示WLW更为合理地处理了壳结构和对称能.