Some Bianchi Type I Viscous Fluid Cosmological Models with a Variable Cosmological Constant     

Anirudh Pradhan  Purnima Pandey 《Astrophysics and Space Science》2006,301(1-4):127-134

Some Bianchi type I viscous fluid cosmological models with a variable cosmological constant are investigated in which the expansion is considered only in two direction i.e. one of the Hubble parameter is zero. The viscosity coefficient of bulk viscous fluid is assumed to be a power function of mass density whereas the coefficient of shear viscosity is considered as constant in first case whereas in other case it is taken as proportional to scale of expansion in the model. The cosmological constant Λ is found to be positive and is a decreasing function of time which is supported by results from recent supernovae Ia observations. Some physical and geometric properties of the models are also discussed.  相似文献   

Higher Dimensional Cosmological Implications Of A Decay Law For λ Term: Expressions For Some Observable Quantities     

Anirudh Pradhan  G. S. Khadekar  Deepak Srivastava 《Astrophysics and Space Science》2006,305(4):415-421

Implications of cosmological model with a cosmological term of the form , where β is a constant, are analyzed in multidimensional space time. The proper distance, the luminosity distance-redshift, the angular diameter distance-redshift, and look back time-redshift for the model are presented. It has been shown that models are found to be compatible with the present observations. This work, has thus generalized to higher dimensions the well-known result in four dimensional space time. It is found that the difference is significant at least in the principal to the anologous situation in four dimensional space time.  相似文献   

On possible release of microbe-containing particulates from a Mars lander spacecraft     

Kenneth Harstad 《Planetary and Space Science》2006,54(3):273-286

Due to possible planet contamination, before Earth-departure, Mars landers and/or rovers are subject to strict requirements on the maximum number of attached spores or particles that carry viable microbes. Estimates of the release rates of these particles on Mars are made considering the three mechanisms of wind shear, collision with suspended dust, and collision with saltating sand particles. The first mechanism is found to apply only to particles of size greater than , the second mechanism has a characteristic particle adhesion half life that is so long as to be of no concern, and the third mechanism is deemed of possible importance, vitally depending on attached particle size and detailed surface characteristics of sand and spacecraft. While not investigated in detail, dust devils are shown to be possible contributors to release of microbe-containing particles.  相似文献   

DZ-1型地质灾害土层含水量监测仪系统的研究与应用          下载免费PDF全文

陈文俊  周策  汤国起 《探矿工程》2005,32(3):39-41

高强度降雨和岩土层含水量过高是山体滑坡等地质灾害的主要诱因，为了更好地对这类地质灾害进行有效预测预报，研制了DZ-1型地质灾害土层含水量监测仪，介绍了该监测仪的工作原理、主要构成、技术性能、监测工艺技术及实际应用效果。  相似文献   

大气边界层湍流能量交换特征研究进展     

李富余张宏升  陈家宜 《气象科技》2004,32(5):305-310

从一维湍流能量平衡方程出发,回顾了近几十年湍流能量平衡方程中的各项以及Karman常数k的研究成果,总结了大气边界层湍流能量交换特征的研究概况和热点问题,并对今后发展趋势做了展望。实验研究表明,湍流能量平衡方程中的各项在不同条件下有不同的形式;传统的能量产生和耗散的局地平衡假设存在不足,特别是在不稳定条件下,垂直的湍流输运和压力脉动对湍流能量收支起了非常重要的作用。Karman常数与Rossby数和Reynolds数无关,在比较光滑的下垫面上k近似等于040±001。  相似文献   

潘集煤矿二叠纪主采煤层中微量元素亲和性研究   总被引：5，自引：0，他引：5  

黄文辉  杨起  汤达祯  唐修义  赵志根 《地学前缘》2000,(Z2)

安徽淮南煤田位于华北地台南端 ,发育了华北地区二叠纪含煤岩系中层位最高的可采煤层。采用仪器中子活化分析法 (INAA)测试了淮南煤田潘集煤矿二叠纪主采煤层 13个样品的 36个微量元素的浓度分布 ,并对其共生组合特点、地球化学特征及稀土元素配比模式作了初步分析 ,结果表明 ,煤中不同微量元素显示出不同的亲和性质。元素Br,As ,Sb ,Ni和Co等趋于在煤中富集 ,其中Br的有机亲和性最大。元素Na ,K ,Rb ,Th ,Hf,Zr ,Ta和REE则在煤层与顶底板接触带的碳质泥岩中富集 ,表现出与细粒陆源碎屑物更强的亲和性。其它元素倾向性不甚明显 ,但Fe ,Ca ,Sr ,HREE等元素在海水影响强度增大的煤层中含量增加。元素As,Cs,Ni,Fe和Ca在煤层中含量变化较大 ,其变异系数大于 1,其它元素则相对稳定 ,表明同一矿区煤层中微量元素含量在不受其它地质作用明显叠加影响时具有一定的稳定性。本区煤层稀土元素配比模式与华北其它地区C—P纪煤基本类似 ,普遍存在Eu亏损现象。 ∑REE在煤中分布范围为30× 10 -6～ 95× 10 -6,在顶板泥岩中超过 2 0 0× 10 -6。煤层中部 ∑REE降低 ,HREE相对富集。聚类分析表明 ,元素As ,Se ,Ag和Fe关系密切 ,这与煤中黄铁矿等成岩矿物有直接关系 ,泥炭沼泽演化期间或之后海水的直接或间接影响会促使这  相似文献   

川北砂岩-泥岩系混合作用地球化学特征   总被引：1，自引：0，他引：1  

孙书勤  刘峰  王建华 《矿物岩石》2000,20(2):19-22

根据沉积岩混合作用判别原理,应用元素铬－钍判别法,判明川北砂岩－泥岩系为二元混合成因。再根据二元混合元素丰度关系定律,由混合变换式求出丰度关系常数,认为川北砂岩－泥岩系既具有互稀释混合作用,又具有稀释混合作用,进而可以对沉积岩端员物质组成进行估算。  相似文献   

岩石矿物组份质量转移的模糊聚类定量计算     

刘德正 《铀矿地质》2000,16(4):212-225

本文根据岩石矿物组份质量分数值的定和特性 ,提出定量计算组份质量转移的新方法。该方法运用模糊动态聚类分析技术 ,通过计算复原定和差并判定差值类型 ,辅以相应的判别参数 ,逐步从中筛选出真恒量组份 ,再利用真恒量组份定值系数 ,计算出变组岩石矿物各组份的真实质量分数值和转移量值。笔者将该方法称为真恒量组份定值法 (TCF法 )。  相似文献   

The equivalence between different Dark (matter) energy scenarios     

Arbab I. Arbab 《Astrophysics and Space Science》2004,291(2):143-149

We have shown that the phenomenological models with a cosmological constant of the type Λ=β( ) and Λ=3αH ², where R is the scale factor of the universe and H is the Hubble constant, are equivalent to a quintessence model with a scalar (φ) potential of the formV∝φ^-n, n= constant. The equation of state of the cosmic fluid is described by these parameters (α, β, n) only. The equation of state of the cosmic fluid (dark energy) can be determined by any of these parameters. The actual amount of dark energy will define the equation of state of the cosmic fluid.All of the three forms can give rise to cosmic acceleration depending the amount of dark energy in the universe.  相似文献   

Some Homogeneous Bianchi type IX Viscous Fluid Cosmological Models with a Varying Λ     

Anirudh?PradhanEmail author  Sudhir?Kumar?Srivastav  Mahesh?Kumar?Yadav 《Astrophysics and Space Science》2005,298(3):419-432

Some Bianchi type IX viscous fluid cosmological models are investigated. To get a solution, a supplementary condition between metric potentials is used. The viscosity coefficient of bulk viscous fluid is assumed to be a power function of mass density, whereas the coefficient of shear viscosity is considered as proportional to scale of expansion in the model. The cosmological constant Λ is found to be positive and is a decreasing function of time, which is supported by results from recent supernovae observations. Some physical and geometric properties of the models are also discussed.  相似文献