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31.
李志阐 《数学物理学报(B辑英文版)》1987,(1)
In this paper, by using the probabilistic method, we obtained a decomposition theorem for the harmonic functions, generalized and strengthened some theorems: Doob's theorem on the limit behaviors of the superharmonic functions, Bocher's theorem on the representation of the harmonic functions and the extension theorem of the harmonic functions etc. 相似文献
32.
We consider rotational motion of an interacting atomic
Bose-Einstein condensate (BEC) with both two- and three-body
interactions in a quadratic-plus-quartic and harmonic-plus-Gaussian
trap. By using the variational method, the influence of the
three-body interaction and the anharmonicity of the trap on the
lowest energy surface mode excitation and the spontaneous shape
deformation (responsible for the vortex formation) in a rotating BEC
is discussed in detail. It is found that the repulsive three-body
interaction helps the formation of the vortex and reduces the lowest
energy surface mode frequency and the critical rotational frequency
of the system. Moreover, the critical rotational frequency for the
vortex formation in the harmonic-plus-Gaussian potential is lower
than that in the quadratic-plus-quartic potential. 相似文献
33.
34.
铁电纳米材料BaTiO_3具有尺寸均匀,形貌统一的单晶纳米立方体结构。以LRS-Ⅲ型激光拉曼/荧光光谱仪为测量仪器研究其在固体纳米材料BaTiO_3分析中的应用。用碱热法制作得到4种无掺杂铁电纳米材料BaTiO_3,分别标记为纯1、纯2、纯3、纯4,将四种固体纳米材料作为标样待测;另取两个不同浓度Eu(铕)元素掺杂的材料分别标记为掺杂1、掺杂2待测。本实验中,不仅对比分析了不同烧结温度和时间下的固体纳米材料BaTiO_3激光拉曼光谱,并做出了相应的解释说明。与此同时,对掺杂BaTiO_3的也做了拉曼光谱对比分析,研究掺杂对固体材料拉曼谱线的影响。研究结果表明,含有相同成分的固体材料其拉曼谱线相似,且不同掺杂引起拉曼谱线的变化不同。最后用相关系数对掺杂材料和无掺杂材料做了进一步分析。从总体来看类内相关系数较高而类间相关系数较低,但即便掺杂的量比较少,对相关系数也有明显的影响。结合相关系数可以明确地判断出两种物质是否同类,如果已知某一种没有掺杂,那么,就可以很容易地判断出另一种材料中是否有掺杂。 相似文献
35.
The effect of tidal torques on rotational mixing in close binaries is investigated. It is found that spin angular momentum can attain a high value due to a strong tidal torque. Nitrogen and helium enrichment occurs early in the binary system that is triggered by tides. The stellar radius can reach a high value in the single star model with high initial velocities at the early stage of the evolution, but efficient rotational mixing can inhibit stellar expanding at the subsequent evolution. Central compactness is increased by the centrifugal force at the early stage of evolution but is reduced by rotational mixing induced by strong tides. The binary models with weak tides have high values of central temperature and stellar radius. Rotational mixing in single stars can slow down the shrinkage of convective cores, while convective cores can be expanded by strong tides in the binary system.Efficient rotational mixing induced by tides can cause the star to evolve towards high temperature and luminosity. 相似文献
36.
张文号 孙袆 张金松 李坊森 郭明华 赵弇斐 张慧敏 彭俊平 邢颖 王慧超 FUJITA Takeshi HIRATA Akihiko 李志 丁浩 汤辰佳 王萌 王庆艳 何珂 季帅华 陈曦 王俊峰 夏正才 李亮 王亚愚 王健 王立莉 陈明伟 薛其坤 马旭村 《中国物理快报》2014,(1):156-160
We prepared one-unit-ceil (1-UC) thick FeSe films on insulating SrTiOa substrates with non-superconducting FeTe protection layers by molecular beam epitaxy for ex situ studies. By direct transport and magnetic measurements, we provide definitive evidence for high temperature superconductivity in the 1-UC FeSe films with an onset Tc above 40 K and an extremely large critical current density fie Jc-1.7× 106 A/cm2 at 2K, which are much higher than Tc-8K and Jc-104 A/cm^2 for bulk FeSe, respectively. Our work may pave the way to enhancing and tailoring superconductivity by interface engineering. 相似文献
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