The Origin of the Element Eu in Extremely Metal-poor Halo Stars

The fast neutron capture process (the r-process) occurs in the neutron-rich circumstance. However its concrete physical environment is not very clear. With recent progress in observations, many extremely metal-poor halo stars have been discovered. They have two characteristics: one is the overabundance of fast neutron elements with the relative abundance consistent with that of the sun; the other is that fast neutron element contents in stars at the same metal abundance have a very large dispersion. This provides a particular way to study the origin of the r-process. Simulation was used to study the galaxy's evolution process and the resulting dispersion of fast neutron nuclide contents in stars. The model of galaxy evolution obtained in this way not only contains spontaneous star formation in the gas region, but also includes the star formation excited by the supernova explosion. It is shown from our results that the supernovae at the low mass end should be the place producing the fast neutron nuclides. In addition, it is also shown that the non-uniformity of the galaxy evolution caused by the supernova explosion is not enough to explain the observed dispersion of fast neutron element contents in halo stars. This problem should be further studied.     

Study of the dependence of the star formation rate in the nuclear regions of 39 Kazarian galaxies on their integral parameters

A statistical study of the dependence of the star formation rate in the nuclear regions of 39 Kazarian galaxies on the integral parameters of these galaxies is carried out on the basis of spectra from SDSS DR6. The value of SFR/kpc² for our sample lies in the range 0.013÷2.04M _⨀ year⁻¹kpc⁻² (with the maximum value of 2.04 corresponding to the Kaz 98 (merger)). It is found that the surface density of the rate of star formation correlates positively with the bar structure parameter and EW(Hα), and that, for spiral galaxies of early morphological types, SFR/kpc² is greater than for the later types. It is shown that the color B-R for the galaxies and the color (u − g) _nucl for the nuclear region correlate positively with the total absorption A(Hα) in the Ha line for the nuclear region. The average value of A(Hα) for our samples is found to be A(Hα)=1.3±0.09 magnitudes. Translated from Astrofizika, Vol. 52, No. 2, pp. 211–224 (May 2009).     

The approximation of neutrino heat conduction with neutrino scattering

We have developed an algorithm for taking into account the neutrino scattering in the approximation of neutrino heat conduction. We show that in the case of incoherent neutrino scattering (e.g., by electrons), the coefficients of the temperature and chemical potential gradients are averaged over the neutrino energy using functions that can be found by numerically solving integral equations. The coherent scattering by free nucleons and atomic nuclei can be described by introducing a transport cross section. We suggest a new method for calculating the neutrino—electron scattering functions that is based on Fermi—Dirac functions of integer indices.     

高放废物地质处置阿拉善预选区巴彦诺日公地段目标深度岩体质量预测

高放废物地质处置阿拉善预选区巴彦诺日公地段位于阿拉善地块东部,主要由二叠纪侵入的花岗岩构成,地壳次稳定。通过踏勘,确定了2个钻孔,布置了若干条物探剖面。以这2个钻孔为中心,在17km×17km范围内进行了工程地质测绘,获得了地表结构面分布特征。地表岩体质量以III级岩体为主,地表以下3m~4m处多为I级和II级岩体。根据钻孔岩芯编录和力学试验数据,对岩芯质量进行评价,岩芯整体质量较好,以Ⅰ级和Ⅱ级岩体为主。对比岩体质量和测井数据,发现岩体质量与岩体的物理参数具有明显的相关性。通过和CSAMT剖面上对应位置的对比,建立了岩体质量与电阻率的关系。结合地表岩体质量、钻孔岩芯质量和物探剖面,对目标深度岩体进行了预测：目标深度（600m深左右）岩体质量以Ⅰ级岩体为主,局部有Ⅱ级岩体和Ⅲ岩体。     

基于L1范数的波阻抗反演

提出了一种新的波阻抗反演方法,首先根据地下反射系数序列是一个稀疏脉冲序列这一假设,将地震波阻抗反演中的目标函数表示为L1范数约束下的L1范数优化问题,并将L1范数用一个平滑函数来近似,从而使得目标函数函数可微。然后将L1范数约束下的基追踪问题转化为无约束最优化问题,并利用基于导数的局部优化方法求解无约束优化问题,求得反射系数,进而计算得到波阻抗。模型和实际资料计算结果均表明该方法可行。     

朝鲜2017年核爆对中国东北地区形变场的影响

基于19个连续GNSS观测站的多种采样率（10 Hz、1 Hz和30 s）数据,分析2017-09-03朝鲜核爆对中国东北地区地壳形变场的影响。静态位移分析结果显示,距核爆现场最近的GNSS观测站JLCB没有产生明显的同震形变,与基于均匀半无限弹性空间断裂位错模型正演模拟的结果一致;GNSS应变结果显示,此次核爆在东北区域引起主应变的略微调整,但总体调整量在10-8以内,没有引起区域范围内面应变的变化;高频GNSS动态形变分析结果显示,核爆在JLCB站处没有引起明显的波形变化。另外,高频GNSS受到多路径效应的影响,可能会引起cm级的扰动,利用恒星日滤波方法可以抑制多路径的影响,得到精度更高、更可靠的动态形变结果。     

撞击事件诱发核反应热力学过程及其在事件地质学研究中的意义

摘要：从大规模撞击事件的基本动力学和热力学公式推导出发,讨论了白垩纪－第三纪界线（Ｋ／Ｔ界线）事件能量随时间的释放过程,并对发生热核聚变反应的条件进行了分析。最后,还对其可能的事件地质学意义进行了讨论．     

核电厂取水明渠泥沙回淤分析

核电厂需用大量冷却水,用水量为工业用水的第一位。明渠取水是核电厂常用的取水方式之一。本文针对电厂取水明渠及口门外水流特点,分析计算了取水明渠内各部位及口门外过渡段的泥沙回淤率,并提出减少明渠泥沙回淤量的措施。     

自由网平差的经典方法及扩展应用

采用经典的最小二乘参数平差结果为一个特解,进而以坐标系定位参数为参数求出自由网的最小范数解。之后,以若干工程实例列举了除变形监测网以外的扩展应用。     

岭澳核电站厂址转移和定位

在广东第二核电站确定在深圳市岭澳地区建设后, 广东省电力设计研究院进一步分析了岭澳地区内各候选地点的特点, 果断地提出厂址由原先推荐的岭澳东移至岭澳西, 并据此完成了项目的可行性研究。实践证明： 厂址转移工作是成功的, 将带来巨大的社会效益。特大型工矿企业的定位是基本建设中的一项战略部署, 本文以岭澳核电站为例, 就厂址转移的原因、工作思路及工作过程作了具体的论述