A mass ratio limit for primordial black holes

We augment our scenario for the formation of astronomical objects from macroscopic superstrings by the assumption that the central matter keeps its identity in the fragmentation. From the condition that the angular momentum per mass squared of this matter should be less than the Kerr limit G/c, we obtain upper limits for the ratio of the mass of central black holes M(BH) to the mass M of the host object. This limit is M(BH)/M ≈ 0.001, and, expressed in observed quantities, approximately M(BH)/M ≈ σ²/(v · c) where σ is the r.m.s. velocity, v the rotational velocity and c the velocity of light. The valuesM(BH) agree with the observed behaviour both in order of magnitude and in the variation with velocity dispersion. (© 2003 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)     

Dynamic Prediction Model of Overburden Settlement in Deep Mining Areas based on Space–Time Relationship

Natural Resources Research - Depletion of shallow mineral resources caused by deep mining has become an inevitable trend, and deep mining can increase safety accidents and geological hazards....     

Temporal and spatial dynamical simulation of groundwater characteristics in Minqin Oasis

Application scope of geostatistics has been gradually extended from original geologic field to soil science and ecological field, etc. and its successful application results have been widely demonstrated. But little information is reported as to the direct use of geostatistical method to work out the distribu- tion map of groundwater characteristics. In this paper the semivariogram of geostatistics, in combina- tion with GIS, was used to quantitatively study the spatial variation characteristics of groundwater table depth and mineralization degree and their relation to the landuse changes. F test of the used spherical model reached a very significant level, and the theoretical model can well reflect the spatial structural characteristics of groundwater table depth and mineralization degree and achieve an ideal result. This shows that the application of the method in the dynamical simulation of groundwater is feasible. And this paper also provides useful reference for the application of geostatistics in the study of the dy- namical variations of groundwater resources in the oasis.     

地磁低点位移法的改进

中低纬度地磁场平静太阳日变化Z分量的极小值出现的时刻常被用于地震预报,即"低点位移"法,但现有算法的时间格式和人工绘制突变界线的模式会产生较大的误差,本文在第一部分针对这些误差改进了原有算法.第一项是改进了地磁低点时间的格式,第二项是引入了Voronoi剖分技术替代人工画线.前者过滤了假的突变界线,消除了系统误差;后者建立了突变界线与地磁台网低点数据之间的解析关系,使它们一一对应,消除了随机误差.本文第二部分内容是提出了新的时间格式与数字化突变界线的计算公式,并用程序实现计算任务.本文第三部分内容是在对地磁台网的低点时间跟踪的过程中,捕捉到了甘肃省周边几次地震前的地磁低点位移现象,并分析这些案例,在结论中证明该方法的可靠性.     

铁路缓和曲线的等间隔放样方法

介绍了铁路缓和曲线设置的目的、作用、基本原则和重要意义，阐述了等间隔放样缓和曲线的基本原理，给出了等间隔放样缓和曲线放样要素采集的基本方法，叙述了缓和曲线等间隔放样的工作过程。     

利用FHT法反演海洋重力

从快速 Hartley变换 (FHT)基本概念入手 ,给出了 Hotine核在平面近似、球面近似、Molodenskii近似下的反演模型。另对 FHT处理中所需的坐标转换以及边缘效应等问题加以讨论。同时 ,为了改善长波特性的重力场信息 ,利用 M阶次的参考重力场对上述 Molo-denskii模型进行了改化。     

基于PSInSAR的成都地区地表沉降空间分布研究

针对成都地区土地规划利用的需要,采用永久散射体合成孔径雷达干涉测量技术(Permanent Scatterer InSAR,PSInSAR)对成都地区地表沉降空间分布情况进行了实验研究。结果表明,在该研究时段内研究区域最大沉降量达到24 mm,最大抬升量达到18 mm。研究区西北至东南方向地表在研究时段内发生了抬升,东北至西南方向出现了地表沉降现象,并对可能造成地表沉降的主要原因进行了分析。     

地面沉降时空形变场的构建方法研究

由于离散分布的精密水准测量数据只能对点状沉降信息进行监测分析,描述特定时间点的静态空间趋势,无法表达区域性地面沉降整体时空变化.该文提出一种地面沉降时空形变场的构建方法,在多项式拟合法构建形变场的基础上考虑时间项,通过探索地面沉降量与坐标、时间的关系,对区域地面形变的整体效果进行拟合,构建地面沉降时空形变场.该方法顾及...