浑沌：它能有多少规律

40年前A.爱因斯坦给M.玻恩的一封信中写道,“上帝不玩骰子。”爱因斯坦是始终反对量子论的概率解释的,他不倦地探索着与经典力学更为直接的类比,即考虑没有概率不定性的确定过程。如今,40年过去了,没有人会惊讶:甚至在一个经典哈密顿动力系统中也存在着(chas)在物理客体规则运动的领域内,在没有人预期会有的地方冒出     

二甲基甲酰胺中Sm（Ⅲ）电化学性质及其合金膜研究

通过循环伏安法研究二甲基甲酰胺中Sm（Ⅲ）在Pt上的电化学性质,表明Sm（Ⅲ）在Pt上的还原为不可逆反应,同时测得传递系数α=0.0289,扩散系数D0=1.288×10^-5cm^2·S^-1;通过塔菲尔曲线求得交换电流密度i0=1.596×10^-7A/cm^2;对Sm（Ⅲ）在Pt上离子成核机理研究表明,Sm（Ⅲ）在Pt电极上是按三维模式扩散控制下连续成核的;用恒电位法可以制得有金属光泽、附着力好、表面均匀致密的Sm-Ni-Co合金膜,与Ni-Co合金膜相比较结构性能有所提高.     

Submillimetre galaxies reside in dark matter haloes with masses greater than 3 × 10(11) solar masses

The extragalactic background light at far-infrared wavelengths comes from optically faint, dusty, star-forming galaxies in the Universe with star formation rates of a few hundred solar masses per year. These faint, submillimetre galaxies are challenging to study individually because of the relatively poor spatial resolution of far-infrared telescopes. Instead, their average properties can be studied using statistics such as the angular power spectrum of the background intensity variations. A previous attempt at measuring this power spectrum resulted in the suggestion that the clustering amplitude is below the level computed with a simple ansatz based on a halo model. Here we report excess clustering over the linear prediction at arcminute angular scales in the power spectrum of brightness fluctuations at 250, 350 and 500?μm. From this excess, we find that submillimetre galaxies are located in dark matter haloes with a minimum mass, M(min), such that log(10)[M(min)/M(⊙)] = 11.5(+0.7)(-0.2) at 350?μm, where M(⊙) is the solar mass. This minimum dark matter halo mass corresponds to the most efficient mass scale for star formation in the Universe, and is lower than that predicted by semi-analytical models for galaxy formation.     

Nickel solvent extraction from cold purification filter cakes of Angouran mine concentrate using LIX984N

Cold purification filter cakes generated in the hydrometallurgical processing of Angouran mine zinc concentrate commonly contain significant amounts of Zn, Cd, and Ni ions and thus are valuable resources for metal recovery. In this research, a nickel containing solution that was obtained from sulfuric acid leaching of the filter cake following cadmium and zinc removal was subjected to solvent extraction experiments using 10vol% LIX984N diluted in kerosene. Under optimum experimental conditions (pH 5.3, volume ratio of organic/aqueous (O:A) = 2:1, and contact time = 5 min), more than 97.1% of nickel was extracted. Nickel was stripped from the loaded organic by contacting with a 200 g/L sulfuric acid solution, from which 77.7% of nickel was recovered in a single contact at the optimum conditions (pH 1–1.5, O:A = 5:1, and contact time = 15 min).