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势模型的英文

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"势模型"怎么读用"势模型"造句

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  • potential model

例句与用法

  • Theoretical study of the interaction potential model for he - hf system
    碰撞体系相互作用势模型的理论研究
  • Vibrating potential model
    振动势模型
  • Describing antiproton - nuclear scattering by using each annihilation potential is feasible
    各湮没势模型都能较好地描写反质子-核散射过程。
  • Parameter correction and application of embedded - atom method potential in investigation of copper clusters
    铜团簇嵌入原子势模型的参数修正及应用
  • Through the experimental work of this thesis , the single - particle potential model is comprehended and some improvements are made
    通过论文的实验工作,我们深入了解并改进了单粒子势模型
  • Besides , considering the differences of the galactic gravitational potential models , there is different influence for the distribution morphologies of all of the orbital parameters of the selected sample clusters
    此外,不同的银河系引力势模型对所选样本的轨道参数的分布形态也有不同程度的影响。
  • Secondly , we use the two - dimensional equivalent potential model to turn the excitons in quantum well into the effective two - dimensional excitons , and calculate the parameters ax and yx versus the quantum well width
    然后,我们用二维等效势模型,把阱中激子等效为二维激子,计算得到了参数_ x和_ x随阱宽的变化。
  • Furthermore , according to the results of the single - particle potential model , the more natural necessary condition for the formation of the halo structure is given with the woods - saxon potential . this condition is more loser than the current one
    此外,根据单粒子势模型计算结果,给出了更合理的woods - saxon势下晕结构形成的必要条件,比目前所知的条件宽松。
  • In chapter three , the present equations of state ( eoss ) used constantly by many investigators are classified and elucidated by virtue of theory foundations , phenomenological potential models , experimental bases , and the applied conditions of eoss
    论文第三章对现有的实用性较为广泛的固体物态方程按照其提出的理论依据、唯象势模型、实验基础、及应用的范围或条件进行了归类、说明、总结与讨论。
  • The differences in orbital morphologies due to different potentials is slighting , however , given a certain potential , for clusters that have perigalactic distance smaller than 1 kpc , some orbits may exhibit a chaotic behavior . the correlation between the metallicity of samples and the orbital morphologies is unclearly ; ( 4 ) it is found that the semi - major axis , apogalactic distance and azimuth period of 29 sample clusters are changed with their metallicity similarly , but a obvious correlation is seen between orbital eccentricity and metallicity . there is a fraction of 24 % of the sample clusters with eccentricities lower than 0 . 4
    不同的引力势模型对球状星团轨道的具体形态影响不大,在给定的引力势模型下,当某些星团的运动轨道穿越距银心1kpc附近的区域时会出现“混沌”现象: ( 4 ) 29个样本星团的轨道半长轴、远银心距和方位周期随金属度的变化规律基本相似,样本星团的金属度与其轨道形态之间的相关性并不明显,然而轨道偏心率与金属度有关,对于所选的晕族样本星团而言,大约有24的样本星团的轨道偏心率低于0 . 4 。
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