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Bose-Einstein Condensates in a One-Dimensional Optical Lattice: from Superfluidity to Number-Squeezed States
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We study the phase coherence property of Bose-Einstein condensates confined in a one-dimensional optical lattice formed by a standing-wave laser field. The lattice depth is determined using a method of Kapitza-Dirac scattering between a condensate and a short pulse lattice potential. Condensates are then adiabatically loaded into the optical lattice. The phase coherence property of the confined condensates is reflected by the interference patterns of the expanded atomic cloud released from the optical lattice. For weak lattice, nearly all of the atoms stay in a superfluid state. However, as the lattice depth is increased, the phase coherence of the whole condensate sample is gradually lost, which confirms that the sub-condensates in each lattice well have evolved into number-squeezed states. 相似文献
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Using the high precision data of the proper motions and parallaxes from Hipparcos catalogue, we obtained the orbital parameters of 1302 stars in the Galaxy based on the mass distribution model provided by Allen and Santillón. Fe abundances of 1295 stars among our samples were analyzed. With the correlation analyses between [Fe/H] and orbital parameters, we obtained that the Fe gradient is - 0.057 ± 0.007 dex/kpc along the direction of the maximum galactocentric distance (hereafter DGmax) in the range of 8.5 kpc < DGmax < 17 kpc. We also got the result that the vertical gradient is steeper than the radial gradient. Furthermore, we divided the samples into two subgroups: giants and dwarfs; F, G and K stars; and then analyzed them respectively. Our results show that the gradient becomes flatter and flatter from giants to dwarfs, from F type to G and K type stars. We also divided the samples into disk and halo stars using maximum vertical distance Zmax = 1 kpc as the criterion and got the result that the abundances of the disk stars are much higher than that of the halo stars. Our work suggests the existence of the galactic gradient and supports those chemlcal evolution medels which show that the halo was formed before the disk at the early stage of the Galaxy. 相似文献
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结合新高中教材(山东科技版)《化学与生活(选修)》和《有机化学基础(选修)》2个模块教材中有关垃圾的妥善处理与利用、污水治理与环境保护、塑料部分内容,设计了一段阅读材料:污水治理与白色污染治理新技术——超临界水技术,并较全面地为教师介绍了超临界水、超临界水技术的相关知识,同时为将超临界水技术用于废塑料处理内容引入课堂教学提出了活动建议,供使用这2个模块教材的教师在教学中选用。 相似文献
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在积累知识的过程中,除如何猎取知识外,还有一个如何储存知识的问题.深刻的理解加上合理的储存,就能运用自如地掌握知识,而靠死记硬背储存知识,遇到灵活性强、比较隐蔽的问题就束手无策了.合理的知识结构应当具有以下特征:一、系统性.处于游离状态的知识,完全失去了其应有价值,成了大脑的负担;而系统化的知识,各个知识点前后呼应,表现出1+1>2的价值,减少了记忆量和记忆难度.因此,学习中不仅要善于获得知识,更要善于整理自己的知识系统. 相似文献
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为了快捷、精准测量脆性易解理氧化镓晶体的断裂韧度,为氧化镓精密加工提供理论依据.采用G200纳米压痕仪对氧化镓晶体进行纳米压痕试验,通过扫描电子显微镜分析压痕形貌,分别采用纳米压痕法、能量法两种方法计算断裂韧度.纳米压痕法测得(010)面氧化镓晶体的断裂韧度为0.769 MPa·m1/2;能量法测得其断裂韧度为0.782 MPa·m1/2.与传统的断裂韧度检测方法相比,基于纳米压痕仪的压痕法和能量法能够微损伤快速检测脆性材料的断裂韧度.能量法是更精准、更便捷的纳米级断裂韧度检测方法. 相似文献
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三次采油耐温抗盐聚合物的合成与评价 总被引:1,自引:0,他引:1
以丙烯酰胺(AM)、2-丙烯酰胺基-2-甲基丙磺酸(AMPS)和氢氧化钠(Na OH)为原料,采用过硫酸铵[(NH4)2S2O8]、亚硫酸钠(Na2SO3)和四甲基脲[N(CH3)2CON(CH3)2]作为新型复合引发体系,通过共聚后水解工艺,合成了高分子量三元共聚物(AM-AANa-AMPSNa).考察了引发剂用量、单体浓度、p H和引发温度对共聚物黏均分子量的影响.确定最优条件为:引发剂用量0.035%,单体质量浓度为25%,介质p H 7,引发温度0℃.通过红外光谱和核磁碳谱表征了其结构,并系统评价了其理化性能指标、黏弹性、注入性和驱油性能.结果表明,该共聚物较高分子量部分水解聚丙烯酰胺(HPAM)具有更优异的耐温抗盐性能.其黏均相对分子量达到3000万以上,在胜利油田III型盐水中,浓度1500 mg/L,温度85℃条件下,溶液表观黏度达到17.7 m Pa s,岩心驱油实验在水驱采收率51.8%基础上,可再提高15.8%.上述性能表明,该高分子量三元共聚物有望应用在高温高盐油藏三次采油技术中. 相似文献