The Amplitude of Mass Fluctuations and Mass Density of the Universe Constrained by Strong Gravitational Lensing     

Da-Ming ChenNational Astronomical Observatories  Chinese Academy of Sciences  Beijing  cdm@bao.ac.cn 《中国天文和天体物理学报》2004,4(2):118-124

We investigate the linear amplitude of mass fluctuations in the universe, σ8, and the present mass density parameter of the Universe, Ωm, from statistical strong gravitational lensing. We use the two population model of lens halos with fixed cooling mass scale Mc = 3×1013h-1M⊙ to match the observed lensing probabilities, and leave σ8 orΩm as a free parameter to be constrained by the data. Another varying parameter, the equation of state of dark energy ω, and its typical values of -1, -2/3, -1/2 and -1/3 are investigated. We find that σ8 is degenerate with Ωm in a way similar to that suggested by present day cluster abundance as well as cosmic shear lensing measurements: σ8Ω0.6m≈0.33. However, both σ8≤0.7 and Ωm≤0.2 can be safely ruled out, the best fit is when σ8 = 1.0, Ωm = 0.3 and ω= - 1. This result is different from that obtained by Bahcall & Bode, who gave σ8 = 0.98±0.1 and Ωm = 0.17 ±0.05. For σ8 = 1.0, the higher value ofΩm = 0.35 requires ω = -2/3 and Ωm = 0.40 require  相似文献   

电偶源频率磁测深二维层状模型参数化反演     

林长佑  罗东山 《物探化探计算技术》1997,19(2):115-121

本大地电磁测深松驰反演理论方法的基础上，探讨了电偶源频率电磁深阻抗阻率的二维反演问题。  相似文献   

利用地面深空激光测距检验相对论的引力时延     

杨远贵 《云南天文台台刊》2002,(2):35-40

讨论了广义相对论的引力时延。根据Mini－ASTROD空间计划方案，利用地面深空激光测距来检验引力时延，给出了测量值与理论值直接比对的方案，并拟合出空间曲率参数γ的值。文中采用非同步的激光应答器、皮秒事件记数器等设备，可以提高测量的精度和稳定性。在地面站和行星探测器之间直接进行激光测距，不仅可以验证广义相对论的引力时延，而且还可以使γ的精度提高至少1－2个量级。这对于宇宙学和引力理论具有十分重要的意义。  相似文献   

冲绳海槽岩浆物理化学性质及其地质意义     

黄朋  李安春  胡宁静 《海洋学报》2008,30(3):85-94

借助冲绳海槽火山岩地球化学分析结果,讨论了海槽不同区段岩浆的温度、压力、密度和黏度等物理化学参数,以确定海槽岩浆的物理性质及其对海槽不同区段岩浆演化过程的影响.海槽北段的岩浆相对于中段表现出高压力、低温度的特征.由于海槽岩浆挥发分含量较高,北段岩浆的密度和黏度要高于中段的.但总的来说,海槽岩浆具有低密度、低黏度的特点,因此岩浆更容易穿透岩石圈,而且有利于岩浆结晶分异作用的进行.对海槽岩浆相对运移速度的研究显示,在外部条件及含水量相同的前提下,在海槽中段岩浆上升速度要大于北段的,这从岩浆物理化学性质的角度解释了为何海槽中段火山活动要强于北段的.  相似文献   

Estimates of AGN Black Hole Mass and Minimum Variability Timescale   总被引：4，自引：0，他引：4  

Guang-Zhong Xie  Luo-En Chen Huai-Zhen Li  Li-Sheng Mao  Hong Dai  Zhao-Hua Xie  Li Ma  Shu-Bai Zhou National Astronomical Observatories  Yunnan Observatory  Chinese Academy of Science  Kunming  Yunnan Astrophysics Center  Yunnan University  Kunming Physics Department  Yunnan Normal University  Kunming Physics Department  Yuxi Normal College  Yuxi Graduate University of Chinese Academy of Sciences  Beijing 《中国天文和天体物理学报》2005,5(5):463-470

Black hole mass is one of the fundamental physical parameters of active galactic nuclei (AGNs), for which many methods of estimation have been proposed. One set of methods assumes that the broad-line region (BLR) is gravitationally bound by the central black hole potential, so the black hole mass can be estimated from the orbital radius and the Doppler velocity. Another set of methods assumes the observed variability timescale is determined by the orbital timescale near the innermost stable orbit around the Schwarzschild black hole or the Kerr black hole, or by the characteristic timescale of the accretion disk. We collect a sample of 21 AGNs, for which the minimum variability timescales have been obtained and their black hole masses (Mσ) have been well estimated from the stellar velocity dispersion or the BLR size-luminosity relation. Using the minimum variability timescales we estimated the black hole masses for 21 objects by the three different methods, the results are denoted by Ms, Mk and Md, respectively. We compared each of them with Mσindividually and found that: (1) using the minimum variability timescale with the Kerr black hole theory leads to small differences between Mσand Mk, none exceeding one order of magnitude, and the mean difference between them is about 0.53 dex; (2) using the minimum variability timescale with the Schwarzschild black hole theory leads to somewhat larger difference between Mσand Ms: larger than one order of magnitude for 6 of the 21 sources, and the mean difference is 0.74 dex; (3) using the minimum variability timescale with the accretion disk theory leads to much larger differences between Mσand Md, for 13 of the 21 sources the differences are larger than two orders of magnitude; and the mean difference is as high as about 2.01 dex.  相似文献   

利用地球定向参数确定依巴谷输入星表与射电天球参考架之间的旋转     

《云南天文台台刊》1997,(1):41-46

  相似文献   

不规则波越浪率计算的一个新公式     

李昌良  梁丙臣 《海洋通报》2008,27(5)

对美国<海岸防护手册>(SPM)中估计不规则波浪下越浪率的计算公式作了分析并对其不足进行了改进,提出利用规则波越浪率来计算不规则波作用下越浪率的一个新的公式.认为当建筑物堤顶高程(从静水面算起)为零时,越浪率不仅与波高有关,波速也是一个重要的影响因素,SPM 法的假定不符合实际的工况,导致 SPM 法不是低估就是高估了越浪率的大小.通过数值模拟,将新改进的公式与 SPM 法、实验数据、以及经验公式作了对比,表明新公式是比较合理的,其计算结果可以作为工程设计的参考依据.  相似文献   

高速公路接线处中线偏差的一个特殊处理案例   总被引：1，自引：1，他引：0  

喻雄 《测绘与空间地理信息》2009,32(1)

笔者结合高速公路勘测设计中的实践,介绍高速公路接线处中线偏差的处理及调整方法,介绍了其在AutoCAD中处理的一个例子.  相似文献   

Physical Parameters of a Flare Dervied from Multi—line 2D Spectroscopy     

YingLiu  Ming－De－Ding 《中国天文和天体物理学报》2001,1(5):460-468

Time series of 2D spectra of Hα and CaⅡ λ8542 for a flare of 1999 December 22 are obtained and analyzed with a new fitting technique. The method we proposed can simultaneously yield the four parameters: the line source function, the optical thickness at line center, the line-of-sight velocity and the Doppler width. We present the spatial distributions of the physical parameters and their temporal evolutions determined from the 2D spectra. Our results are consistent with the general picture predicted by the flare dynamic models.  相似文献   

前处理工艺与合成参数对金刚石生长的影响     

石明达 《冶金地质探矿技术》1989,(4):15-18

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