碎裂反应和放射性核束的产生

本总结了中能重离子碰撞产生同位素分布的计算方法和模型,包括参数化公式,擦碎模型和统计擦碎模型。介绍了模型的物理基础和计算方法,并讨论了对擦碎模型和统计擦碎模型的修正。同时用统计擦碎模型探讨了碎裂瓜在产生的同位素分布的同位旋效应。然后介绍了放射性核束的产生方法,并对放射性束流物理的发展前景作了简要介绍。     

分形集的两种密度定义

给出了分形集的两种密度定义,讨论了它们的关系及性质。通过Ｖｉｔａｌｉ覆盖定理,证明了Ｈａｕｓｄｏｒｆｆ凸密度定理。     

基于DWT-SVD的数字水印嵌入方法

目前基于SVD的水印算法是直接对宿主图像或水印图像进行奇异值变换(SVD),然后将水印嵌入宿主图像的的奇异值中。本文提出了一种新的基于SVD-DWT的水印算法,先对宿主图像和水印图像进行小波变换(DWT),然后将水印嵌入各频带的奇异值中,并且水印嵌入系数随频带不同而不同。在JPEG压缩、图像旋转及剪切等攻击方式下,对该水印算法进行了鲁棒性分析,数值实验表明该水印算法具有良好的抗攻击性和安全性.     

三七总皂苷对家兔出血性坏死性肠炎的影响

探讨了三七总皂苷对家兔出血性坏死性肠炎的影响。将30只家兔随机分为对照组、内毒素组、三七总皂苷组。肠系膜动脉钳夹 浆膜下注射内毒素方法制作家兔出血性坏死性肠炎模型,分别于6、24h后取血,酶联免疫吸附(ELLSA)法测定IL-6、肿瘤坏死因子(TNF)水平。24h后处死家兔,观察肠管、肺的病理组织学改变。结果表明:三七总皂苷组与内毒素组相比,IL-6和TNF均较内毒素组有明显降低。三七总皂苷组肠管病理组织学损伤改变较内毒素组明显减轻。三七总皂苷通过抑制LPS产生炎症介质的作用,干预家兔MODS出血性坏死性肠炎的发生与发展。     

最大度较小的图的线性着色

本文研究了最大度较小的图的线性着色问题。通过分析未着色顶点的邻近顶点的着色情况,扩充图的部分线性着色,利用数学归纳法证明了△（G）≤4的非4正则图G的线性色数有lc（G）≤7和△（G）≤5的非5正则图G的线性色数有lc（G）≤13。     

20Mgβ衰变谱学与15O(α,γ)19Ne反应(英文)

15O（α,γ）19Ne（p,γ）20Na反应链是高温CNO循环向快速质子俘获过程突破的一条关键路径,相关的反应率输入量可通过20Mg的β衰变可布居19Ne共振态并测量其衰变性质来获得。通过高效率高精度地测量20Mg β衰变中产生的质子与γ射线得到了20Mg衰变的详细信息,并构建了完整的衰变纲图,还进行了19Ne 4 033 keV共振态衰变性质的探索,获得了该态在20Mg β衰变中被布居的分支比上限。通过比20Mg和20O镜像能级跃迁的结果确认了同位旋非对称性,为检验相关理论模型提供了精确的实验数据。对于突破路径中有重要影响的19Ne 4 033 keV共振态的性质,有待更高统计的实验进一步研究。The breakout from the hot CNO cycle to the rapid proton capture process can occur via the 15O(α,γ)19Ne(p,γ)20Na reaction sequence, and the β decay of 20Mg can be used as an alternative method to characterize some specific resonances, which will provide detailed nuclear structure input for reaction rate calculations. The reliable information on the decay properties and structure of 20Mg was obtained by measuring the emitted particles and γ-rays in the β decay with high efficiency and high resolution. Attempt was also made to search for the decay channels associated with the 4 033 keV resonance in 19Ne. To test fundamental symmetries, the transitions in the mirror decays of 20Mg and 20O were compared. The precise experimental data presented here would be important to constrain the theoretical calculations. It is desirable to clarify the astrophysically relevant problem by further experiments with improved statistics on the basis of the present work.     

叔丁氧基自由基引发氢迁移过程的理论研究

采用多种密度泛函理论方法(如CAM-B3LYP, M062x和wB97x方法), 并辅以极化连续介质模型对叔丁氧基自由基(^tBuO·)与一系列胺类、 烷烃、 醇类和醚类反应物之间氢迁移反应的反应机理进行研究. 计算结果表明, 这类氢迁移反应主要受熵的控制. 通过对液相平动熵和气相平动熵得到的活化自由能数据进行对比, 可以看出, 使用气相平动熵得出的活化自由能明显偏高于实验测量值, 而以液相平动熵计算的反应活化自由能垒与实际结果相近, 3种方法对胺类和烷烃类反应物体系得出的结果更可靠, 对醇类和醚类反应物体系自由能垒则略低.     

Impact parameter and beam energy dependence for azimuthal asymmetry of direct photons and free protons in intermediate energy heavy-ion collisions

Hard photon emitted from energetic heavy ion collisions is of very interesting since it does not experience the late-stage nuclear interaction, therefore it is useful to explore the early-stage information of matter phase. In this work, we have calculated the impact parameter and beam energy dependence for azimuthal asymmetry, characterized by directed transverse flow parameter F and elliptic asymmetry coeffcient v2, of direct photons and the corresponding free protons in intermediate energy heavy-ion collisions. It is further shown the anti-correlated azimuthal asymmetry between direct photons and free protons.     

Impact parameter and beam energy dependence for azimuthal asymmetry of direct photons and free protons in intermediate energy heavy-ion collisions

Hard photon emitted from energetic heavy ion collisions is of very interesting since it does not experience the late-stage nuclear interaction, therefore it is useful to explore the early-stage information of matter phase. In this work, we have calculated the impact parameter and beam energy dependence for azimuthal asymmetry, characterized by directed transverse flow parameter F and elliptic asymmetry coefficient v₂, of direct photons and the corresponding free protons in intermediate energy heavy-ion collisions. It is further shown the anti-correlated azimuthal asymmetry between direct photons and free protons.     

基于巨灾模型的巨灾保险组合研究

巨灾风险所造成的巨大损失已经威胁到人类社会的可持续发展.巨灾保险是分散巨灾损失的一种途径,利用巨灾模型研究被保风险的累积损失和个人损失分布的数学性质,且考虑损失率是巨灾强度的函数.通过巨灾模型和保险公司破产概率的计算和数值仿真,得到不能仅仅依靠保费的选择而分散巨灾风险.