高斯骨架差分进化算法与回声状态网络的结合应用

针对回声状态网络(ESN)对于不同时间序列的学习上无法有效地确定储备池参数的问题,提出一种新型预测模型。利用改进的高斯骨架差分进化算法(DE)来优化回声状态网络。在DE算法中引入了变异策略选择因子,并将选择因子随个体共同参与进化,使每个个体执行当前最适合的变异策略。改善了原始DE算法进化过程中的盲目性,同时选择因子的动态自适应特性保持了骨架算法近似无参数的优点,最后为避免算法早熟加入停滞扰动策略改善算法的寻优性能。为验证模型的有效性,对Mackey-Glass时间序列、赣州月平均气温数据集进行仿真实验。由实验结果可知,该模型可以提高时间序列的预测精度,且具有良好的泛化能力及实际应用价值。     

Charge state effect on the K-shell ionization of iron by xenon ions near the Bohr velocity

Fe K-shell ionization cross sections induced by 2.4–6.0 MeV Xe20+are measured and compared with different binaryencounter-approximation(BEA)models.The results indicate that the BEA model corrected both by the Coulomb repulsion and by the effective nuclear charge(Zeff)agrees well with the experimental data.Comparison of Fe K-shell X-ray emission induced by 5 MeV xenon ions with different initial charge states(20+,22+,26+,30+)verifies the applicability of the effective nuclear charge(Zeff)correction for the BEA model.It is found that Zeffcorrection is reasonable to describe direct ionization induced by xenon ions with no initial M-shell vacancies.However,when the M shell is opened,the Zeffcorrected BEA model is unable to explain the inner-shell ionization,and the electron transfer by molecular-orbital promotion should be considered.     

张弦梁(桁架)结构的找形方法——分级卸载法

对张弦梁(桁架)结构的找形问题进行了深入研究,根据该类结构的受力特点,提出了分级卸载法。该方法无需假定结构零状态几何,而可以一次得到对应于初状态(即预应力态)几何的结构施工放样尺寸(即零状态几何),并通过分级加载对该方法的精度进行了检验。     

正交异性板条的渐近分析

本文阐明由三维薄弹性体的渐近分析导出各级精度板壳理论的基本方法。将多尺度分析用于板的内部区域和边界层区域导出应力,应变和位移等物理量的不同的无量纲小厚度参数ε的渐近展开式。与工程的方法不同,推导仅基于ε→0的渐近分析,对板的变形不做任何假定。给出正交异性板的平面应变渐近展开的具体列式,仅有一些常数待定。结果表明,内域解渐近级数的首项正是熟知的Kirchhoff板理论解。本文为内域解和边界层解的渐近匹配,从而正确表述圣维南原理并用以建立各级渐近解的边界条件进而求解的研究做好了准备。     

A corresponding-state approach to quark-cluster matter

The state of super-dense matter is essential for us to understand the nature of pulsars; however, non- perturbative quantum chromodynamics makes it very difficult to make direct calculations of the state of cold matter at realistic baryon number densities inside compact stars. Nevertheless, from an observational point of view, it is conjectured that pulsars could be made up of quark clusters since the strong coupling between quarks might render the quarks to be grouped in clusters. In this paper, we attempt to find an equation of state of condensed quark-cluster matter in a phenomenological way. Supposing that the quark-clusters could be analogized to inert gases, we apply here the corresponding-state approach to derive the equation of state of quark-cluster matter, as was similarly demonstrated for nuclear and neutron-star matter in the 1970s. According to the calculations that we have presented, the quark-cluster stars, which are composed of quark-cluster matter, could have a high maximum mass that is consistent with observations and, in turn, further observations of pulsar mass could also place a constraint on the properties of quark-cluster matter. We will also briefly discuss the melting heat during the solid-liquid phase conversion and its related astrophysical consequences.     

可观测度的探讨及其在捷联惯导系统可观测性分析中的应用

可观测度是为了分析线性系统中组合状态的可观测程度而提出来的,在卡尔曼滤波的滤波效果分析中得到了应用。文中先对已有的两种可观测度分析方法进行了简述,并且分析了两种方法的等价性;然后从理论上分析了此描述方法的不全面性。通过典型例子说明了理论分析的结果,给出了一种更全面的描述系统可观测组合状态可观测度的方法,并且用新的描述方式分析了捷联惯导系统的各状态可观测度。结果表明,该数值刻画方式能够定量的给出系统状态可观测的程度,是解析分析方法的很好的补充。     

具有时滞的生态-传染病模型的定性分析

针对一类疾病在食饵中传播而把食饵分为易感和染病的时滞生态-传染病模型,以时滞(即传染病在食饵种群中的潜伏期)作为分支参数,讨论了系统正平衡点在时滞τ=0时的局部渐近稳定性,在τ0时在一列临界值处发生了Hopf分支,并且对保持正平衡点稳定时时滞的范围也给出了估计.     

二元联合生存状态与Makeham死亡律

证明了在生存群中,如果对任意二元联合生存状态,总能找到一个联合生存状态由两个年龄相同的个体组成,并且这两个联生状态的生存分布相同,则群体死亡力为线性函数或Makeham死亡力.最终得到结论如下,二元联合生存状态中的两个个体可以由两个年龄相同的个体替代的充分必要条件是,群体死亡力服从Makeham死亡律或线性死亡律.     

基于几何均值的惩罚型状态变权向量的构造及应用

依据惩罚型状态变权向量的定义和对各因素间的均衡性要求,构造了含有几何平均值的惩罚型状态变权向量.给出了各因素的几何平均值相等和几何平均值不相等两种情况的构造方法,对多因素的变权综合提供了有效的理论支持.最后,用一个实例验证了该方法的可行性和有效性.     

Ultrafast Excited State Dynamics of t~rans-4-Aminoazobenzene Studied by Femtosecond Transient Absorption Spectroscopy

The ultrafast excited state dynamics of trans-4-aminoazobenzene （trans-4-AAB） in ethanol was investigated by femtosecond transient absorption spectroscopy. After being excited to the S2 state by 400 nm, trans-4-AAB decays from the S2 state to the hot S1 state by internal conversion with time constant of -70 fs. The photoisomerization through inversion mechanism on the S1 potential energy surface and the internal conversion from the S1 state to the hot So state are observed, respectively. The average timescale of these two decay pathways is -0.7 ps. And the vibrational cooling of the hot So state of cis- and trans-4- AAB occur with time constants of -4 and N13 ps, respectively. Furthermore, the ultrafast intersystem crossing process are also observed. The timescale of intersystem crossing from the S2 state to the T4 state is about 480 ps while from the S1 state to the T2 state is -180 ps.