| 1. | Number density profile
数密度轮廓 |
| 2. | Thermodynamical fluctuation of number density of particles in grand canonical ensemble of perfect systems
理想体系巨正则系综中粒子数密度的热力学涨落 |
| 3. | With the cell cycle model , the cell cycle related variables , such as fraction of budding cells ( fbc ) and cell number density , can be simulated
通过细胞循环模型，求得与细胞循环过程相关的变量，如细胞带芽分率和细胞数目浓度。 |
| 4. | The macro - mechanical properties ( the elastic constants ) of the fractured rocks can be connected with the micro - parameter of crack ( crack number density )
这个模型将微观随机参数(裂纹数密度)与非均匀裂缝介质的宏观性质(弹性常数)直接联系起来。 |
| 5. | The distribution of the void number density has been numerically investigated under the condition of the same ratio of inner and outer diameters for all voids
假设所有孔洞的内外半径之比相同，用数值方法定性分析了材料在层裂损伤过程中孔洞数密度分布的变化。 |
| 6. | For the low pr hadrons , the bayon number density is very low and shows the evidence of early stage equilibrium . there exists elliptic flow character for the high pt hadrons
对于低竹强于，在h 0处呈现较低的重子数密度，有早期平衡的明显证据；对于高ptjffi子，有椭性流的特点。 |
| 7. | In high energy neutrino - emulsion collisions , the normalized distribution of two - particle relative pseudorapidity and the correlation between the mean maximum number density of shower particles and multiplicity are investigated
摘要论述了高能中微子与核乳胶碰撞中，归一化的两粒子相对鹰快度分布，和平均最大簇射粒子数密度与多重数的关联。 |
| 8. | Influences of initial damage on development of spalling damage have been indicated by analyzing the distribution of void number density , the cumulative percentage of void volume and the volume fraction of the different - seize voids
通过分析孔洞数密度分布、孔洞体积累积百分比、不同大小孔洞所占体积份额的计算结果，指出初始损伤对损伤演化有直接影响。 |
| 9. | The chemical reactions in the flame area are very complex . it is very difficult to measure the number density distribution of the particles ( atoms , ions and molecules ) , so the relative intensity method is employed
由于固体推进剂燃烧区内发生的化学反应非常复杂,直接测量火焰区内的粒子(原子、离子以及分子等)数密度比较困难,因此选用相对强度法来进行计算。 |
| 10. | Our results show that with the up to date experimental data , 13c can not sufficiently burn , the neutron number density decrease , the timescale of neutron source become long and these come into conflict with model of thermal pulse agb star
研究结果表明，在新实验结果下， ’ 3c不能充分燃烧，中子数密度降低，中子源持续的时标变长，这与热脉冲agb星的现有模型出现矛盾。 |
