中学数学教材中能否给出曲线渐近线定义

众所周知,现行中学数学教材中没有给出曲线的渐近线的定义.而事实上,从初中数学中学习反比例函数图象的知识起,已经涉及到曲线的渐近线这一概念.但就是到了《全日制普通高级中学教科书(必修)·数学》(第二册·上)中“圆锥曲线”部分,对双曲线的渐近线的定义也是描述性的(见上述     

中能区丰中子核反应总截面与中子过剩自由度的关系研究

发展了一个适用于计算中能区核反应总截面的修正微观模型,讨论了中子皮厚度,基态形变及与中子过剩自由度有关的核物质弥散度对核反应总截面的影响.计算结果和现有实验数据的比较表明,与中子过剩自由度有关的核物质弥散度是反应总截面随中子过剩增加而迅速增加的一个重要因素.     

Isospin Effects on Anisotropic Flows in Intermediate Energy Heavy Ion Collisions

Anisotropic flows per nucleon （v1/A, v2/A, v3/A and v4/A） of light fragments up to the mass number 4 as a function of transverse momentum per nucleon are studied for 55 Me V/nucleon 58Fe＋58Fe and 58 Ni＋ 58 Ni at large impact parameters by the isospin-dependent quantum molecular dynamics model. The effects of symmetry energy and nucleon-nucleon cross sections, which are both isospin-dependent on anisotropic flows, are studied in detail. In comparison of the two systems with or without symmetry potential term, the results show that the strength of flows is sensitive to symmetry potential and nucleon-nucleon cross sections, which mainly cause a repulsion effect in this energy region.     

寒冬中能否苏醒？

应该说相对于传统产业几乎崩盘的境地，处于高速发展的IT及消费电子产业面对经济危机时只是放绥了发展的步伐，快速的技术更迭、功能应用的创新、市场有序的竞争在这个行业从来就不匮乏     

X射线背景辐射谱佯谬的解释 *

宇宙X射线背景(CXB)谱佯谬是指分立X射线源(主要是活动星系核,AGNS)叠加的谱与CXB的观测谱不一致.采用68个AGNs中能X射线谱,统计分析出X射线谱指数的演化规律,并计算对CXB的贡献可达100%,特别是在2～10keV能段叠加的谱与CXB谱一致,解释了谱佯谬.     

中能重离子碰撞中横向流电荷依赖的形状以及实验条件对横向流的影响(英文)

从35 MeV/nucleon 40Ca+40Ca反应实验数据中提取了碎片Z从1到9的横向流,发现探测器阈值、探测系统的角分辨等实验条件对横向流电荷依赖的形状有显著的影响。在考虑实验条件并采用软的核物质状态方程（K=200 MeV）之后,CoMD模型计算结果很好地重现了实验中横向流电荷依赖的形状。这表明如果要更加精确地提取实验中的横向流,必须使用阈值更低、角分辨更好的探测系统。此外,结合Kohley等[Phys Rev C,2012,85:064605]从实验中提取的横向流,讨论了横向流电荷依赖的形状存在异同的原因。1 ≤ Z ≤ 6的横向流电荷依赖呈肩峰形状可能是实验条的影响引起的,而我们的实验中Z ≥ 6的横向流的减小可能是由于动量守恒对集体运动的抑制。The transverse flow in the reaction of 40Ca+40Ca at 35 MeV/nucleon has been determined for emitted isotopes with Z=1 to 9. A significant modification of the Z-dependent flow pattern caused by the experimental filters, the detector thresholds and the angular resolutions (△?) of the detector array, is observed. With the application of the appropriate experimental filters, the general trend of the experimental Z-dependent flow is well reproduced by the Constrained Molecular Dynamics (CoMD) simulation, employing an effective interaction corresponding to a soft EOS (K=200 MeV). This fact suggests that to determine the flow values more precisely, a detection system with lower energy threshold and better angular resolution is urgently required. Additionally, together with the parallel work of Z. Kohley et al.[Phys Rev C, 2012, 85:064605], the pattern of the experimental Z dependence of transverse flow is also discussed. The shoulder patterns of Z-dependent flow for 1 ≤ Z ≤ 6 can be attributed by the experimental filters, while the reduction of flow for Z ≥ 6 in our experiment can be caused by the suppression of collective motion under the momentum conservation.     

中能质子相对论光学势分析

本文采用一套普适的中能质子相对论唯象光学势定性地讨论了光学势参数对散射截面及自旋观察量的影响.分析表明,与低能情况不同,当核子能量大于300MeV时,散射总截面随能量变化很缓慢,位势的强度变化对总截面影响也较小,但散射角分布和自旋观察量不仅依赖于光学势的体积分,还依赖于光学势的强度和形状.文章还讨论了Walecka模型给出的相对论微观光学势在中能范围的适用程度.