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91.
A. Bhadra 《Astrophysics and Space Science》2007,310(1-2):169-172
Scalar tensor (ST) theories of gravitation contain an attractor mechanism towards general relativity. The mechanism is supposed
to start back at time of inflation. Consequently the characteristic coupling function of the ST theories could attain a very
large value during the radiation epoch. Here ST cosmology in the radiation dominated universe is studied under such situation.
A general solution of the scale factor in the radiation dominated flat universe is obtained that is characterized by an additional
degree of freedom. An implication of this extra parameter is discussed.
相似文献
92.
张量CSAMT(可控源音频大地电磁法)能完整地描述三维的地电信息,更适应复杂地质条件下的地质勘探。采用将总场分解为一次场和二次场的策略,用差分近似微分形成大型线性方程组,通过解方程组得到张量CSAMT三维正演结果。通过计算低阻和高阻目标体的响应,发现卡尼亚视电阻率和视阻抗相位对低阻体表现为低值异常,对高阻体表现为高值异常,视阻抗相位达到极值时的频率比视电阻率达到极值时的频率要高。张量CSAMT对低阻体比高阻体更灵敏,在同样条件下,高阻体的异常区位置相比于低阻体会上移。某工区的勘察案例表明,根据卡尼亚视电阻率异常能定性地判断地下异常体的存在,为解决地质类问题提供了依据。本研究为张量CSAMT三维反演提供了基础。 相似文献
93.
查明泥河湾盆地新生界及中生界地层序列及基底的分布与赋存形态是研究泥河湾盆地形成机制的基础性工作。本研究在泥河湾盆地桑干河与壶流河交接处附近采集了四条测线的反射地震数据,通过对精细处理后的地震剖面进行详细分析,在剖面上厘定了三个具有明显强反射标志的地层,即古近系的玄武岩、侏罗系上统的含煤地层和侏罗系下统的含煤地层;其中,新近系沉积层与古近系玄武岩界面在地震剖面上出现的双程旅行时为0.3~0.6s,深度范围为300~500m,而第四系泥河湾组底界由南西到北东逐渐加深,其界面深度为200~300m;侏罗系上统含煤地层在地震剖面上出现的双程旅行时在0.8s上下波动,其深度约为1200m,探测出侏罗系上统顶界面的深度范围为800~1100m;侏罗系下统含煤地层在地震剖面上出现的双程旅行时为1.0~1.4s,深度范围为1800~2000m,由此推测出中生界侏罗系与古生界寒武系地层分界线的深度为2000m左右;根据地震反射波阻抗差别推测出新元古界和太古界地层的分界面在地震剖面上出现的时间约为2.5s,其深度为4000m左右。本研究通过四条反射地震测线的数据基本上查明了泥河湾盆地位于探测区处第四系泥河湾组底界面的深度分布范围及起伏形态、侏罗系上统顶界面和下统底界面的大致埋深,为查明泥河湾盆地新生界及中生界地层序列提供了基础性的参考信息。 相似文献
94.
Axially symmetric cosmological models with cosmic string source are obtained in a scalar-tensor theory of gravitation proposed
by Saez and Ballester (Phys. Lett. A113, 467, 1985). The models obtained give us axially symmetric geometric (Nambu) string, p-string and Reddy string (Astrophys. Space Sci. 286, 2003b) in Saez-Ballester theory. Some physical properties of the models are also discussed. 相似文献
95.
The effects of soil–structure interaction (SSI) while designing the liquid column damper (LCD) for seismic vibration control of structures have been presented in this study. The formulation for the input–output relation of a flexible‐base structure with attached LCD has been presented. The superstructure has been modelled by a single‐degree‐of‐freedom (SDOF) system. The non‐linearity in the orifice damping of the LCD has been replaced by equivalent linear viscous damping by using equivalent linearization technique. The force–deformation relationships and damping characteristics of the foundation have been described by complex valued impedance functions. Through a numerical stochastic study in the frequency domain, the various aspects of SSI on the functioning of the LCD have been illustrated. A simpler approach for studying the LCD performance considering SSI, using an equivalent SDOF model for the soil–structure system available in literature by Wolf (Dynamic Soil–Structure Interaction. International Series in Civil Engineering and Engineering Mechanics. Prentice‐Hall: Englewood Cliffs, NJ, 1985) has also been presented. Copyright © 2005 John Wiley & Sons, Ltd. 相似文献
96.
A numerical procedure to determine the equivalent permeability tensor of a fractured rock is presented, using a stochastic REV (Representative Elementary Volume) concept that uses multiple realizations of stochastic DFN (Discrete Fracture Network) models. Ten square DFN models are generated using the Monte Carlo simulations of the fracture system based on the data obtained from a site characterization program at Sellafield, Cumbria, UK. Smaller models with varying sizes of from 0.25 m×0.25 m to 10 m×10 m are extracted from the generated DFN models and are used as two-dimensional geometrical models for calculation of equivalent permeability tensor. The DFN models are also rotated in 30º intervals to evaluate the tensor characteristics of calculated directional permeability. Results show that the variance of the calculated permeability values decreases significantly as the side lengths of the DFN models increase, which justifies the existence of a REV. The REV side length found in this analysis is about 5 m and 8 m with 20% and 10% acceptable variations, respectively. The calculated directional permeability values at the REV size have tensor characteristic that is confirmed by a close approximation of an ellipse in a polar plot of the reciprocal of square roots of the directional permeability.
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Ki-Bok MinEmail: Phone: +46-8-7907919Fax: +46-8-7906810 |
97.
Yves Grandati Alain Bérard Hervé Mohrbach 《Celestial Mechanics and Dynamical Astronomy》2009,103(2):133-141
In the category of motions preserving the angular momentum direction, Gorringe and Leach exhibited two classes of differential
equations having elliptical orbits. After enlarging slightly these classes, we show that they are related by a duality correspondence
of the Arnold–Vassiliev type. The specific associated conserved quantities (Laplace–Runge–Lenz vector and Fradkin–Jauch–Hill
tensor) are then dual reflections of each other. 相似文献
98.
99.
随着传感器技术的发展,重力场与重力张量场测量技术发展迅速,为实现地下密度分布精细反演提供了数据保障。正演是反演的基础,解决任意密度分布复杂地质体重力场与重力张量正演高效、高精度计算问题,是实现重力高效、精细反演、人机交互反演解释的关键。针对起伏地形和任意密度分布这种复杂条件下二维重力场及重力张量场高效高精度正演问题,这里提出了一种空间波数混合域正演算法,其关键环节包括:①结合新的矩形二度体组合模型波数域表达式和一维Gauss-FFT算法,提出了一种任意密度分布和起伏地形下重力场及重力张量高效、高精度正演算法;②采用新的二维正演算法,计算观测最高点和最低点之间多个不同高度水平网格重力场及重力张量,结合三次样条插值方法,实现了起伏地形上重力场及重力张量场高效、高精度正演。模型算例结果表明,新方法具有高效、高精度的显著特点。 相似文献
100.
提出了一种新的波阻抗反演方法,首先根据地下反射系数序列是一个稀疏脉冲序列这一假设,将地震波阻抗反演中的目标函数表示为L1范数约束下的L1范数优化问题,并将L1范数用一个平滑函数来近似,从而使得目标函数函数可微。然后将L1范数约束下的基追踪问题转化为无约束最优化问题,并利用基于导数的局部优化方法求解无约束优化问题,求得反射系数,进而计算得到波阻抗。模型和实际资料计算结果均表明该方法可行。 相似文献