Gravitational Waves and Gravitational-wave Sourcestwo

The recent discovery of gravitational-wave burst GW150914 marks the coming of a new era of gravitational-wave astronomy, which provides a new window to study the physics of strong gravitational field, extremely massive stars, extremely high energy processes, and extremely early universe. In this article, we introduce the basic characters of gravitational waves in the Einstein's general relativity, their observational effects and main generation mechanisms, including the rotation of neutron stars, evolution of binary systems, and spontaneous generation in the inflation universe. Different sources produce the gravitational waves at quite different frequencies, which can be detected by different methods. In the lowest frequency range (f < 10^?15 Hz), the detection is mainly dependent of the observation of B-mode polarization of cosmic microwave background radiation. In the middle frequency range (10^?9 < f < 10^?6 Hz), the gravitational waves are detected by analyzing the timing residuals of millisecond pulsars. And in the high frequency range (10 ? 4 < f < 10⁴ Hz), they can be detected by the space-based and ground-based laser interferometers. In particular, we focus on the main features, detection methods, detection status, and the future prospects for several important sources, including the continuous sources (e.g., the spinning neutron stars, and stable binary systems), the burst sources (e.g., the supernovae, and the merge of binary system), and the stochastic backgrounds generated by the astrophysical and cosmological process. In addition, we forecast the potential breakthroughs in gravitational-wave astronomy in the near future, and the Chinese projects which might involve in these discoveries.     

What do parameterized Om(z) diagnostics tell us in light of recent observations?

In this paper, we propose a new parametrization for Om(z) diagnostics and show how the most recent and significantly improved observations concerning the H(z) and SN Ia measurements can be used to probe the consistency or tension between the ΛCDM model and observations. Our results demonstrate that H0 plays a very important role in the consistency test of ΛCDM with H(z)data. Adopting the Hubble constant priors from Planck 2013 and Riess, one finds considerable tension between the current H(z) data and ΛCDM model and confirms the conclusions obtained previously by others. However, with the Hubble constant prior taken from WMAP9, the discrepancy between H(z) data and ΛCDM disappears, i.e., the current H(z) observations still support the cosmological constant scenario. This conclusion is also supported by the results derived from the Joint Lightcurve Analysis(JLA) SN Ia sample. The best-fit Hubble constant from the combination of H(z)+JLA(H00 = 68.81+1.5-1.49 km s-1 Mpc-1) is very consistent with results derived both by Planck 2013 and WMAP9, but is significantly different from the recent local measurement by Riess.     

Changing Connectivities of Chinese Cities in the World City Network,2010–2016

Against the backdrop of the sizable economic growth of China in recent years, this paper uses the most recent data gathering of the Globalization and World Cities(Ga WC) research network to update and supplement earlier research on the shifting global connectivity of Chinese cities. The update consists of an evaluation of the connectivity of Chinese cities in 2016, the supplement of an analysis of the changing position of Chinese cities in the world city network between 2010 and 2016. To this end, we build on a specification of the world city network as an ‘interlocking network' in which producer services firms play the crucial role in city network formation. Information about the presence of leading producer services firms in cities in 2010 and 2016 is used as the input to a bipartite network projection algorithm in order to measure cities' network connectivity. The first set of results discusses the geographies of urban connectivity in the world city network in 2016. The second set of results discusses standardized measures of change to reveal the major dimensions of the transformations between 2010 and 2016. We find that, with the exception of Hong Kong, Macau and Kaohsiung of Taiwan, all Chinese cities record connectivity gains. This wholesale rise in connectivity is nonetheless geographically uneven, with above all Beijing, Chengdu/Chongqing and Changsha/Wuhan becoming more connected. We conclude that the wholesale rise of Chinese cities in the world city network and their changing trajectories in the post-crisis era are embedded in shifting external and internal political economies.     

北京高空温度的统计特征

对１９６１～１９９４年自地面至高空２０ｈＰａ的温度资料进行了统计分析,以了解北京高空气温的季节变化、垂直分布和长期变化趋势。研究发现：以１５０ｈＰａ层为界,其上部和下部的温度变化有着不同的气候特征,如在该层以下各层上的温度年较差为正值,而其上则为负值;近３０余年来,对流层下层温度显著增加,对流层上层和平流层的温度在降低,对流层温度直减率加大     

青藏高原多向碰撞─揳入隆升地球动力学模式

论证了青藏高原形成与隆升过程中的变形构造格局。岩石圈结构、青藏高原隆升与周边前陆沉积盆地耦合关系、高原隆升的地球动力学模式等。提出青藏高原碰撞-隆升过程中,高原边缘以走滑-挤压构造为主,高原内部以伸展构造为主;高原隆升过程中,岩石圈变形总体是：上部以伸展变形为主,中部以挤压变形为主,下部以伸展变形为主。通过青藏高原及周边岩石圈结构及隆升过程变形作用时-空耦合关系的对比研究,建立起青藏高原隆升机制的多向碰撞-入隆升地球动力学模式。     

江西金山金矿床两类矿化及其石英热发光特征

金山金矿床为一大型剪切带型独立矿床,主要矿化类型分为含金石英脉及硅化岩型两种,前者分布于金山剪切带上盘粉砂质千枚岩中,受顺层剪切裂隙控制,规模较小;后者主要受金山剪切带内Ｒ型剪切裂隙控制,规模大。研究表明,两类矿化是性质相同的含矿变质流体以不同方式在不同构造位置发生成矿作用的产物。石英热发光特征是评价两者含矿性的有效标志。     

反射波法检测水泥搅拌桩的可行性和方法研究

水泥搅拌桩作为桩基础的一种特殊形式,在软土地基地区已被广泛应用。由于其桩身纵波波速远低于混凝土桩的波速,且长径比一般较小及桩身均质性等问题,所以应用于混凝土桩的小应变反射波检测方法是否可以应用于对水泥搅拌桩进行检测,在测桩界尚存在分歧意见。作者从理论上分析了反射波法的本质,指出波阻抗差异,分辨率和波长的关系是反射波法的要害。本文讨论了长径比的实际意义及其与一维波动理论的关系．提出了水泥搅拌桩“桩身质量“的新观点。从理论分析和实际检测结果资料的讨论出发．肯定了反射渡完全可以对水泥搅拌桩进行检测,并总结了实际检测过程中的方法技术。     

蒙古裸腹溞染色体组型研究

本文对驯养于实验室自然海水中的蒙古裸腹溞（Ｍｏｉｎａ ｍｏｎｇｏｌｉｃａＤａｄａｙ）染色体进行了分析、研究。结果表明：蒙古裸腹溞染色体数目为ｎ＝１２, ２ｎ＝２４。其中１０条为中部着丝点染色体,２条为亚中部着丝点染色体,１２条为端部着丝点染色体,总臂数ＮＦ＝３６。其核型公式为２Ｎ＝１０Ｍ＋２ＳＭ＋１２Ｔ。本文还与溞属（Ｄａｐｈｎｉａ）６个种类的染色体形态进行了比较,并对蒙古裸腹溞孤雌生殖与两性生殖及性转化的问题开展了讨论。     

西藏谢通门县北1998年7月20日6.1级地震烈度及灾害损失评估

１９９８年７月２０日西藏谢通门６．１级地震发生在甲岗东麓断层上。宏观震中位于谢通门县青都乡凯仁村附近,震中烈度为Ⅶ度。该地震震害波及１市、１县、１１个乡、７９个行政村,受灾人口２４ ０５８人,受灾面积达６ ７００ｋｍ ２,造成直接经济损失达９ ７６３ ０００元     

岩溶水系统溶蚀速度的多重耦合模型——以山西太原东山水文地质系统为例

本文运用化学热力学与水文地质系统耦合理论,将太原东山水文地质系统划分成矿物溶解、沉淀各异的区带;通过各区带内的化学—数学与相关分析法的耦合模型,计算出各区带碳酸、硫酸盐岩的综合溶蚀模量;再将综合溶蚀模量和用化学动力学理论确定地下水实际速度的解析解公式与有限单元法耦合,计算确定出各节点的溶蚀速度。从而不仅有效地评价了水文地质系统内的溶蚀特点,还可反映区内地质构造和水文地质条件,以及含水层在倾向方向随埋深增大呈幂函数变化的规律;进而可确定出区内供水、矿井防治水的最佳勘探地段。这些不仅具有一定理论意义,也具有一定的社会和经济效益