On bending angles by gravitational lenses in motion     

Simonetta Frittelli 《Monthly notices of the Royal Astronomical Society》2003,340(2):457-462

  相似文献   

Importance of perturbed gravitational potentials in differentially rotating Newtonian stars     

S. Karino 《Monthly notices of the Royal Astronomical Society》2003,343(1):175-180

  相似文献   

The 550-au Mission: a critical discussion     

S. G. Turyshev  B-G. Andersson 《Monthly notices of the Royal Astronomical Society》2003,341(2):577-582

We have studied the science rationale, goals and requirements for a mission aimed at using the gravitational lensing from the Sun as a way of achieving high angular resolution and high signal amplification. We find that such a mission concept is compromised by several practical problems. Most severe are the effects due to the plasma in the solar atmosphere which cause refraction and scattering of the propagating rays. These effects either limit the frequencies that can be observed to those above ∼1 THz, or they move the optical point outwards beyond the vacuum value of ≥550 au. (Thus for observing frequency of 300 GHz the optical point is moved outwards to ∼ 680 au.) Density fluctuations in the inner solar atmosphere will further cause random pathlength differences for different rays. The corrections for the radiation from the Sun itself will also be a major challenge at any wavelength used, but could be mitigated with coronographic techniques. Given reasonable constraints on the spacecraft (particularly in terms of size and propulsion), source selection as well as severe navigational constraints further add to the difficulties for a potential mission. Nevertheless, unbiased surveys of small-scale structure on the sky at short wavelengths might be the most promising application of such a mission.  相似文献   

On determining the cluster abundance normalization     

Elena Pierpaoli  Stefano Borgani  Douglas Scott  Martin White 《Monthly notices of the Royal Astronomical Society》2003,342(1):163-175

  相似文献   

A Solution of Einstein's Field Equations fora Tachyonic Gas: Possible Astrophysical Applications     

W.J. Cocke  K.H. Green 《Astrophysics and Space Science》2003,288(4):327-346

In this paper we show that a change in the signs of some of the metric components of the solution of the field equations for the classical cosmic string results in a solution which we interpret as a time-dependent wall composed of tachyons. We show that the walls have the property of focusing the paths of particles which pass through them. As an illustration of this focusing, we demonstrate the results of a simple simulation of the interaction between one such tachyon wall and a rotating disk of point masses. This interaction leads to the temporary formation of spiral structures. These spiral structures exist for a time on the order of one galactic rotation. This revised version was published online in July 2006 with corrections to the Cover Date.  相似文献   

Cosmic structure growth and dark energy     

E. V. Linder  A. Jenkins 《Monthly notices of the Royal Astronomical Society》2003,346(2):573-583

Dark energy has a dramatic effect on the dynamics of the Universe, causing the recently discovered acceleration of the expansion. The dynamics are also central to the behaviour of the growth of large-scale structure, offering the possibility that observations of structure formation provide a sensitive probe of the cosmology and dark energy characteristics. In particular, dark energy with a time-varying equation of state can have an influence on structure formation stretching back well into the matter-dominated epoch. We analyse this impact, first calculating the linear perturbation results, including those for weak gravitational lensing. These dynamical models possess definite observable differences from constant equation of state models. Then we present a large-scale numerical simulation of structure formation, including the largest volume to date involving a time-varying equation of state. We find the halo mass function is well described by the Jenkins et al. mass function formula. We also show how to interpret modifications of the Friedmann equation in terms of a time-variable equation of state. The results presented here provide steps toward realistic computation of the effect of dark energy in cosmological probes involving large-scale structure, such as cluster counts, the Sunyaev–Zel'dovich effect or weak gravitational lensing.  相似文献   

空间扰动引力的谱分析   总被引：1，自引：0，他引：1  

赵德军  吴晓平 《海洋测绘》2005,25(2):6-8

基于重力场的频谱理论，给出了扰动引力在全球平均意义下的功率谱表达式，揭示了扰动引力的传播特性。通过数值试验，给出了扰动引力随高度变化规律，并分析了不同高度上，扰动引力恢复重力场的最高阶数及相应分辨率。从理论上分析了航空重力测量探测重力场中高频信息的能力，对制定飞行方案有一定参考价值。  相似文献   

高原山区局部大地水准面精化方法研究     

李海文  罗满建  吴友平  王家帮 《测绘科学》2008,33(5)

局部大地水准面精化的实质是精确计算出大地水准面的起伏变化情况。一般情况下,需要密度足够的重力数据,依重力异常密集计算大地水准面差距或高程异常。但是在大陆西部高原山区重力点密度是不够的,无法达到大地水准面精化的目的。本文从理论上证实了用地形和岩石密度数据进行局部大地水准面精化的可行性。  相似文献   

弹道计算中的扰动引力影响研究     

LI Xiao-yan    WANG Xing-tao  LI Jian-tao 《测绘学院学报》2008,(4)

随着弹道导弹系统技术的不断改进,影响导弹精度的工具类误差已逐渐降低,地球重力场扰动引力已经成为影响导弹命中精度的主要因素。这里从3个方面分析了扰动引力对弹道的影响,模拟结果表明,对于射程为10000 km以上的远程导弹,扰动引力的影响会造成超过1 km的落点偏差;5×10-5m s-2的扰动引力系统性偏差对导弹落点有明显影响。因此,扰动引力对导弹落点的影响不容忽视。  相似文献   

太平庄井地下流体动态主要干扰因素研究   总被引：1，自引：0，他引：1  

刘成龙  陶京玲  王志敏 《华北地震科学》2003,21(3):59-64

通过分析多年的观测资料，认为太平庄井地下流体动态的主要干扰因素为区域地下热水开采，其次为降雨。气压的明显变化对水位、水温也有一定干扰。区域开采造成太平庄井水位、水温同步下降，氢气测值升高；降雨导致太平庄井水位上升、水温下降。  相似文献