黑洞吸积理论及其天体物理学应用的近期发展(Ⅱ)

黑洞吸积理论是天体物理学的一个基础理论,是认识许多高能天体系统如活动星系核、黑洞X射线双星,以及伽马暴等的重要物理基础.该文评述近年来黑洞吸积理论尤其是径移主导吸积流模型(advection-dominated accretion flow)及其变种的主要发展,并介绍该理论在银河系中心、低光度活动星系核、黑洞X射线双星等方面的应用.共分为两篇,该文是第2篇,内容是关于黑洞热吸积流理论在低光度活动星系核以及黑洞X射线双星方面的应用.     

Iron line profiles and self-shadowing from relativistic thick accretion discs

We present Fe Kα line profiles from and images of relativistic discs with finite thickness around a rotating black hole using a novel code. The line is thought to be produced by iron fluorescence of a relatively cold X-ray-illuminated material in the innermost parts of the accretion disc and provides an excellent diagnostic of accretion flows in the vicinity of black holes. Previous studies have concentrated on the case of a thin, Keplerian accretion disc. This disc must become thicker and sub-Keplerian with increasing accretion rates. These can affect the line profiles and in turn can influence the estimation of the accretion disc and black hole parameters from the observed line profiles. We here embark on, for the first time, a fully relativistic computation which offers key insights into the effects of geometrical thickness and the sub-Keplerian orbital velocity on the line profiles. We include all relativistic effects such as frame-dragging, Doppler boost, time dilation, gravitational redshift and light bending. We find that the separation and the relative height between the blue and red peaks of the line profile diminish as the thickness of the disc increases. This code is also well suited to produce accretion disc images. We calculate the redshift and flux images of the accretion disc and find that the observed image of the disc strongly depends on the inclination angle. The self-shadowing effect appears remarkable for a high inclination angle, and leads to the black hole shadow being in this case, completely hidden by the disc itself.     

释放化学物质耗空电离层电子密度的研究

电离层作为电波传播的主要通道和载体,影响着无线电通信的质量,因此人工电离层扰动具有广阔的应用前景,在电离层中释放具有较强电子亲和力的化学物质可以耗空电离层F区的电子密度,是人工电离层扰动的有效手段之一.本文通过对CO2和SF6气体在电离层中的扩散和离子化学反应过程的分析,理论计算了在我国北京地区上空释放这两种气体后电离...     

Primordial black holes

Primordial black holes (PBHs) are a profound signature of primordial cos-mological structures and provide a theoretical tool to study nontrivial physics of the early Universe. The mechanisms of PBH formation are discussed and observational constraints on the PBH spectrum, or effects of PBH evaporation, are shown to re-strict a wide range of particle physics models, predicting an enhancement of the ul-traviolet part of the spectrum of density perturbations, early dust-like stages, first or-der phase transitions and stages of superheavy metastable particle dominance in the early Universe. The mechanism of closed wall contraction can lead, in the inflation-ary Universe, to a new approach to galaxy formation, involving primordial clouds of massive BHs created around the intermediate mass or supermassive BH and playing the role of galactic seeds.     

锦屏一级水电站地下厂房系统对穿预应力锚索孔孔斜控制施工技术

锦屏一级水电站地下厂房洞室主机间、主变室、母线洞等洞室系统的边墙、蚀变岩段和较大断层采用了对穿预应力锚索加强支护。在对穿预应力锚杆的施工过程中,根据不同的地质地层段,采取严格的孔斜控制措施,并不断地改进控制方法,基本解决了对穿预应力锚索造孔孔斜控制的技术问题,满足了设计技术要求,积累了对穿预应力锚索孔斜控制施工经验。     

灌注桩后注浆单桩竖向极限承载力研究

近年来,后注浆技术得到了广泛的应用。钻孔灌注桩可大大降低建筑物的沉降,并使建筑物的沉降更加均匀,文章介绍后注浆工艺的承载力提高机理及在天津地区的几个工程实例,分析了注浆前后单桩竖向极限承载力对比情况及影响单桩竖向极限承载力的几个因素。     

钻探工作中常见孔内事故的预防与处理

钻探工作中,由于地层,机械,及工作人员的水平等原因会发生各种孔内事故,根据事故的具体原因,应选择相应的处理方式,预防孔内事故的发生会减少工作成本,提高工作效率。本文研究了孔内事故的预防及处理事故的方法。