The model of a flat (Euclidean) expansive homogeneous and isotropic relativistic universe in the light of the general relativity,quantum mechanics,and observations

Assuming that the relativistic universe is homogeneous and isotropic, we can unambiguously determine its model and physical properties, which correspond with the Einstein general theory of relativity (and with its two special partial solutions: Einstein special theory of relativity and Newton gravitation theory), quantum mechanics, and observations, too.     

海水中碳酸根与固体粒子的相互作用

本文研究了海水中碳酸根在固体粒子上的吸附。碳酸根在各种因素颗粒物上的吸附程度上大小顺序为：赤铁矿〉δ－ＭｎＯ２〉水锰矿〉ＳｉＯ２,最大吸附量可达到约２ｍｇＣ／ｇ吸附剂,且最大吸附值均在天然海水ｐＨ（ｐＨ８）左右。在低ＰＨ时,碳酸根对ＮａＣｌ介质中砷酸根的吸附没有影响,在高ｐＨ时,则降低了砷酸根在固体颗粒物上的吸附量,因此碳酸根的存在对其他阴离子的吸附会产生竞争作用。     

Numerical sea ice prediction in China

ＮｕｍｅｒｉｃａｌｓｅａｉｃｅｐｒｅｄｉｃｔｉｏｎｉｎＣｈｉｎａＷｕＨｕｉｄｉｎｇ,ＢａｉＳｈａｎ,ＺｈａｎｇＺｈａｎｈａｉ１（ＲｅｃｅｉｖｅｄＳｅｐｔｅｍｂｅｒ１２,１９９６;ａｃｃｅｐｔｅｄＪｕｎｅ５,１９９７）Ａｂｓｔｒａｃｔ──Ａｄｙｎａｍｉ...     

回声测深仪在水下地形测量中的应用

本文在介绍回声测深仪基本工作原理的同时,介绍了回声测深仪在杭州湾口外一拟建大型码头下地形测量的一个应用实例。     

强震水化学前兆场特征

研究了唐山、松潘两次７级以上强震的水化学前兆场特征。结果表明，两次强震水化学前兆场有相似的特征。在震源区，水化趋势性异常和短临突变异常所占的比例大，远离震源区所占的比例小，且有逐渐减小的趋势；在震源区，水化趋势性异常起始的时间早，远离震源区异常起始的时间晚，趋势异常的形态均为逐渐升高。水化学前兆场的形成与区域应力场有关，但与震源应力场关系密切，可能起主导作用的是震源应力场。     

鄂尔多斯及其周缘地热分布的某些特征

利用鄂尔多斯及其周缘的大地热流、地温梯度和地温分布等资料研究了其展布特征和差异性变化，并讨论了地热分布与地壳深浅构造的关系。认为，鄂尔多斯块体内大地热流、地温梯度值整体偏低，而其周缘地区则呈现出环状高值异常带。该区地震活动主要集中分布在鄂尔多斯周缘地区，即鄂尔多斯周缘存在着高热流、高地温梯度和地震丛集分布相统一的现象。这一现象说明，地热和地震活动之间存在着某种必然的联系。     

The idea and project of the “Medium-Scale Experiment Field for Earthquake Prediction”

A brief account of the development of the research on mining earthquakes and the general situation of the Mentougou Coal Mine medium-scale experiment field for earthquake prediction and the project of monitor and prediction is given. The differences of waveforms between mining earthquakes and natural earthquakes is discussed. The magnitude-frequency distribution of the 79 000 mining earthquakes of overM _l 1. 0 from 1984 to 1995 is summarized. Finally, taking PH and PV, the principal compressive stress components of the focal mechanism of the mining earthquakes, as the criteria, analyses the stress background of the 12 large mining earthquakes.     

All-sky ultraviolet surveys: the needs and the means

This is a crucial time in the history of astronomy with major all-sky surveying work being carried out in all spectral bands, as well as in astrometry. The results of this activity are advancing all fields of astrophysical research, from the investigation of exo-planetary systems to the study of the chemical evolution of the Universe. Full sky surveys are available from the radio domain to X-ray wavelengths but not in the ultraviolet range (UV). While large UV missions are currently under discussion within the astrophysical community and at the major Space Agencies, the efficient use of resources requires preparatory work that can fill the UV surveying gap. This article summarizes the research and on-going activities in this field.     

Exact solution of anisotropic compact stars via mass function

Studying relativistic compact objects is important in modern astrophysics to understand several astrophysical issues. It is therefore natural to ask for an internal structure and physical properties of specific classes of compact stars from astrophysical observations. We obtain a class of new relativistic solutions with anisotropic distribution of matter for compact stars. More specifically, stellar models, described by an anisotropic fluid, establishing a relation between metric potentials and generating a specific form of mass function, are explicitly constructed within the framework of General Relativity. New solutions can be used to model compact objects, which adequately describe compact strange star candidates like SMC X-1, Her X-1 and 4U 1538-52, with observational data taken from Gangopadhyay et al. (Mon. Not. R. Astron. Soc. 431:3216, 2013). As a possible astrophysical application the obtained solutions could explain the physics of selfgravitating objects, and might be useful for strong-field regimes where data are currently inadequate.     

Study of some chaotic inflationary models in $$ gravity

In this paper, we discuss an inflationary scenario via scalar field and fluid cosmology for an anisotropic homogeneous universe model in \(f(R)\) gravity. We consider an equation of state which corresponds to a quasi-de Sitter expansion and investigate the effect of the anisotropy parameter for different values of the deviation parameter. We evaluate potential models like linear, quadratic and quartic models which correspond to chaotic inflation. We construct the observational parameters for a power-law model of \(f(R)\) gravity and construct the graphical analysis of tensor–scalar ratio and spectral index which indicates the consistency of these parameters with Planck 2015 data.